Refine
Has Fulltext
- no (4728) (remove)
Year of publication
Document Type
- Article (4100)
- Doctoral Thesis (376)
- Monograph/Edited Volume (117)
- Other (83)
- Review (35)
- Preprint (9)
- Conference Proceeding (4)
- Habilitation Thesis (3)
- Postprint (1)
Is part of the Bibliography
- yes (4728)
Keywords
- stars: massive (56)
- gamma rays: general (46)
- stars: early-type (45)
- stars: winds, outflows (42)
- diffusion (39)
- Magellanic Clouds (38)
- cosmic rays (38)
- radiation mechanisms: non-thermal (38)
- X-rays: stars (37)
- ISM: supernova remnants (36)
- anomalous diffusion (35)
- X-rays: binaries (33)
- acceleration of particles (33)
- gamma rays: galaxies (33)
- quasars: absorption lines (33)
- stars: atmospheres (33)
- stars: mass-loss (33)
- intergalactic medium (31)
- stars: evolution (31)
- stars: Wolf-Rayet (30)
- methods: numerical (29)
- galaxies: active (28)
- stars: magnetic field (24)
- subdwarfs (22)
- techniques: spectroscopic (22)
- astroparticle physics (21)
- binaries: close (21)
- galaxies: formation (20)
- turbulence (19)
- instabilities (18)
- organic solar cells (18)
- stars: abundances (18)
- stars: fundamental parameters (17)
- Galaxy: halo (16)
- binaries: general (16)
- galaxies: evolution (16)
- galaxies: jets (16)
- magnetic fields (15)
- Sun: corona (14)
- Sun: coronal mass ejections (CMEs) (14)
- Sun: flares (14)
- Sun: magnetic fields (14)
- magnetohydrodynamics (MHD) (14)
- stars: neutron (14)
- white dwarfs (14)
- BL Lacertae objects: general (13)
- hydrodynamics (13)
- methods: data analysis (13)
- relativistic processes (13)
- shock waves (13)
- stochastic processes (13)
- surveys (13)
- Sun: activity (12)
- galaxies: ISM (12)
- methods: observational (12)
- perovskite solar cells (12)
- stars: variables: general (12)
- Galaxy: evolution (11)
- ISM: abundances (11)
- ISM: clouds (11)
- MHD (11)
- binaries: spectroscopic (11)
- climate change (11)
- gamma rays: stars (11)
- Sun: photosphere (10)
- galaxies: high-redshift (10)
- gamma rays: ISM (10)
- gamma-ray burst: general (10)
- plasmas (10)
- stars: winds (10)
- techniques: imaging spectroscopy (10)
- techniques: photometric (10)
- ISM: structure (9)
- Sun: chromosphere (9)
- dark ages, reionization, first stars (9)
- dark matter (9)
- galaxies: interactions (9)
- stars: AGB and post-AGB (9)
- stars: kinematics and dynamics (9)
- synchronization (9)
- Sun: filaments, prominences (8)
- X-ray refraction (8)
- azobenzene (8)
- cosmology: observations (8)
- galaxies: dwarf (8)
- galaxies: starburst (8)
- gamma-rays: galaxies (8)
- outflows (8)
- quasars: general (8)
- stars: activity (8)
- stars: emission-line, Be (8)
- stars: rotation (8)
- techniques: polarimetric (8)
- waves (8)
- Hertzsprung-Russell and C-M diagrams (7)
- Kuramoto model (7)
- binaries: eclipsing (7)
- catalogs (7)
- circumstellar matter (7)
- galaxies: abundances (7)
- organic photovoltaics (7)
- photochemistry (7)
- planets and satellites: rings (7)
- radiation belts (7)
- radiative transfer (7)
- solar wind (7)
- sunspots (7)
- H II regions (6)
- ISM: kinematics and dynamics (6)
- Local Group (6)
- X-rays: ISM (6)
- additive manufacturing (6)
- charge transport (6)
- diffuse radiation (6)
- dust, extinction (6)
- dynamics (6)
- infrared: stars (6)
- magnetosphere (6)
- model (6)
- morphology (6)
- planetary nebulae: general (6)
- pulsars: general (6)
- residual stress (6)
- stars (6)
- stars: horizontal-branch (6)
- stars: late-type (6)
- techniques: image processing (6)
- Brownian motion (5)
- Galaxy: center (5)
- ISM: jets and outflows (5)
- ISM: lines and bands (5)
- ISM: magnetic fields (5)
- RIXS (5)
- Residual stress (5)
- Resonant inelastic X-ray scattering (5)
- Synchronization (5)
- Ti-6Al-4V (5)
- ageing (5)
- analysis (5)
- chemotaxis (5)
- comets: general (5)
- cosmology: theory (5)
- electrons (5)
- elementary particles (5)
- first passage (5)
- first passage time (5)
- fractional Brownian motion (5)
- galaxies: haloes (5)
- galaxies: halos (5)
- galaxies: nuclei (5)
- gamma-rays: general (5)
- geometric Brownian motion (5)
- gravitational waves (5)
- methods: analytical (5)
- nanoparticles (5)
- neutron diffraction (5)
- photoluminescence (5)
- planet-star interactions (5)
- polarization (5)
- polymers (5)
- scattering (5)
- solar cells (5)
- stars: chemically peculiar (5)
- stars: formation (5)
- supergiants (5)
- supernovae: general (5)
- ultraviolet: ISM (5)
- Coupled oscillators (4)
- Electrets (4)
- Enceladus (4)
- Galaxy: structure (4)
- ISM: molecules (4)
- Levy flights (4)
- Organic solar cells (4)
- Planetary rings (4)
- Radiation belts (4)
- Solar cells (4)
- Spectroscopy (4)
- Van Allen Probes (4)
- X-ray emission spectroscopy (4)
- X-ray spectroscopy (4)
- accretion, accretion disks (4)
- activity (4)
- chaos (4)
- charge generation (4)
- climate impacts (4)
- conjugated polymers (4)
- convection (4)
- creep (4)
- density (4)
- errata, addenda (4)
- first-passage time (4)
- galaxies: fundamental parameters (4)
- galaxies: star formation (4)
- globular clusters: general (4)
- history and philosophy of astronomy (4)
- hysteresis (4)
- large-scale structure of Universe (4)
- line: identification (4)
- neutrinos (4)
- noise (4)
- non-fullerene acceptors (4)
- nonergodicity (4)
- photoelectron spectroscopy (4)
- piezoelectricity (4)
- planets and satellites: atmospheres (4)
- recombination (4)
- stars: black holes (4)
- stars: low-mass (4)
- stars: magnetic fields (4)
- stochastic resetting (4)
- voltage losses (4)
- ARPES (3)
- Aluminum alloys (3)
- Anomalous diffusion (3)
- Atlantic meridional overturning circulation (3)
- BL Lacertae objects: individual: Mrk 421 (3)
- BL Lacertae objects: individual: PKS 2155-304 (3)
- Cosmic rays (3)
- Curie transition (3)
- DNA (3)
- Dictyostelium (3)
- Dictyostelium discoideum (3)
- Diffusion (3)
- EMIC (3)
- Electrophoretic deposition (3)
- Ferroelectrets (3)
- Fokker-Planck equation (3)
- Genetic programming (3)
- ISM: bubbles (3)
- Langevin equation (3)
- Levy walk (3)
- Lyapunov exponent (3)
- Mittag-Leffler functions (3)
- Neutron diffraction (3)
- P(VDF-TrFE-CFE) terpolymer (3)
- STM (3)
- Saturn, Rings (3)
- Statistical and Nonlinear Physics (3)
- Sun (3)
- Sun: atmosphere (3)
- Sun: filaments (3)
- Transformation toughening (3)
- X-ray (3)
- X-ray absorption spectroscopy (3)
- X-ray imaging (3)
- X-rays (3)
- astrophysical plasmas (3)
- black hole physics (3)
- carbon nitride (3)
- catalogues (3)
- catalysis (3)
- charge transfer (3)
- charge-transfer (3)
- chemical modification (3)
- comets: individual: 67P/Churyumov-Gerasimenko (3)
- computed tomography (3)
- conductivity (3)
- confinement (3)
- control (3)
- damage (3)
- dark ages (3)
- dark matter theory (3)
- data analysis (3)
- dielectric relaxation spectroscopy (3)
- doping (3)
- dust (3)
- electrostatic interactions (3)
- electrostatics (3)
- entanglement (3)
- ferroelectret (3)
- films (3)
- first-passage (3)
- galaxies: individual: LMC (3)
- global jets (3)
- globular clusters: individual: NGC 6397 (3)
- group field theory (3)
- helical magnetic fields (3)
- individual (3)
- infrared: diffuse background (3)
- interactions (3)
- line: profiles (3)
- magnetic reconnection (3)
- methods: statistical (3)
- microscopy (3)
- mobility (3)
- networks (3)
- nonlinear dynamics (3)
- open-circuit voltage (3)
- organic semiconductors (3)
- oscillations (3)
- particle-in-cell simulations (3)
- pattern formation (3)
- phase separation (3)
- photocurrent generation (3)
- photovoltaic devices (3)
- piezoelectret (3)
- piezoelectrets (3)
- planets and satellites: individual (Saturn) (3)
- polymer solar cells (3)
- porosity (3)
- processing (3)
- quantum friction (3)
- quantum thermodynamics (3)
- radio continuum: stars (3)
- random walks (3)
- reionization (3)
- relativistic jets (3)
- scaled Brownian motion (3)
- sea-level rise (3)
- spectra (3)
- spectroscopy (3)
- stars: (3)
- stars: coronae (3)
- stars: distances (3)
- stars: mass loss (3)
- stars: oscillations (3)
- stars: pre-main sequence (3)
- starspots (3)
- statistical physics (3)
- stochastic models (3)
- stochastic processes (theory) (3)
- subdiffusion (3)
- superstatistics (3)
- surface (3)
- surface relief grating (3)
- surface treatment (3)
- synchrotron X-ray diffraction (3)
- synthesis (3)
- temperature (3)
- transport (3)
- vulnerability (3)
- 2D perovskites (2)
- 4 (2)
- AFM (2)
- Active regions, magnetic fields (2)
- Additive manufacturing (2)
- Atmosphere (2)
- Azobenzene containing cationic surfactants (2)
- BL Lacertae objects: individual (Mrk 501) (2)
- BL Lacertae objects: individual: Mrk 501 (2)
- Bayesian inference (2)
- Blocking (2)
- Boltzmann distribution (2)
- Bose-Einstein condensate (2)
- Bose-Einstein condensation (2)
- Capacitive sensor (2)
- Cassini (2)
- Cations (2)
- Ceramics (2)
- Collisional physics (2)
- Comb model (2)
- Comets (2)
- Complex networks (2)
- Computed tomography (2)
- Convolutional neural networks (2)
- Corona, active (2)
- Cosmology (2)
- Crack deflection (2)
- Crystallization (2)
- DFT (2)
- Dark matter (2)
- Debye screening (2)
- Deep learning (2)
- Dielectric materials (2)
- Doping (2)
- Dust (2)
- Dynamical systems (2)
- Electron spectroscopy (2)
- Embedding (2)
- Equilibrium-line altitudes (2)
- FLASH (2)
- Fox H-function (2)
- Fractional moments (2)
- Galaxy: formation (2)
- Galaxy: kinematics and dynamics (2)
- Galaxy: stellar content (2)
- Gamma-ray astronomy (2)
- Gas phase (2)
- Gaussian processes (2)
- Gold (2)
- Granulation (2)
- Greenland (2)
- HII regions (2)
- Hertzsprung-Russell and colour-magnitude diagrams (2)
- Hilbert transform (2)
- Holocene (2)
- Hydraulic models (2)
- Hydraulic networks (2)
- Hydrodynamics (2)
- Hydrogel (2)
- Hysteresis (2)
- IACT (2)
- ISM (2)
- ISM: individual objects: G338.3-0.0 (2)
- Instrumentation (2)
- Instrumentation and data management (2)
- Interstellar medium (2)
- Irradiation (2)
- Klimawandel (2)
- Kuramoto (2)
- LDPE nanocomposites (2)
- Laboratory astrophysics (2)
- Laser powder bed fusion (2)
- Lasers (2)
- Levy walks (2)
- MU-M (2)
- Magnetic field, photosphere, corona (2)
- Magnetic fields, corona (2)
- Mars (2)
- Maximum entropy method (2)
- Missions (2)
- Molecular dynamics (2)
- Molecules (2)
- Multilayer (2)
- NAP-XPS (2)
- Network reconstruction (2)
- Nitrogen (2)
- Nonlinear coupling (2)
- Organic electronics (2)
- Organic semiconductors (2)
- Oscillator ensembles (2)
- Outflows (2)
- PCPDTBT (2)
- Perovskites (2)
- Phase transitions (2)
- Photoelectron spectroscopy (2)
- Physics (2)
- Pipe networks (2)
- Plume (2)
- Probability (2)
- Professional Knowledge (2)
- Prominences, active (2)
- Pump-probe (2)
- Radiative transfer (2)
- Raman imaging (2)
- Raman spectroscopy (2)
- Residual stresses (2)
- Resonances (2)
- Rings (2)
- Saturn (2)
- Scher-Montroll transport (2)
- Semiconductors (2)
- Shocks (2)
- Sinai diffusion (2)
- Stability (2)
- Structural health monitoring (2)
- Sun: UV radiation (2)
- Sun: heliosphere (2)
- Sun: magnetic topology (2)
- Sun: sunspots (2)
- Supernova remnants (2)
- Surface science (2)
- Surface treatment (2)
- Synchronization control (2)
- TIG-welding (2)
- Thin films (2)
- UV-vis spectroscopy (2)
- Unterrichtsplanung (2)
- VERB (2)
- VERB code (2)
- Viscoelasticity (2)
- Water distribution systems (2)
- X-ray computed tomography (CT) (2)
- X-ray photoelectron spectroscopy (2)
- XAS (2)
- XES (2)
- XPS (2)
- Yttria stabilized zirconia (2)
- acceleration (2)
- accretion (2)
- accretion discs (2)
- active transport (2)
- aggregation (2)
- aspect ratio (2)
- astronomical databases (2)
- astronomy (2)
- azobenzene containing surfactants (2)
- behavior (2)
- bidirectional reflectance (2)
- biological physics (2)
- biological transport (2)
- biophysics (2)
- blue stragglers (2)
- bulk heterojunction (2)
- bulk heterojunctions (2)
- bumps (2)
- capacitive sensor (2)
- celestial mechanics (2)
- cell migration (2)
- charge-carrier transport (2)
- charge-transfer states (2)
- chimera state (2)
- chorus waves (2)
- climate (2)
- collective dynamics (2)
- collective motion (2)
- complementarity (2)
- complex systems (2)
- connections between chaos and statistical physics (2)
- conservation laws (2)
- continuous time random walk (2)
- continuous time random walk (CTRW) (2)
- core-shell nanostructure (2)
- corona (2)
- coronal mass ejections (CMEs) (2)
- correlations (2)
- cosmic background radiation (2)
- coupled oscillators (2)
- coupled rotators (2)
- critical avalanche dynamics (2)
- critical phenomena (2)
- crowded fluids (2)
- cylindrical geometry (2)
- data (2)
- dielectric barrier discharge (DBD) (2)
- dielectric barrier discharges (2)
- dielectric properties (2)
- diffraction (2)
- diffusing diffusivity (2)
- distance scale (2)
- driving force (2)
- dwarfs galaxies (2)
- dynamic loading (2)
- early Universe (2)
- electrets (2)
- electroactive polymer (2)
- electromagnetic radiation (2)
- electronic structure (2)
- energetic (2)
- exposed water ice (2)
- figure of merit (2)
- financial time series (2)
- first stars (2)
- first-hitting time (2)
- fluctuations (theory) (2)
- fluorescence (2)
- fluoroethylenepropylene (FEP) copolymer (2)
- fractal (2)
- fractal dimension (2)
- galaxies (2)
- galaxies: clusters: general (2)
- galaxies: general (2)
- galaxies: individual: SMC (2)
- galaxies: individual: Small Magellanic Cloud (2)
- galaxies: magnetic fields (2)
- galaxies: star clusters: general (2)
- galaxies: stellar content (2)
- galaxies: structure (2)
- gamma rays: diffuse background (2)
- general (2)
- general relativity (2)
- genomic DNA conformation (2)
- global surface warming (2)
- gold (2)
- granite (2)
- graphene (2)
- gravitational lensing: strong (2)
- gravity (2)
- green solvents (2)
- horizontal-branch (2)
- hybrid material (2)
- hyperbolic attractor (2)
- ice absorption features (2)
- impact (2)
- infrared thermography (2)
- infrared: galaxies (2)
- inner magnetosphere (2)
- inorganic perovskites (2)
- instability (2)
- interface recombination (2)
- interstellar ice (2)
- ion mobility spectrometry (2)
- ionosphere (2)
- iron (2)
- kinetic instabilities (2)
- kink-like instability (2)
- laser pulses (2)
- linearized gravity (2)
- loss mechanisms (2)
- low (2)
- low-density polyethylene (2)
- machine learning (2)
- magnetoconvection (2)
- magnetostriction (2)
- mechanical properties (2)
- mechanobiology (2)
- membrane (2)
- memory and delay (2)
- memory effects (2)
- metal (2)
- meteorological extremes (2)
- microcracking (2)
- microstructure (2)
- mid-temperature transition (2)
- miscellaneous (2)
- modeling (2)
- modelling (2)
- models (2)
- murchison meteorite (2)
- nanocomposite (2)
- neural networks (2)
- neuronal networks (2)
- nitrogen (2)
- noisy systems (2)
- non-Langevin recombination (2)
- non-equilibrium (2)
- non-linear dynamics (2)
- nonfullerene acceptors (2)
- nonlocal coupling (2)
- nonradiative recombination (2)
- nonradiative voltage losses (2)
- novae, cataclysmic variables (2)
- nucleosome (2)
- numerical relativity (2)
- ocean heat uptake (2)
- open clusters and associations: general (2)
- optical manipulation (2)
- optics (2)
- organic electronics (2)
- pQCT (2)
- peptides (2)
- permittivity enhancement (2)
- perovskite solar cell (2)
- phase transition (2)
- phase transitions (2)
- photo-isomerization (2)
- photocatalysis (2)
- photoelectron (2)
- photoluminescence quenching (2)
- photosensitive surfactants (2)
- photovoltaics (2)
- pitch angle (2)
- planetary rings (2)
- planetary systems (2)
- planets and satellites: fundamental parameters (2)
- planets and satellites: gaseous planets (2)
- planets and satellites: general (2)
- plasma instabilities (2)
- plasmaspheric hiss (2)
- polyelectrolyte adsorption (2)
- polyethylene (2)
- polymer (2)
- power spectral analysis (2)
- pp-wave solutions (2)
- probability density function (2)
- professional knowledge (2)
- proper motions (2)
- protein search (2)
- pulsars: individual: PSR B0833-45 (2)
- pump-probe (2)
- quantum field theory (2)
- quartz crystal microbalance (2)
- quasi-Fermi level splitting (2)
- quenched energy landscape (2)
- radiation mechanisms: nonthermal (2)
- random diffusivity (2)
- reaction kinetics theory (2)
- recollimation shocks (2)
- recombination order (2)
- relaxor-ferroelectric polymer (2)
- resolution infrared-spectroscopy (2)
- ring current (2)
- rotation (2)
- rupturing of metal film (2)
- selective laser melting (2)
- selective laser melting (SLM) (2)
- sensors and actuators (2)
- space-charge stability (2)
- specific surface area (2)
- spin (2)
- spin-orbit interaction (2)
- split Hopkinson pressure bar (2)
- stars: flare (2)
- stars: individual (WR 6) (2)
- stars: individual ([HD 36486]delta Ori A) (2)
- stars: individual (gamma Cassiopeiae) (2)
- stars: individual: WR 102c (2)
- stars: individual: WR 102ka (2)
- stars: jets (2)
- stars: solar-type (2)
- stars: variables: Cepheids (2)
- statistics (2)
- stochastic thermodynamics (2)
- structural health monitoring (2)
- structure (2)
- structures (2)
- submillimetre: ISM (2)
- sulfur (2)
- superalloys (2)
- surface modification (2)
- surface-enhanced Raman scattering (2)
- synchronization transition (2)
- synchrotron X-ray refraction radiography (2)
- synchrotron radiation (2)
- systems (2)
- techniques (2)
- techniques: radial velocities (2)
- teleconnections (2)
- temperature dependence (2)
- texture (2)
- thermal (2)
- thermal expansion (2)
- thermally stimulated discharge (2)
- thick junctions (2)
- thin films (2)
- time averaging (2)
- time-series analysis (2)
- titanium dioxide (2)
- trabecular bone (2)
- transient chaos (2)
- tropical cyclones (2)
- ultrafast X-ray diffraction (2)
- ultrafast dynamics (2)
- ultraviolet: galaxies (2)
- ultraviolet: stars (2)
- weak ergodicity breaking (2)
- work function (2)
- young stellar objects (2)
- (16) Psyche (1)
- (PEDOT (1)
- (Z)-isomer (1)
- (galaxies:) intergalactic medium (1)
- (galaxies:) quasars: absorption lines (1)
- (high-)voltage measurements (1)
- (magnetohydrodynamics) MHD (1)
- 1,3,4-oxadiazole (1)
- 1/f noise (1)
- 15 (1)
- 16 (1)
- 2101 duplex stainless steel (1)
- 2D colloid ordering (1)
- 3-D diffusion simulation (1)
- 30S subunit (1)
- 3D medical image analysis (1)
- 3D printing (1)
- 3D tomography (1)
- 3d metals (1)
- 4-nitrobenzenethiol (1)
- 4-nitrophenol (1)
- 6H-SiC (1)
- 7924 (1)
- 7934 (1)
- 7959 (1)
- AG (1)
- AGN (1)
- AI (1)
- ANFO (1)
- APCI (1)
- APECS (1)
- ARFIMA (1)
- ARTOF (1)
- ASDs (1)
- ASR-sensitive aggregate (1)
- AU (1)
- Absorption (1)
- Acceleration of particles (1)
- Accelerator mass spectrometry (1)
- Accelerometer (1)
- Accretion (1)
- Accretion processes (1)
- Acoustic probing of electric-field profiles (1)
- Actin cytoskeleton dynamics (1)
- Actin waves (1)
- Active Galactic Nuclei (1)
- Active flow control (1)
- Active galactic nuclei (1)
- Actuator (1)
- Actuators (1)
- Adam-Delbruck scenario (1)
- Adhesion (1)
- African climate (1)
- Ageing (1)
- Aggregate states (1)
- Air showers (1)
- Airless bodies (1)
- All-polymer heterojunctions (1)
- Alternating copolymers (1)
- Amazon rainforest (1)
- Ambipolar charge transport (1)
- Ambipolar materials (1)
- Amplitude death (1)
- Analysis technique (1)
- Anions (1)
- Anisotropy (1)
- Annealing (metallurgy) (1)
- Annealing treatment (1)
- Anomalous diffusion exponent (1)
- Anomalous transport (1)
- Answer Set Programming (1)
- Antarctica (1)
- Anthropocene (1)
- Antibiotics (1)
- Aqueous solution (1)
- Arabidopsis thaliana (1)
- Arctic clouds (1)
- Arnold diffusion (1)
- Astrobiology (1)
- Astronomy and astrophysics (1)
- Astronomy and planetary science (1)
- Astronomy data (1)
- Astronomy databases (1)
- Astroparticle physics (1)
- Astrophotonics (1)
- Astrophotonik (1)
- Astrophysics (1)
- Astrosphere (1)
- Astrostatistics tools (1)
- Asymmetric warming (1)
- Asymptotic expansions (1)
- Atlantic Meridional Overturning Circulation (1)
- Atmospheric entry (1)
- Atmosphärendynamik (1)
- Au nano-particle (1)
- Au-Pd nanorods (1)
- Auger decay (1)
- Auger electron (1)
- Auger electron spectroscop (1)
- Auger electron spectroscopy (1)
- Auger–Meitner (1)
- BESSY II (1)
- BL Lacertae objects: individual (1)
- BL Lacertae objects: individual (1ES 0229+200, VER J0232+202) (1)
- BL Lacertae objects: individual (1ES 0414+009, ERJ0416+011) (1)
- BL Lacertae objects: individual (1ES 1959+650) (1)
- BL Lacertae objects: individual (1ES 1959+650=VER J1959+651) (1)
- BL Lacertae objects: individual (1ES1218+30.4) (1)
- BL Lacertae objects: individual (B2 1215+30, VER J1217+301) (1)
- BL Lacertae objects: individual (BL Lacertae = VER J2202+422) (1)
- BL Lacertae objects: individual (HESS J1943+213, VER J1943+213) (1)
- BL Lacertae objects: individual (PG 1553+113) (1)
- BL Lacertae objects: individual (PKS 1424+240)-cosmic background radiation (1)
- BL Lacertae objects: individual (RBS 0413-VER J0319+187) (1)
- BL Lacertae objects: individual (RX J0648.7+1516, 1FGL J0648.8+1516, VER J0648+152) (1)
- BL Lacertae objects: individual (TXS 0506+056, VER J0509+057) (1)
- BL Lacertae objects: individual (VER J0521+211) (1)
- BL Lacertae objects: individual: 1ES 1312-423 (1)
- BL Lacertae objects: individual: 1ES 2322-409 (1)
- BL Lacertae objects: individual: 1ES 2344+514=VERJ2347+517 (1)
- BL Lacertae objects: individual: AP Librae (1)
- BL Lacertae objects: individual: Markarian 501 (1)
- BL Lacertae objects: individual: Mrk501 (1)
- BL Lacertae objects: individual: PKS 1424+240 (1)
- BL Lacertae objects: individual: SHBL J001355.9-185406 (1)
- BL Lacertae objects: individual: lES 0229+200 (1)
- BL Lacertae objects: individual: lES 1101-232 (1)
- Backbone modifications (1)
- Bacterial biofilms (1)
- Baseline shift (1)
- Bastille Day geomagnetic storm (1)
- Bayesian Model Averaging (1)
- Bayesian estimation (1)
- Be-10 exposure dating (1)
- Beam dynamics (1)
- Beam-plasma instability (1)
- Benzoic acids (1)
- Bessel functions (1)
- Beta-eucryptite (1)
- Bethe (1)
- Bi-harmonic coupling function (1)
- Bifurcations (1)
- Bifurcations of tori (1)
- Bilayer solar cells (1)
- Bio-electrochemical sensing (1)
- Biodiversity (1)
- Biofilms (1)
- Biological Physics (1)
- Biological defense mechanisms (1)
- Biomaterial (1)
- Biomechanics (1)
- Biosignature (1)
- Bipolar (1)
- Black– Scholes model (1)
- Bleihalogenid-Perowskite (BHP) (1)
- Bloch-Torrey equation (1)
- Blue stars (1)
- Booster cavity (1)
- Boreal forest diebacks (1)
- Bose-Hubbard model (1)
- Bosonic stimulation (1)
- Boundary value problem (1)
- Bragg peak (1)
- Breathing chimera states (1)
- Brillouin zone (BZ) (1)
- Brillouin-Zone (BZ) (1)
- Broadband synchronization (1)
- Brownian diffusion (1)
- Brownian motors (1)
- Brownian nanomachines (1)
- Brownian yet non-Gaussian diffusion (1)
- Bryophyte (1)
- Bulk heterojunction (1)
- C60 (1)
- CAL-72 osteoblasts (1)
- CAPS (1)
- CDA (1)
- CH center dot center dot center dot F hydrogen bonds (1)
- CH3NH3SnI3 (1)
- CMAS (1)
- CMIP-5 (1)
- CO desorption (1)
- COVID-19 (1)
- CT (1)
- CZTSe (1)
- Caged compounds (1)
- Callisto (1)
- Capacitance spectroscopy (1)
- Carbon fiber (1)
- Carbon nitride (1)
- Carrier dynamics (1)
- Cartilage tissue engineering (1)
- Casimir effect (1)
- Catalysis (1)
- Cattaneo equation (1)
- Cauchy problem (1)
- Causality (1)
- Cavity quantum electrodynamics (1)
- Cavity-quantum electrodynamics (1)
- Cayley trees (1)
- Ce/Zr (1)
- Cell fusion (1)
- Cell polarity (1)
- Cells (1)
- Cellular polypropylene (PP) (1)
- Central Chile (1)
- Central asia (1)
- Chain of van der Pol oscillators (1)
- Chaos (1)
- Chaos spreading (1)
- Chaos synchronization (1)
- Chaotic System (1)
- Characteristic function (1)
- Charge extraction (1)
- Charge generation (1)
- Charge recombination (1)
- Charge separation (1)
- Charge stability (1)
- Charge storage and transport (1)
- Charge transport (1)
- Charge-transfer state (1)
- Charging or poling (1)
- Chebyshev inequality (1)
- Chemotaxis (1)
- Cherenkov Telescopes (1)
- Cherenkov radiation (1)
- Chimera (1)
- Chorus waves (1)
- Chromatin pairing (1)
- Chromosphere (1)
- Chromosphere, active (1)
- Chromosphere, quiet (1)
- Churyumov-Gerasimenko (1)
- Circumplanetary dust (1)
- Classroom management (1)
- Climate change (1)
- Climate modeling (1)
- Climate variability (1)
- Climatic tipping points (1)
- Clock Tree Implementation (1)
- Coherence (1)
- Coherence-incoherence (1)
- Cohesive finite elements (1)
- Collision cross-section (1)
- Colombia (1)
- Colorimetric analysis (1)
- Comb-lattice model (1)
- Comets composition (1)
- Comets nucleus (1)
- Competencies (1)
- Complementarity (1)
- Complete Bernstein function (1)
- Completely monotone function (1)
- Composite fractional derivative (1)
- Composites (1)
- Composition (1)
- Compton and Pair Creation Telescope (1)
- Compton and pair creation telescope (1)
- ConCap (1)
- Conceptual model (1)
- Condensed matter physics (1)
- Conducting polymers (1)
- Confocal Raman microscopy (1)
- Conformational disorder (1)
- Conjugated polymeric thin film (1)
- Conservation policy (1)
- Core-hole clock (1)
- Corona (1)
- Coronal mass ejection (CME) (1)
- Coronal mass ejections (1)
- Coronal mass ejections, initiation and propagation (1)
- Correlation function (1)
- Cosmic Antimatter (1)
- Cosmic Rays (1)
- Cosmic-ray acceleration (1)
- Cosmogenic isotopes (1)
- Cosmogenic nuclides (1)
- Coster–Kronig (1)
- Counterparts of gravitational waves (1)
- Covalent interaction (1)
- Crack detection (1)
- Creep (1)
- Critical freshwater threshold (1)
- Crossmodal matching (1)
- CryoSat-2 (1)
- Crystalline phases (1)
- CsPbI2Br (1)
- Cu-Zn disorder (1)
- Cu2ZnSnSe4 (1)
- CuI (1)
- Curie-transition (1)
- Cw electron beam (1)
- Cycle-averaged tilt angle (1)
- Cyclones (1)
- Cylindrical comb (1)
- Cystic fibrosis (1)
- D. discoideum (1)
- DAQ (1)
- DIC (1)
- DNA hybridization (1)
- DNA methylation (1)
- DNA supercoiling (1)
- DNA volume and persistent length (1)
- DNA-PAINT (1)
- DNA-protein binding (1)
- DNA-surfactant complexes (1)
- Damage (1)
- Dark Matter (1)
- Data acquisition (1)
- Data analysis (1)
- Datenanalyse (1)
- Decay semigroups (1)
- Degradable polymer (1)
- Dehydrothermal cross linking (1)
- Deimos (1)
- Delphi study (1)
- Density functional theory (1)
- Design concepts (1)
- Detector modelling and simulations II (electric fields, charge transport, multiplication and induction, pulse formation, electron emission, etc) (1)
- Detergent (1)
- Deutschland (1)
- Dielectric Relaxation Spectroscopy (DRS) (1)
- Dielectric elastomer (1)
- Dielectric elastomer actuator (DEA) (1)
- Dielectric hysteresis (1)
- Dielectric polymer (1)
- Differential Code Biases (DCB) (1)
- Differential Scanning Calorimetry (DSC) (1)
- Diffraction (1)
- Diffuse radiation (1)
- Diffusion NMR (1)
- Diffusion coefficients (1)
- Dilational rheology (1)
- Diphenyl-1,3,4-oxadiazole (1)
- Diphenyl-oxadiazoles (1)
- Direct searches (1)
- Disaggregation (1)
- Disaster impact analysis (1)
- Disks (1)
- Dislocation motion (1)
- Disorder (1)
- Disperse dyes (1)
- Dispersion force (1)
- Distributed order diffusion-wave equations (1)
- Diversity (1)
- Donor materials (1)
- Donor-Acceptor (DA) interface (1)
- Donor-acceptor copolymers (1)
- Doped semiconductors (1)
- Double-jet (1)
- Driving mechanism (1)
- Drop profile analysis tensiometry (1)
- Drude model (1)
- Dust dynamics (1)
- Dust sources and sinks (1)
- Dwarf galaxies (1)
- Dye transfer (1)
- Dynamic loading (1)
- Dynamical invariants (1)
- Dynamik in rumpfangeregten Zuständen (1)
- E-ring (1)
- E.coli (1)
- EAP (1)
- EBSD (1)
- EMIC waves (1)
- ESA cosmic vision (1)
- Early Universe (1)
- Earth System trajectories (1)
- East Africa (1)
- Ecological-economic modelling (1)
- Econophysics (1)
- Edwards-Anderson order parameter (1)
- Effect of sintering (1)
- Efficiency optimization (1)
- Electric polarization (1)
- Electric potential (1)
- Electrical insulation (1)
- Electrical monitoring (1)
- Electrical properties (1)
- Electrical properties and parameters (1)
- Electro-active and electro-passive dielectrics (1)
- Electrochemical impedance spectroscopy (1)
- Electrodes (1)
- Electromagnetic waves (1)
- Electron back-scattered diffraction (1)
- Electron populations (1)
- Electron traps (1)
- Electron-phonon coupling (1)
- Electronic and spintronic devices (1)
- Electronic properties (1)
- Electronic properties and materials (1)
- Electronic structure (1)
- Electronics, photonics and device physics (1)
- Electrospray ionization (1)
- Electrostatic screening (1)
- Electrostatics (1)
- Elliptic complex (1)
- Energetic disorder (1)
- Energy (1)
- Energy science and technology (1)
- Energy-dispersive Laue diffraction (1)
- Energy-level alignment (1)
- Enzymatic degradation (1)
- Epidemic spreading models (1)
- Epoxy resin (1)
- Epoxy resins (1)
- Equilibrium (1)
- Erhebungsinstrument (1)
- Eukaryotic chemotaxis (1)
- Europa (1)
- European storm-time model (1)
- Event synchronization (1)
- Excitable dynamics (1)
- Excitable systems (1)
- Excited-state calculations; (1)
- Excitonic interactions (1)
- Experimental techniques (1)
- Explainable AI (1)
- External quantum efficiency (1)
- Extragalactic astronomy (1)
- Extreme precipitation (1)
- Extremotolerant (1)
- Extremum seeking (1)
- F-region dynamo currents (1)
- FRAP (1)
- Fachdidaktik (1)
- Fachwissen (1)
- False negative (1)
- False positive (1)
- Fe-Ni-Meteorite (1)
- Fe2TiO5 (1)
- Fermi (1)
- Fermi-level alignment (1)
- Fermi-level pinning (1)
- Ferroelectret (1)
- Ferroelectric polarization (1)
- Ferroelectric polymer (1)
- Feshbach resonance (1)
- Fiber-reinforced concrete (1)
- Field emission (1)
- Field-effect (1)
- Field-emission-based quasi continuous-wave electron beam (1)
- Flare (1)
- Flares, dynamics (1)
- Flashing ratchets (1)
- Flexible membrane (1)
- Flims (1)
- Fluorescence quantum yield (1)
- Flussfotolyse (1)
- Fokker-Planck equations (1)
- Fokker-Planck-Smoluchowski equation (1)
- Fokker– Planck equation (1)
- Forcemyography (1)
- Forward and reverse shocks (1)
- Fox H-functions (1)
- Fractal (1)
- Fractal dimension (1)
- Fractional Brownian motion (1)
- Fractional calculus (primary) (1)
- Fractional diffusion equation (1)
- Frank-Condon analysis (1)
- Free carrier generation (1)
- Free electron laser (1)
- Free-electron laser (1)
- Free-electron-laser science (1)
- Fusion crust (1)
- GEANT4 modeling (1)
- GISAXS (1)
- GMR sensors (1)
- GPS and Glonass (1)
- GRACE-FO (1)
- Galactic Ring Survey (1)
- Galactic cosmic rays (1)
- Galaxies: high-redshift (1)
- Galaxies: interactions (1)
- Galaxy: abundances (1)
- Galaxy: centre (1)
- Galaxy: general (1)
- Gamma ray astronomy (1)
- Gamma rays: General (1)
- Gamma-Ray Bursts (1)
- Gamma-ray bursts (1)
- Ganglion (1)
- Ganymede (1)
- Gardner equation (1)
- Gelatin-NaCMC (1)
- Gelatin-NaPAA composites (1)
- Gelatin-PLGA Scaffold (1)
- Generalized Langevin equation (1)
- Generic modelling (1)
- Geochemistry (1)
- Ginzburg-Landau lattice (1)
- Glaciation (1)
- Glaciation Central Asia (1)
- Global Navigation Satellite System (GNSS) (1)
- Global supply chains (1)
- Gold nanoparticles (1)
- Gold@polydopamine (1)
- Gompertz growth function (1)
- Granite (1)
- Graphene (1)
- Green formulas (1)
- Green function (1)
- Green's function (1)
- Green’ s functions (1)
- Grimmia sp (1)
- Ground based gamma ray astronomy (1)
- Grunwald-Letnikov approximation (1)
- HAT-P-16 (1)
- HESS (1)
- HESS Galactic Plane Survey (1)
- HESS J1825-137 gamma-rays (1)
- HRTEM (1)
- HTL (1)
- Haake-Lewenstein-Wilkens approach (1)
- Half-center oscillator (1)
- Haptics (1)
- Heat Transfer (1)
- Heavy-tails (1)
- Heliosphere (1)
- Helium (1)
- Hermite polynomial expansion (1)
- Heteroclinic cycle (1)
- Heterogeneous (1)
- Heterogeneous catalysis (1)
- Hexagonal grid (1)
- Hierarchical Design (1)
- Higgs boson (1)
- High specific surface area (1)
- High transmission micro focus beamline (1)
- High-Energy Astrophysics (1)
- High-Energy Gamma-Ray Astronomy (1)
- High-impact polystyrene (1)
- Hilbert Scales (1)
- Hitzewellen (1)
- Hodgkin-Huxley model (1)
- Holocene extension (1)
- Homology (1)
- Hong-Ou-Mandel effect (1)
- Hp30 (1)
- Hp60 (1)
- Hpo (1)
- Humic substance (1)
- Hurricane Sandy (1)
- Hybrid materials (1)
- Hybrid solar cells (1)
- Hydroclimate (1)
- Hydrogen activation (1)
- Hydrolytic degradation (1)
- Hyperbolic chaos (1)
- Hypernetwork (1)
- IMPTAM (1)
- IN718 (1)
- IR ellipsometry (1)
- IR spectroscopy (1)
- IR-MALDI (1)
- ISM : supernova remnants (1)
- ISM: Supernova remnants (1)
- ISM: general (1)
- ISM: individual objects (Crab Nebula) (1)
- ISM: individual objects (G120.1+01.4, Tycho=VER J0025+641) (1)
- ISM: individual objects (LMC N11) (1)
- ISM: individual objects (RX J1713.7-3946) (1)
- ISM: individual objects (RX J1713.7-3946, G347.3-0.5) (1)
- ISM: individual objects (SNR G338.3-0.0, SNR G338.5+0.1) (1)
- ISM: individual objects: Crab nebula (1)
- ISM: individual objects: HESS J1832-093 (1)
- ISM: individual objects: IRAS 20286+4105 (1)
- ISM: individual objects: M 42 (1)
- ISM: individual objects: Puppis A (1)
- ISM: individual objects: SNR G1.9+0.3 (1)
- ISM: individual objects: SNR G22.7-0.2 (1)
- ISM: individual objects: SNR G330.2+1.0 (1)
- ISM: individual objects: Tarantula Nebula (30 Doradus Nebula) (1)
- ISM: individual objects: Tycho's SNR (1)
- ISOS-L-1I protocol (1)
- IZO (1)
- Ice core (1)
- Ices (1)
- Impurity segregation (1)
- In-situ (1)
- India (1)
- Indian summer monsoon (1)
- Indirect searches (1)
- Information coding (1)
- Infrared observations (1)
- Infrared radiation (1)
- Inhibitory neurons (1)
- Initiation and propagation (1)
- Inner magnetosphere (1)
- Instructional quality (1)
- Instrumental effects (1)
- Insulators (1)
- Integrated Kalman filter (1)
- Integrated spectrograph (1)
- Inter-hemispheric (1)
- Interaction (1)
- Interaction of radiation with matter (1)
- Interdisciplinary Physics (1)
- Interface (1)
- Interface dipole (1)
- Interfaces (1)
- Interfacial molecular interaction (1)
- Interfacial strength (1)
- Interfacial tension (1)
- Interior (1)
- Interlayer (1)
- Intermittency (1)
- Internal stress (1)
- Interplanetary dust (1)
- Interpretation (1)
- Intrachain order (1)
- Intragap states (1)
- Intramolecular deactivation (1)
- Intrinsically disordered protein (1)
- Inverted solar cells (1)
- Ion mobility spectrometry (1)
- Ionospheric monitoring and modeling (1)
- Ir(111) (1)
- Janus gels (1)
- Jets (1)
- Jetstream (1)
- Josephson junction (1)
- Junction model (1)
- Jupiter's magnetosphere (1)
- K-Kanten Weichröntgenspektroskopie (1)
- K-edge soft X-ray spectroscopy (1)
- Kelvin probe (1)
- Khalerchinskaya tundra (1)
- Kinesthetic representations (1)
- Kompetenzerwerb (1)
- Konzentration (1)
- Konzeption (1)
- Kp index (1)
- Kurzzeitspektroskopie mit optischer Anregung und Röntgendetektion (1)
- L-929 fibroblasts (1)
- L-Asterisk (1)
- L-edge spectroscopy (1)
- LCST behavior (1)
- LHC (1)
- LLG equation (1)
- Lagrangian statistics (1)
- Land use (1)
- Land-sea thermal contrast (1)
- Landslide (1)
- Lanthanides (1)
- Large deviation statistics (1)
- Larsen Ice Shelf (1)
- Laser resonators (1)
- Laser spectroscopy (1)
- Late embryogenesis abundant protein (1)
- Lattice dynamics (1)
- Lax-Phillips theory (1)
- Layer-by-layer (1)
- Lehramtsstudent (1)
- Lehrer (1)
- Lehrerbildung (1)
- Levy flight (1)
- Levy foraging hypothesis (1)
- Life cycle assessment (1)
- Ligand-field state (1)
- Ligands (1)
- Light induced diffusioosmotic flow (1)
- Light-harvesting complex (1)
- Linear theory (1)
- Linearly increasing voltage (CELIV) (1)
- Lipid bilayer (1)
- Liquid Jet (1)
- Liquids (1)
- Local density of states (1)
- Local spectroscopy (1)
- Localization regime (1)
- Localized chaos (1)
- Long-range bridging (1)
- Long-range dependence (1)
- Longitudinal Analysis (1)
- Low Earth Orbit (1)
- Low band-gap (1)
- Low carbon steel (1)
- Low voltage losses (1)
- Lysozyme (1)
- Längsschnittstudie (1)
- Längsschnittuntersuchung (1)
- Lévy flights (1)
- Lévy walks (1)
- M37 (NGC2099) (1)
- MATROSHKA-R (1)
- MD simulations (1)
- MD-Simulationen (1)
- Machine learning (1)
- Machine learning control (1)
- Magellanic Cloud (1)
- Magnetic field amplification (1)
- Magnetic fields (1)
- Magnetic stray field (1)
- Magnetism (1)
- Magneto-hydrodynamic modeling (1)
- Magnetohydrodynamics (1)
- Magnetosphere (1)
- Magnetospheres (1)
- Magnetospheric physics (1)
- Markarian 421 (1)
- Markov additive processes (1)
- Mass spectroscopy (1)
- Massive stars (1)
- Maule 2010 earthquake (1)
- Maximum likelihood estimation (1)
- Mean first encounter time (1)
- Mechanical alloying (1)
- Mechanosensitive proteins (1)
- Mechanosensitiven Proteine (1)
- Mediation-model (1)
- Mellin transform (1)
- Melting experiments (1)
- Membrane stability (1)
- Membrane tension (1)
- Membranspannung (1)
- Memory device (1)
- Memory effects (1)
- Meridional overturning circulation (1)
- Messung (1)
- Metal complexation (1)
- Metal matrix composite (1)
- Metals (1)
- Meteorites (1)
- MgO nanoparticles (1)
- Microcracked ceramics (1)
- Microfluidics (1)
- Micromechanical modeling (1)
- Micromechanical schemes (1)
- Micropipette aspiration (1)
- Microscopic charcoal (1)
- Microscopic morphology (1)
- Microstructure (1)
- Microstructure and (1)
- Microstructure and texture (1)
- Microwave processing (1)
- Mid-temperature transition (1)
- Migration (1)
- Mikrokanal (1)
- Minerals (1)
- Minimax convergence rates (1)
- Mittag-Leffler (1)
- Mittag-Leffler function (1)
- Mixed adsorption layers (1)
- MoS2 (1)
- Mobility imbalance (1)
- Mobility relaxation (1)
- Mode function (1)
- Model ligand (1)
- Model structural error (1)
- Moisture change (1)
- Molar water content (1)
- Molecular clouds (1)
- Molecular structure (1)
- Monitoring (1)
- Monolayer (1)
- Monomolecular reaction (1)
- Monopolar (1)
- Monte Carlo simulation (1)
- Moon (1)
- Moonlets (1)
- Moonlight (1)
- Motivation (1)
- Multi-branch entrainment (1)
- Multi-dimensional Markovian embedding of non-Markovian dynamics (1)
- Multilayer graphene (1)
- Multiphase composites (1)
- Multiple trapping model (1)
- Multiwavelength Observations of the Universe (1)
- NEXAFS (1)
- NGC 1786 (1)
- NGC 1898 (1)
- NLP (1)
- NTCM (1)
- Nano-dielectrics (1)
- Nanocomposites (1)
- Nanograin charge (1)
- Nanograins (1)
- Nanoparticles (1)
- Nanoreactor (1)
- Nanoscale heat transfer (1)
- Nanostructure (1)
- Natural satellites (1)
- Near edge X-ray absorption fine structure (1)
- Near infra-red (1)
- Near-Field Optics (1)
- Near-field thermal radiation (1)
- Negative (1)
- Network (1)
- Network inference (1)
- Neural network (1)
- Neurooscillators (1)
- Next generation Cherenkov telescopes (1)
- Ni (1)
- Ni(111) (1)
- Nickel-based (1)
- Nickel-based superalloy (1)
- Node degree distribution (1)
- Noether theorem (1)
- Non-Gaussian (1)
- Non-Markovian processes (1)
- Non-geminate recombination (1)
- Non-linear analysis (1)
- Non-linear dielectric spectroscopy (1)
- Non-perturbative analysis (1)
- Nonaqueous sol-gel (1)
- Noncommutative geometry (1)
- Nonlinear X-ray spectroscopy (1)
- Nonlinear analysis (1)
- Nonlinear polarization spectroscopy in the frequency domain (1)
- Nonlinearity (1)
- Nonradiative recombination (1)
- North Atlantic variability (1)
- Northern sinking (1)
- Nuclear Astrophysics (1)
- Nuclear physics (1)
- Nucleosynthesis (1)
- Numerical simulations (1)
- OFET (1)
- OLED (1)
- Oberflächen-Brillouin-Zone (OBZ) (1)
- Observations (1)
- Observing methods (1)
- Ocean (1)
- Odor discrimination (1)
- Olfactory system (1)
- Open-circuit voltage (1)
- Optical modeling (1)
- Optical properties (1)
- Optimal control (1)
- Optimization (1)
- Opto-mechanically induced scission of polymer chains (1)
- Optoelectronic devices and components (1)
- Optoelectronic properties (1)
- Optoelectronics (1)
- Organic FeFET (1)
- Organic LEDs (1)
- Organic TFT (1)
- Organic matter (1)
- Organic thermoelectrics (1)
- Ornstein–Uhlenbeck process (1)
- Oscillator populations (1)
- Ott - Antonsen reduction (1)
- Ott-Antonsen equation (1)
- Ott-Antonsen reduction (1)
- Ott-Antonsen theory (1)
- Overturning sensitivity (1)
- Oxygen (1)
- P(VDF-TFE) copolymer (1)
- P(VDF-TrFE-CFE) (1)
- PBD (1)
- PBLG (1)
- PBT7 (1)
- PBTTT (1)
- PDA (1)
- PEDOT (1)
- PEDOT:PSS (1)
- PI3K (1)
- PIP2 (1)
- PIP3 (1)
- PIP3 signals (1)
- PNIPAM (1)
- PNIPAm (1)
- POD (1)
- PSD (1)
- PSS)-coated porous (1)
- PTEN (1)
- PVPVA (1)
- Packing motif (1)
- Paleoclimate modeling (1)
- Parametric drift estimation (1)
- Pareto analysis (1)
- Pareto law (1)
- Partial synchrony (1)
- Partial wavelet coherence (1)
- Partially alternating copolymers (1)
- Particle acceleration (1)
- Particles precipitating (1)
- Particles trapped (1)
- Paschen's law (1)
- Patch clamp (1)
- Pedagogical professional knowledge (1)
- Peptides (1)
- Performance Assessment (1)
- Performanztest (1)
- Periodic solutions (1)
- Permittivity (1)
- Perovskite solar cell (1)
- Perovskite solar cells (1)
- Phase dynamics (1)
- Phase gate (1)
- Phase modulation (1)
- Phase reconstruction (1)
- Phase transition (1)
- Phonons (1)
- Photo-CELIV (1)
- Photocatalysis (1)
- Photoconductivity (1)
- Photocurrent (1)
- Photon density wave spectroscopy (1)
- Photonic devices (1)
- Photosensitive azobenzene containing polyamines (1)
- Photosensitive brushes (1)
- Photosensitive polymer brushes (1)
- Photosensitive polymer film (1)
- Photosensitive polymer films (1)
- Photosensitive surfactant (1)
- Photosphere (1)
- Photothermal conversion (1)
- Photovoltaic gap (1)
- Physical Implementation (1)
- Physik (1)
- Physikunterricht (1)
- Pickering Janus emulsions (1)
- Picosecond ultrasonics (1)
- Piezo1 (1)
- Piezo2 (1)
- Piezoelectrically generated Pressure Steps (PPSs) (1)
- Pigment-pigment interactions (1)
- Plane grating emission spectrometer (1)
- Planetary interior (1)
- Planetary rings and tori (1)
- Plant performance (1)
- Plasma Physics (1)
- Plasmonics (1)
- Platform magnetometers (1)
- Plio-Pleistocene (1)
- Polarization (1)
- Polaron (1)
- Pollen (1)
- Poly-epsilon-caprolactone (1)
- Polycrystals (1)
- Polyelectrolyte multilayer (1)
- Polyetlioxysiloxane (1)
- Polymer (1)
- Polymer infiltration (1)
- Polymer intermixing (1)
- Polymer-dispersed liquid crystal (1)
- Polymer/surfactant interaction (1)
- Porosity (1)
- Porous scaffold (1)
- Post-inhibitory rebound (1)
- Potential of mean force (1)
- Precise Point Positioning (PPP) (1)
- Prediction (1)
- Probabilistic projections (1)
- Probe instruments (1)
- Process analytical technology (1)
- Process atmosphere (1)
- Professional knowledge (1)
- Professionswissen (1)
- Prominences (1)
- Prominences, dynamics (1)
- Prominences, magnetic field (1)
- Prominences, quiescent (1)
- Propellers (1)
- Protein (1)
- Protein crowding (1)
- Protein folding (1)
- Protein-membrane interaction (1)
- Protonendynamik molekularer Systeme (1)
- Protonentransfer in angeregten Zuständen (1)
- Pseudo-Voigt fit function (1)
- Pseudomonas aeruginosa (1)
- Psyche mission (1)
- Pulse induced transparency (1)
- PyTorch (1)
- Pycnocline depth (1)
- Python (1)
- Quantum optics (1)
- Quartz (1)
- Quasicrystals (1)
- Quaternary glaciations (1)
- Quiescent (1)
- Quiet (1)
- RF gun (1)
- RIXS (resonant inelastic X-ray scattering) (1)
- RIXS at FELs (1)
- Radiation dose calculation (1)
- Radiation mechanisms: Non-termal (1)
- Radiation on the ISS (1)
- Radiation protection (1)
- Radio-frequency electron gun (1)
- Radiocarbon (1)
- Rainfall patterns (1)
- Random walks (1)
- Rare elements (1)
- Rashba effect (1)
- Rat model (1)
- Rayet (1)
- Reaction mechanism (1)
- Reactive adsorption (1)
- Reactive coupling (1)
- Reactive foaming (1)
- Real time (1)
- Real-time earthquake monitoring and early warning (1)
- Recombination losses (1)
- Recurrence analysis (1)
- Recurrence plots (1)
- Recurrence quantification analysis (1)
- Recurrent neural networks (1)
- Redox (1)
- Reflective writing (1)
- Reflexion (1)
- Reflexion (Phil) (1)
- Reflexionsmodell (1)
- Reflexionsqualität (1)
- Reflexionstiefe (1)
- Regionalization (1)
- Relaxor-ferroelectric (RF) fluoropolymers (1)
- Relaxor-ferroelectric polymer (1)
- Release (1)
- Reproducing kernel Hilbert space (1)
- Residue (1)
- Resolved and unresolved sources as a function of wavelength (1)
- Resonance fluorescence (1)
- Resonance-free ultrasound emitter (1)
- Resonant interaction (1)
- Retina (1)
- RhB degradation (1)
- RhB photodegradation (1)
- Riesz-Feller fractional derivative (1)
- Ring tensiometry (1)
- Robin boundary condition (1)
- Rock (1)
- Rock avalanche (1)
- Rocks (1)
- RsgA (1)
- Rydberg atoms (1)
- SCAPS-1D (1)
- SCP (1)
- SEM (1)
- SERS (1)
- SFXTs (1)
- SHPB (1)
- SIR model (1)
- SLM (1)
- SPR (1)
- SVD (1)
- Saddle Point (1)
- Satellites, Composition (1)
- Satellites, Surfaces (1)
- Saturn, Satellites (1)
- Saturn, rings (1)
- Saturn, satellites (1)
- Scaling exponents (1)
- Scan strategies (1)
- Scanning near-field optical microscopy (1)
- Scanning transmission electron microscopy (1)
- Scattering (1)
- Scattering breakdown (1)
- Scattering theory (1)
- Scher-Montroll Transport (1)
- Schottky junction (1)
- Schrödinger equation (1)
- Schulpraktikum (1)
- Science education (1)
- Seebeck coefficient (1)
- Seebeck ratchet (1)
- Sensing skin (1)
- SgXBs (1)
- Shannon entropy (1)
- Shape recognition (1)
- Shear flow (1)
- Shockley-Queisser model (1)
- Shockley-Read-Hall (1)
- SiO2 composite material (1)
- Signal transduction (1)
- Silica source (1)
- Silicification (1)
- Silicon (1)
- Silicon carbide (1)
- Siliziumdioxid-auf-Silizium (1)
- Simulations (1)
- Singularities (1)
- Smale - Williams solenoid (1)
- Small (1)
- Snap-through instability (1)
- Soft X-ray monochromator (1)
- Solar Cycle, observations (1)
- Solar chromosphere (1)
- Solar energy (1)
- Solar energy and photovoltaic technology (1)
- Solar physics (1)
- Solid state detectors (1)
- Solvents (1)
- Space charge (1)
- Space mining (1)
- Space mission (1)
- Space plasmas (1)
- Space radiation (1)
- Space vehicles: instruments (1)
- Space weather (1)
- Spacecraft (1)
- Specific surface (1)
- Spectral diffusion (1)
- Spike sequences (1)
- Spin-Bahn-Wechselwirkung (SBW) (1)
- Spin-echo (1)
- Spin-orbi coupling (SOC) (1)
- Spontaneous decay (1)
- Sputum (1)
- Stalagmite (1)
- Stars (1)
- Stars: atmospheres early type (1)
- Stars: individual: 4U2206+54, BD+53 2790 (1)
- Stars: mass-loss (1)
- Stars: winds (1)
- State space reconstruction (1)
- Statistical Physics (1)
- Statistical copolymers (1)
- Statistical inference (1)
- Statistical inverse problem (1)
- Statistical mechanics (1)
- Statistics (1)
- Stellar evolution (1)
- Stellar outflows (1)
- Stellar winds (1)
- Steppest Descend method (1)
- Stern-Gerlach effect (1)
- Stille-type cross-coupling (1)
- Stimulated scattering (1)
- Stimuli-responsive materials (1)
- Stochastic differential equations (1)
- Stochastic modelling (1)
- Stochastic reaction– diffusion (1)
- Storage rings (1)
- Strain gages (1)
- Strain gauge (1)
- Strain hardening (1)
- Strain monitoring (1)
- Stratosphere (1)
- Stratton-Chu formulas (1)
- Stress-strain relations (1)
- Stretchable sensor (1)
- Strong-motion sensor (1)
- Strontium (1)
- Structure-performance relationship (1)
- Structure-property relationships (1)
- Student Teachers (1)
- Sub-gamma random variable (1)
- Subdiffusion (1)
- Sublimation with good yield (1)
- Subretinal (1)
- Sun: Chromosphere (1)
- Sun: faculae, plages (1)
- Sun: filaments, pominences (1)
- Sun: infrared (1)
- Sun: magnetic reconnection (1)
- Sun: oscillations (1)
- Sun: radio radiation (1)
- Sun: solar radio bursts (1)
- Sun: surface magnetism (1)
- Sunspots (1)
- Sunspots, magnetic fields (1)
- Supernova Remnants (1)
- Supernovae (1)
- Superradiance (1)
- Surface (1)
- Surface Relief Grating (1)
- Surface composition (1)
- Surface plasmons (1)
- Surface properties (1)
- Surface relief grating (1)
- Surface-enhanced Raman scattering (1)
- Surfactant (1)
- Surfactants (1)
- Survival probability (1)
- Swift - Hohenberg equation (1)
- Synchrotron (1)
- Synchrotron Radiation (1)
- Synchrotron radiation (1)
- TCAD (1)
- TCOs (1)
- TD-DFT (1)
- TEM01 mode (1)
- TIC 278659026 (1)
- Tail (1)
- Talbot-Lau interferometer (1)
- Talbot-Lau interferometry (1)
- Tandem solar cells (1)
- Taylor-Couette flow (1)
- TeV gamma rays (1)
- TeV gamma-ray astronomy (1)
- Teacher Education (1)
- Teacher professional development (1)
- Techniques: imaging spectroscopy (1)
- Techniques: spectroscopy (1)
- Teleconnection patterns (1)
- Telekonnektionen (1)
- Tensile load (1)
- Tension (1)
- Terrestrial cosmogenic nuclide (1)
- Test (1)
- Testauswertung (1)
- Thermal Radiation (1)
- Thermal conductivity (1)
- Thermal diffusivity (1)
- Thermal effects (1)
- Thermal inertia (1)
- Thermal sound generation (1)
- Thermal wave method (1)
- Thermo-acoustic effect (1)
- Thermoclectrics (1)
- Thermodynamic efficiency (1)
- Thermodynamic properties (1)
- Thermodynamics of adsorption (1)
- Thermophone (1)
- Thermoplastics (1)
- Thermoresponsive (1)
- Thin film (1)
- Thin nanocrystalline TiO2 layer (1)
- Thiouracil (1)
- Tien Shan (1)
- Tikhonov regularization (1)
- Tilt angles (1)
- Time delay (1)
- Time of flight (1)
- Time series (1)
- Time series analysis (1)
- Time-dependent mobility (1)
- Time-of-flight (TOF) (1)
- Time-resolved spectroscopy (1)
- Time-varying Delay (1)
- Tip-sample interactions (1)
- Titan (1)
- Topological matter (1)
- Total Electron Content (TEC) (1)
- Trace elements (1)
- Transient fluorescence (1)
- Transient photocurrent (1)
- Transition-metal ion (1)
- Transport properties titania (1)
- Trapped charges (1)
- Tropics (1)
- Trypanosoma cruzi (1)
- Turbulence (1)
- Two-temperature model (1)
- US east coast river geomorphology (1)
- UV (1)
- UV cross-linking (1)
- UV irradiation (1)
- UV nanoimprint lithography (1)
- UV-VIS Spectroscopy (1)
- Ultra-high energy cosmic rays (1)
- Ultra-low (1)
- Ultrafast (1)
- Ultrafast X-ray diffraction (1)
- Ultrafast photoacoustics (1)
- Ultrafast spectroscopy (1)
- Ultrafast surface science (1)
- Ultrafast x-ray (1)
- Ultrafast x-ray diffraction (1)
- Ultrasound (1)
- Ultraviolet photoelectron spectroscopy (1)
- Ultraviolet: ISM (1)
- University physics (1)
- Unterrichtsgestaltung (1)
- Upconversion luminescence (1)
- Uracil (1)
- Uranus (1)
- V OC-deficit (1)
- V*V884 Sco (1)
- V-OC loss (1)
- VERITAS (1)
- VHE (1)
- VHE gamma-ray astronomy (1)
- Vacuum fields (1)
- Vacuum-level alignment (1)
- Valenzband (VB) (1)
- Valenzbandmaximum (VBM) (1)
- Validity (1)
- Validität (1)
- Venus, surface (1)
- Vibrio Harveyi clade (1)
- Visual representations (1)
- Voronoi entropy (1)
- WAAM (1)
- WASP-108 (1)
- WASP-113 (1)
- WASP-120 (1)
- WASP-123 (1)
- WASP-136 (1)
- WASP-140 (1)
- WASP-20 (1)
- WASP-76 (1)
- WASP-93 (1)
- Wartezeitverteilung (1)
- Washing fastness (1)
- Watanabe-Strogatz theory (1)
- Water Vapor (1)
- Water-assisted crystallization (1)
- Water/air interface (1)
- Wave Propagation (1)
- Wave generation (1)
- Wavelets (1)
- Wealth and income distribution (1)
- Weather regimes (1)
- West Antarctic Ice Sheet (1)
- Wind-fed systems (1)
- Wirtschaftsnetzwerk (1)
- Wolf-Rayet (1)
- Wrinkling (1)
- X-ray Spectroscopy (1)
- X-ray absorption (1)
- X-ray and (1)
- X-ray and neutron diffractions (1)
- X-ray binary (1)
- X-ray computed (1)
- X-ray diffraction (1)
- X-ray emission (1)
- X-ray emission spectra (1)
- X-ray mu CT (1)
- X-ray phase contrast (1)
- X-ray probe (1)
- X-ray refraction; (1)
- X-ray scattering (1)
- X-ray stars (1)
- X-ray structure (1)
- X-ray switching (1)
- X-ray synchrotron diffraction (1)
- X-rays : stars (1)
- X-rays: galaxies (1)
- X-rays: general (1)
- X-rays: individual (Carina) (1)
- X-rays: individual (Cygnus X-3) (1)
- X-rays: individual: 3A 1954+319 (1)
- X-rays: individual: 4U1700+24; (1)
- X-rays: individual: AX J1714.1-3912 (1)
- X-rays: individual: GJ 1151 (1)
- X-rays: individual: IGRJ17329-2731 (1)
- X-rays: individual: SXP 1323 (1)
- X-rays: individual: SctX-1 (1)
- X-rays: individuals: Circinus X-1 (1)
- X-rays: individuals: G15.4+0.1 (1)
- X-rays: individuals: GRS 1915+105 (1)
- X-rays: individuals: IGRJ16328-4726 (1)
- X-rays: individuals: IGRJ17354-3255 (1)
- X-rays: individuals: IGRJ17544-2619 (1)
- X-rays: individuals: IGRJ18450-0435 (1)
- X-rays: individuals: SAXJ1818.6-1703 (1)
- X-rays: individuals: V4641 Sgr (1)
- X-rays: individuals: Vela Jr (RX J08520-4622) (1)
- X-rays: individuals: Vela X-1 (1)
- XCT (1)
- XMCD (1)
- Yield strength (1)
- Young's double-slit experiment (1)
- Yttria stabilized zirconia multilayers (1)
- Zeolite synthesis (1)
- ZnO (1)
- Zufallsbewegung (1)
- ab initio (1)
- abelian group (1)
- absorption (1)
- absorption lines (1)
- absorption spectroscopy (1)
- accretion, accretion discs (1)
- acidic crosslinking (1)
- acoustic transducers (1)
- acoustic waves (1)
- acoustic-transducer materials (1)
- actin (1)
- actin dynamics (1)
- actin polymerization (1)
- actin waves (1)
- activator–inhibitor models (1)
- active matter (1)
- active particles (1)
- active solar (1)
- active solar chromosphere (1)
- activity - stars (1)
- activity - sun (1)
- actuator (1)
- actuators (1)
- adaptation (1)
- adaptation and mitigation (1)
- addenda (1)
- additive (1)
- additive manufacturing (AM) (1)
- adsorption (1)
- advective-diffusive codes (1)
- aftershock distribution (1)
- aging (1)
- air mass transformation; (1)
- alkali-silica reaction (ASR) (1)
- all-organic (1)
- all-organic ferroelectret nanogenerator (FENG) (1)
- all-perovskite tandems (1)
- allycyanide (1)
- aluminium alloys (1)
- aminothiophenol (1)
- amoeboid motility (1)
- amorphous solids (1)
- amorphous state (1)
- amphiphilic side chains (1)
- analysis - techniques (1)
- analytical model (1)
- analyzer-based imaging (1)
- anatomical connectivity (1)
- and governance (1)
- and surface diffusion (1)
- animal models (1)
- anisotropic fiber orientation (1)
- anomalous (1)
- anomalous (or non-Fickian) diffusion (1)
- anomalous diffusion and transport (1)
- anomalous dynamics with memory (1)
- anomalous heat conduction (1)
- anomalous response and relaxation (1)
- anti-Stokes resonant x-ray raman scattering (1)
- antidynamo theorem (1)
- antimicrobial peptides (1)
- antimicrobial polymers (1)
- antireflection (1)
- ap30 (1)
- ap60 (1)
- apo (1)
- applications (1)
- applied classical electromagnetism (1)
- approximate methods (1)
- arrayed waveguide grating (1)
- assembly factor (1)
- asteroid magnetospheres (1)
- asteroseismology (1)
- astrobiology (1)
- astrochemistry (1)
- astrometry (1)
- astronomical databases: miscellaneous (1)
- astronomy (Energetic particles) (1)
- astronomy spectrograph (1)
- astroparticle physic (1)
- astrophysics (1)
- asymmetric Levy flights (1)
- asymptotic analysis (1)
- asynchronous design (1)
- atmosphere (1)
- atmosphere - sun (1)
- atmosphere dynamics (1)
- atmospheric effects (1)
- atom-surface interaction (1)
- atomic data (1)
- atomic displacement parameters (1)
- atomic distances (1)
- atomic force microscopy (AFM) (1)
- atomic processes (1)
- atomtronics (1)
- attosecond phenomena (1)
- autocorrelation (1)
- autocorrelation function (1)
- autocorrelations (1)
- automated image processing (1)
- autoregressive models (1)
- axial next nearest neighbour Ising chains (1)
- azobenzene containing photosensitive material (1)
- azobenzene containing polymer films (1)
- azobenzene containing polymers (1)
- azobenzene containing surfactant (1)
- azobenzene elastomers (1)
- azobenzene photosensitive polymer films (1)
- azobenzene-containing molecules (1)
- background (1)
- bacteria (1)
- bacterial swimming (1)
- bacterial swimming strategies (1)
- ball mill (1)
- balloon telescopes (1)
- bandgap (1)
- barrier escape (1)
- barrier height (1)
- basis-sets (1)
- beam splitter (1)
- beyond Standard Model (1)
- bi-harmonic coupling (1)
- bi-photons (1)
- bifurcation (1)
- bifurcation analysis (1)
- bifurcation theory (1)
- bifurcations (1)
- bimetallic nanoparticles (1)
- binaries: symbiotic (1)
- binaries: visual (1)
- binary neutron stars (1)
- biochemical oscillators (1)
- biohybrid microsystems (1)
- bioindicators (1)
- biological invasions (1)
- biological robustness (1)
- bioluminescence (1)
- biophysical model (1)
- bioreceptors (1)
- biosensing (1)
- biosphere feedbacks (1)
- birefringence (1)
- bismuth (1)
- bismuthene (1)
- blade (1)
- block copolymer films (1)
- bonding layer at the metal/polymer interface (1)
- bottlebrush copolymers (1)
- boundary local time (1)
- brain rhythms (1)
- brain synchronization (1)
- bridges (1)
- broad-spectrum permittivity enhancement (1)
- brown dwarfs (1)
- brownian motion (1)
- brushes (1)
- bubbles (1)
- built-in potential (1)
- bulk (1)
- bulk-heterojunction solar cells (1)
- cAMP (1)
- cAMP receptor (1)
- caffeine (1)
- caged cAMP (1)
- calibration (1)
- cambridge cb4 0wf (1)
- cambs (1)
- cancer diagnosis (1)
- capacitance spectroscopy (1)
- carbon nitride thin film (1)
- cardiomyopathy (1)
- carrier density (1)
- cascading regime (1)
- cataclysmic variables (1)
- catanionic vesicles (1)
- causal discovery algorithm (1)
- cell motility (1)
- cell nucleus (1)
- cell polarity (1)
- cell wall deficient mutant (1)
- cell-cell (1)
- cellular (1)
- cellular signalling (1)
- cellular structures (1)
- cesium lead halides (1)
- chains (1)
- chalcogenide (1)
- channel (1)
- chaotic motion (1)
- chaotic neural dynamics (1)
- characterization (1)
- characterization of ultrasonic measurement systems (1)
- characterization tools (1)
- charge (1)
- charge accumulation (1)
- charge carrier density (1)
- charge carrier extraction (1)
- charge carrier processes (1)
- charge carrier recombination (1)
- charge carrier transport (1)
- charge collection (1)
- charge density (1)
- charge generation yield (1)
- charge injection across hybrid interfaces (1)
- charge localisation (1)
- charge recombination (1)
- charge recombination yield (1)
- charge repulsion (1)
- charge selectivity (1)
- charge shielding (1)
- charge stability (1)
- charge storage (1)
- charge transfer states (1)
- charge transfers (1)
- charge transport layers (1)
- charge-transfer excitations (1)
- chemical (1)
- chemical equilibrium (1)
- chemical oxidative polymerization (1)
- chemical relaxation (1)
- chemically reactive flow (1)
- chemomechanical coupling (1)
- chimera (1)
- chimera states (1)
- chirality (1)
- chlimate impacts (1)
- chloroplast ribosome (1)
- chromatin (1)
- chromosphere (1)
- chromosphere - methods (1)
- cirrus clouds (1)
- climate trends (1)
- climate variability (1)
- climate-driven evolution (1)
- cluster model (1)
- clustering (1)
- coagulation-fragmentation (1)
- coarse-grained order parameter (1)
- coating (1)
- code (1)
- codifference (1)
- coefficient (1)
- coefficients (1)
- coherence (1)
- coherent phonons (1)
- coincidence (1)
- cold air outbreak (1)
- colloidal particles (1)
- coloured (1)
- coloured and quantum noise (1)
- coma (1)
- comb-like model (1)
- comets (1)
- comets: individual ((596) Scheila) (1)
- comets: individual: 67P (1)
- compacton (1)
- compatibilized filler molecules (1)
- complex (1)
- complex networks (1)
- compliant electrodes (1)
- components (1)
- computational biochemistry (1)
- concentration (1)
- concrete (1)
- conducting polymer (1)
- conducting polymers (1)
- conduction (1)
- confocal Raman microscopy (1)
- conformational analysis (1)
- conformational and hydrodynamic characteristics (1)
- conformational changes (1)
- conformational properties (1)
- connectivity (1)
- consecutive disasters (1)
- consequences (1)
- conservative random walks (1)
- contact resistance (1)
- continental rifting (1)
- continuous distribution model (1)
- continuous symmetries (1)
- continuous time random (1)
- continuous time random walks (1)
- contraction (1)
- convolutional neural networks (1)
- coordinate measurement machine (1)
- copper iodide (1)
- core-excited state dynamics (1)
- coronae (1)
- correlated noise (1)
- correlation functions (1)
- cortical network (1)
- cortical network models (1)
- cortical oscillations (1)
- cosmic ray propagation (1)
- cosmic ray theory (1)
- cosmological parameters (1)
- cosmology: cosmic background radiation (1)
- cosmology: cosmological parameters (1)
- cosmology: dark matter, large-scale structure of the Universe (1)
- cosmology: distance scale (1)
- cosmology: miscellaneous (1)
- cosmology: miscellaneous cosmology (1)
- costs (1)
- coupled climate model (1)
- coupled initial boundary value problem (1)
- coupling (1)
- coupling function (1)
- covariance (1)
- crack (1)
- critical adsorption (1)
- critical fluctuations (1)
- cross layer chip (1)
- cross-over effect (1)
- crosslinked poly(propylene) (1)
- crosslinking (1)
- crossover anomalous diffusion dynamics (1)
- crossover dynamics (1)
- crowding (1)
- cryolithology (1)
- crystal (1)
- crystal growth (1)
- crystal orientation (1)
- crystal structure (1)
- crystal texture (1)
- crystalline ordering (1)
- crystalline phases (1)
- crystallinity (1)
- crystallization (1)
- cultural heritage (1)
- current voltage analysis (1)
- cyclic voltammetry (1)
- damage evolution (1)
- damage quantification (1)
- dark energy theory (1)
- dark matter detectors (1)
- dark matter experiments (1)
- data based NARMAX modeling (1)
- data behind figure (1)
- data processing (1)
- decomposing anomalous diffusion (1)
- deep learning (1)
- defect detection (1)
- defects (1)
- degradation (1)
- delay differential equation (1)
- delay faults (1)
- delay-differential equation (1)
- delayed feedback (1)
- density functional calculations (1)
- density functional theory (1)
- dependent velocity (1)
- deposition (1)
- dermis (1)
- design for Testability (1)
- detection (1)
- detectors (1)
- diamagnetic currents (1)
- diaspora (1)
- dichalcogenides (1)
- dielectric (1)
- dielectric elastomer (1)
- dielectric hysteresis (1)
- dielectric polarisation (1)
- dielectric polymer (1)
- dielectric relaxation (1)
- dielectric resonance spectroscopy (1)
- dielectrics (1)
- differential scanning calorimetry (1)
- diffraction enhanced imaging (1)
- diffraction-elastic constants (1)
- diffusion coefficients (1)
- diffusion exponent (1)
- diffusion length (1)
- diffusion-controlled reactions (1)
- diffusion-influenced (1)
- diffusion-radation mechanisms (1)
- diffusion-wave equation (1)
- dimensional reduction (1)
- dipole grafting (1)
- directed transport (1)
- direction of optomechanical stress (1)
- diselenide (1)
- dislocations (1)
- disordered systems (theory) (1)
- dispersion (1)
- dispersion force (1)
- distortion (1)
- distribution (1)
- diurnal rhythm (1)
- doctor-blade coating (1)
- domain memory in polymer brushes (1)
- domain purity (1)
- domino effect (1)
- donor (1)
- donor-acceptor interfaces (1)
- double-layer (1)
- doubly transient chaos (1)
- drift length (1)
- drift-diffusion models (1)
- driven (1)
- driven diffusive systems (theory) (1)
- droughts (1)
- dub-ambient (1)
- durability (1)
- dynamic mechanical (1)
- dynamic structure factor (1)
- dynamical cluster (1)
- dynamical systems (1)
- dynamical transitions (1)
- dynamics simulation (1)
- dynamo (1)
- early warning indicators (1)
- ecological (1)
- ecology and biodiversity (1)
- economic network (1)
- economic ripple resonance (1)
- economic ripples (1)
- econophysics (1)
- effective polarization (1)
- efficiency (1)
- efficiency potentials (1)
- eingefrorene Energielandschaft (1)
- ejecta (1)
- elastic conductor (1)
- elastomers (1)
- electret polymers (1)
- electret stability (1)
- electric field noise (1)
- electric sensing devices (1)
- electrical breakdown (1)
- electrical polarization hysteresis (1)
- electricity consumption (1)
- electro-electrets (1)
- electro-fused zirconia (1)
- electro-mechanical transducers (1)
- electro-mechanically active polymers (1)
- electro-modulation microscopy (1)
- electro-optical materials (1)
- electroacoustic probing (1)
- electroanalysis (1)
- electrochemistry (1)
- electrodes (1)
- electromagnetic ion cyclotron waves (1)
- electromechanically active polymer (1)
- electron backscatter diffraction (EBSD) (1)
- electron contact (1)
- electron flux (1)
- electron flux forecasts (1)
- electron lifetimes (1)
- electron localization (1)
- electron microscopy (1)
- electron number density (1)
- electron spectroscopy (1)
- electron-phonon scattering (1)
- electron-transfer (1)
- electron-transport layers (1)
- electrostatic (1)
- elementary excitation (1)
- elevated-temperature effects on the operation of dielectric-elastomer (1)
- ellipsometry (1)
- embrittlement (1)
- emic waves (1)
- empirical modeling (1)
- empirical prediction (1)
- enacted PCK (1)
- energetic disorder (1)
- energetic disorders (1)
- energetic electrons (1)
- energetic offset (1)
- energetic particle (1)
- energy (1)
- energy gradients (1)
- energy losses (1)
- energy-level alignments (1)
- england (1)
- enhanced raman-scattering (1)
- ensemble (1)
- ensemble and time averaged mean squared displacement (1)
- entrance test (1)
- entropy production (1)
- enzymatic sensors (1)
- epidermis (1)
- epigenetics (1)
- epilepsy (1)
- epitaxial layers (1)
- equation (1)
- equation approach (1)
- equation of state (1)
- equation of state; (1)
- equatorial plasma depletions (1)
- equivalent-circuit (1)
- erasure (1)
- ergodicity (1)
- errata (1)
- evolution (1)
- exact results (1)
- exaction (1)
- excess energy (1)
- excited state proton transfer (1)
- excited state selectivity (1)
- excited-state proton-transfer (1)
- exciton dynamics (1)
- excitonic materials (1)
- exclusion process (1)
- exclusion processes (1)
- exoplanets (1)
- expanded polytetrafluoroethylene (1)
- expanding medium (1)
- experiments (1)
- exploit (1)
- explosives (1)
- external generation efficiency (1)
- external quantum efficiency (1)
- extraction (1)
- extraterrestrial intelligence (1)
- extremal values (1)
- extreme statistics (1)
- extreme weather (1)
- extrusion (1)
- fabric electrodes (1)
- far infrared (1)
- fastest first-passage time of N walkers (1)
- femtochemistry (1)
- femtosecond laser spectroscopy (1)
- femtosecond slicing (1)
- ferro- and piezoelectrets (1)
- ferroelectrets (1)
- ferroelectric and paraelectric phases (1)
- ferroelectric polymer (1)
- ferroelectric polymers (1)
- ferroelectric semiconductors (1)
- ferroelectric thin films (1)
- ferroelectricity and piezoelectricity in polymers (1)
- fiber optic sensors (1)
- fiber-electrophoresis chip (1)
- field experience (1)
- field line (1)
- field-aligned currents (1)
- field-effect (1)
- field-effect transistor (1)
- field-effect-transistor (1)
- fields (1)
- fill factor (1)
- fill factor losses (1)
- film (1)
- film sensor (1)
- finite-size effects (1)
- first arrival (1)
- first passage process (1)
- first star (1)
- first-arrival density (1)
- first-passage time distribution (1)
- first-passage times (1)
- first-reaction time (1)
- flagellum (1)
- flare - stars (1)
- flares (1)
- flashover (1)
- flexible (1)
- flexible tandem solar cells (1)
- flow (1)
- flow network (1)
- flow photolysis (1)
- fluctuating surfaces (1)
- fluctuation dissipation (1)
- fluctuation dissipation theorem (1)
- fluctuation forces (1)
- fluctuation phenomena (1)
- fluctuation relations (1)
- fluctuation-dissipation theorem (1)
- fluid shells (1)
- fluorinated ethylene-propylene copolymer (FEP) (1)
- fluorinated organic spacer (1)
- fluorination (1)
- food security (1)
- force methods (1)
- forces generated during surface relief grating formation (1)
- forecast (1)
- formal specification (1)
- formal verification (1)
- formation (1)
- fractional diffusion (1)
- fractional dynamic equations (1)
- fractional dynamics (1)
- fractional generalized Langevin equation (1)
- fractography (1)
- free electron lasers (1)
- free shear layers (1)
- free-electron laser (1)
- frequency response (1)
- friction (1)
- frictional memory kernel (1)
- fullerene (1)
- fullerenes (1)
- function (1)
- functional connectivity (1)
- functional materials (1)
- functional theory (1)
- fungus (1)
- galaxies: (1)
- galaxies: Local Group (1)
- galaxies: Seyfert (1)
- galaxies: active-galaxies: individual: PMN J0948+0022 (1)
- galaxies: clusters: individual (47 Tucanae) (1)
- galaxies: clusters: individual (Coma (ACO 1656)) (1)
- galaxies: clusters: intracluster medium (1)
- galaxies: distances and redshifts (1)
- galaxies: elliptical and lenticular, cD (1)
- galaxies: groups, clusters (1)
- galaxies: individual (1)
- galaxies: individual (B2 1215+30) (1)
- galaxies: individual (BL Lacertae, VER J2202+422) (1)
- galaxies: individual (Hydra II) (1)
- galaxies: individual (Large Magellanic Cloud, Small Magellanic Cloud) (1)
- galaxies: individual (M 87) (1)
- galaxies: individual (M 87, VER J1230+123) (1)
- galaxies: individual (Markarian 501) (1)
- galaxies: individual (RGB J2243+203) (1)
- galaxies: individual: 1ES 1741+196=VER J1744+195 (1)
- galaxies: individual: AM1353-272 B (1)
- galaxies: individual: Antennae Galaxy (1)
- galaxies: individual: ESO 338-4 (1)
- galaxies: individual: Magellanic Clouds (1)
- galaxies: individual: NGC 4038, NGC 4039 (1)
- galaxies: individual: PKS 0625-354 (1)
- galaxies: kinematics and dynamics (1)
- galaxies: magnetic (1)
- galaxies: star clusters (1)
- galaxies: star clusters: individual (1)
- galaxies:active (1)
- galaxies:distances and redshifts (1)
- galaxy evolution (1)
- galaxy: kinematics and dynamics (1)
- gamma ray detectors (1)
- gamma rays : stars (1)
- gamma rays: (1)
- gamma rays: diffuse (1)
- gamma rays: galaxies: clusters (1)
- gamma rays: general(HESS J0632+057, VER J0633+057) (1)
- gamma-ray burst: individual (GRB 130427A) (1)
- gamma-ray burst: individual (GRB 150323A) (1)
- gamma-ray burst: individual (GRB 170817A) (1)
- gamma-ray burst: individual (MGRO J1908+06, VER J1907+062) (1)
- gamma-ray burst: individual: GRB 100621A (1)
- gamma-ray bursts: general (1)
- gamma-ray polarization (1)
- gamma-rays: ISM (1)
- gamma-rays: stars (1)
- gas (1)
- gas chromatography (1)
- gas phase electron spectroscopy (1)
- gel network (1)
- gelatin (1)
- geminate recombination (1)
- gene regulatory networks (1)
- generalised Langevin equation (1)
- generalised langevin equation (1)
- generalized diffusion equation (1)
- generational comparison (1)
- genetic Allee effects (1)
- genetic networks (1)
- geomagnetic activity (1)
- geomagnetic activity dependence (1)
- geomagnetic storms (1)
- geometrical deformations (1)
- geostationary orbit (1)
- glacial-isostatic adjustment (1)
- glaciology (1)
- glassy systems (1)
- globular clusters: individual: (SMASH 1) (1)
- globular clusters: individual: 47 Tuc (1)
- globular clusters: individual: 47 Tucanae (1)
- globular clusters: individual: NGC 2808 (1)
- globular clusters: individual: NGC 3201 (1)
- globular clusters: individual: NGC 6656 (1)
- globular clusters: individual: NGC5139 (1)
- glycerol oxidation (1)
- gold cluster (1)
- gold intercalation (1)
- gold nanoflowers (1)
- gold nanoparticle (1)
- gradients (1)
- grafted polymers (1)
- granular gas (1)
- grating interferometry (1)
- gravitational-wave astronomy (1)
- guided self assembly (1)
- halo (1)
- haptic feedback (1)
- hatural language (1)
- healing (1)
- heart cycle (1)
- heart failure (1)
- heat diffusion (1)
- heat transfer (1)
- heat treatment (1)
- heat-treatment (1)
- heatwaves (1)
- heterogeneous catalysis (1)
- heterogeneous diffusion (1)
- heterogeneous diffusion process (1)
- heterogeneous ensemble of Brownian particles (1)
- heterogeneous media (1)
- heterojunction silicon solar cells (1)
- heterostructures (1)
- hierarchical modular networks (1)
- high field mobility (1)
- high impact polystyrene (1)
- high latitude (1)
- high performance polymers (1)
- high resolution spectroscopy (1)
- high strain rate (1)
- high temperature (1)
- high-energy astrophysical phenomena (1)
- high-frequency force (1)
- high-redshift (1)
- higher-order effects (1)
- histomorphometry (1)
- histone modifications (1)
- hole (1)
- hole extraction (1)
- hole selective materials (1)
- hopf-bifurcation (1)
- hopping dynamics (1)
- host-guest systems (1)
- human behaviour (1)
- humidity (1)
- hybrid functional (1)
- hybrid manufacturing (1)
- hybrid metal oxides (1)
- hybrid nanomaterials (1)
- hybrid simulations (1)
- hybrid synthesis (1)
- hydrochemistry (1)
- hydrodynamic model (1)
- hydrogels (1)
- hydrogen (1)
- hydrogen bonds (1)
- hydrogen evolution reaction (1)
- ice clouds (1)
- ice-sheet (1)
- iceberg calving (1)
- image processing (1)
- image registration (1)
- imaging (1)
- imidazolium (1)
- immunosensors (1)
- impacts (1)
- impedance spectroscopy (1)
- imprinted electrodes (1)
- in situ atomic force microscopy (1)
- in situ monitoring (1)
- in situ thermography (1)
- incoherent light (1)
- incoherent radiation (1)
- income inequality (1)
- income mobility (1)
- individual: CU Vir (1)
- individual: NGC1501 (1)
- indomethacin (1)
- induced deformation (1)
- influence of weak magnetic fields on living systems (1)
- information (1)
- information theory (1)
- infrared: ISM (1)
- infrared: general (1)
- infrared: planetary systems (1)
- injection (1)
- inner radiation zone and slot region (1)
- instability control (1)
- instructional (1)
- instructional explanation (1)
- instrumentation: adaptive optics (1)
- instrumentation: miscellaneous (1)
- integrability (1)
- integrierter Spektrograph (1)
- interaction parameter (1)
- interface engineering (1)
- interfaces (1)
- interfacial layers (1)
- interference pattern (1)
- interferometry (1)
- interiors (1)
- interlayer time (1)
- intermittency (1)
- intermolecular force (1)
- international migration (1)
- interoception (1)
- interoceptive sensitivity (1)
- interspecific competition (1)
- interstellar matter (1)
- interstellar medium (1)
- intersystem crossing (1)
- intrinsic neuronal diversity (1)
- inverse analysis (1)
- inversion (1)
- ion channels (1)
- ion migration (1)
- ion optics (1)
- ion trap (1)
- ionic conductivity (1)
- ionic crosslinking (1)
- ionic liquid (1)
- ionic liquids (1)
- ionogels (1)
- ionosphere interactions (1)
- iron cyanides (1)
- irregular firing activity (1)
- isostatic rebound (1)
- iteration method (1)
- jet stream (1)
- jump detection (1)
- keratocytle-like motility (1)
- kesterite (1)
- kinetic Alfven (1)
- kinetic of cis-trans isomerization (1)
- kinetic theory (1)
- kinetic-theory (1)
- kinetics (1)
- kink instability (1)
- label-free detection (1)
- laboratory x-ray diffraction (1)
- lake shorelines (1)
- large area devices (1)
- large deviation function (1)
- large deviation theory (1)
- large-deviation statistic (1)
- large-scale structure of universe (1)
- large-scale system (1)
- laser illumination (1)
- laser powder bed fusion (1)
- laser powder bed fusion (L-PBF) (1)
- laser powder bed fusions (1)
- laser-based additive manufacturing (1)
- lattice gas (1)
- lattice structures (1)
- lattices (1)
- lead halide perovskite (1)
- lead halide perovskite films (1)
- lead halide perovskites (LHP) (1)
- leakage scheme (1)
- lesson planning (1)
- lidar (1)
- life history evolution (1)
- lifetime (1)
- lifetime‐ mobility product (1)
- light driven reversible change of surface topography and thickness (1)
- light emission (1)
- light management (1)
- light photocontrol (1)
- light polarisation (1)
- light responsive DNA (1)
- light responsive microgels (1)
- light responsive polymer brushes (1)
- light-driven diffusioosmosis (1)
- light-emitting diodes (1)
- light-induced DNA de-compaction (1)
- light-induced mass transport (1)
- line: formation (1)
- linear cellular automaton (1)
- linear response theory (1)
- linear stability analysis (1)
- linker histones (1)
- liposomes (1)
- liquid crystal (1)
- liquid crystal alignment (1)
- liquid crystal polymers (1)
- literature review (1)
- living cells (1)
- local (1)
- local equilibrium (1)
- local insterstellar matter (1)
- local seismicity (1)
- localization microscopy (1)
- longitudinal study (1)
- loss (1)
- loss propagation (1)
- low donor content (1)
- low-dimensional models (1)
- low-frequency force (1)
- magnetic beads (1)
- magnetic field (1)
- magnetic fields - methods (1)
- magnetic microstructures (1)
- magnetic nanoparticles (1)
- magnetic pressure (1)
- magnetic proximity effect (1)
- magnetic stray field (1)
- magnetisation (1)
- magnetism (1)
- magnetohydrodynamics (1)
- magnetosonic (1)
- magnetosonic equatorial noise (1)
- magnetospheric average ion mass (1)
- magnetospheric plasma spatial (1)
- man-made dipole (1)
- manipulation (1)
- manufacturing (AM) (1)
- manufacturing automation (1)
- marine ice-sheet instability (1)
- masers (1)
- mass (1)
- mass conservation (1)
- mass spectrometry (1)
- mass-transport (1)
- massive stars (1)
- master (1)
- material (1)
- matrix composites (1)
- maximum and range (1)
- maximum entropy analysis (1)
- mean residence time (1)
- mean square displacement (1)
- mean squared displacement (1)
- mean versus most probable reaction times (1)
- mean-field model (1)
- mechanical effects of light (1)
- mechanisms (1)
- mechano-chemical coupling and thermodynamic efficiency (1)
- melt-quench-anneal (1)
- melting slm (1)
- membrane channel (1)
- memory kernel (1)
- mesocrystals (1)
- mesoporous silicon (1)
- metabolic regulation (1)
- metabolomics (1)
- metal halide perovskites (1)
- metal matrix composite (1)
- metal nanoparticles (1)
- metal optics (1)
- metal oxide (1)
- metal-free photocatalysis (1)
- metal/multilayered graphene/polymer interfaces (1)
- metal/polymer interface (1)
- methane localization (1)
- methods (1)
- methods: Data analysis (1)
- methods: MHD (1)
- methods: Observational (1)
- micelles (1)
- micro computed tomography (XCT) (1)
- micro-energy harvesting (1)
- microchannel (1)
- microfluidic paper analytic device (mu PAD) (1)
- microfluidics (1)
- microgel (1)
- microstructure-property relations (1)
- microtransport and -assembly (1)
- mid-temperature transition(s) (1)
- migration (1)
- migration transition (1)
- milton rd (1)
- minor planets, asteroids: general (1)
- mixed boundary conditions (1)
- mixed domains (1)
- mobile ions (1)
- mobile-immobile model (1)
- modes of (1)
- modified electrode (1)
- modified gravity (1)
- modular logic programs (1)
- molar mass distribution (1)
- mold (1)
- molecular and Brownian motors (1)
- molecular bottle brushes (1)
- molecular brushes (1)
- molecular conformation (1)
- molecular crystals (1)
- molecular doping (1)
- molecular dynamics (1)
- molecular dynamics method (1)
- molecular hydrodynamics and (1)
- molecular imprinted polymers (1)
- molecular overcrowding (1)
- molecular proton dynamics (1)
- molecular weight (1)
- molecular weight distribution (1)
- molecules (1)
- molten sulfur (1)
- molybdenum oxide (1)
- monitoring (1)
- monolayer (1)
- monsoon (1)
- monsoon failure (1)
- monte-carlo (1)
- moon absorption (1)
- motion (1)
- motion of adsorbed nano-particles (1)
- motion registration (1)
- movement data (1)
- mu CT imaging (1)
- multi-layer systems (1)
- multi-messenger astrophysics (1)
- multi-scaling (1)
- multi-stakeholder (1)
- multichannel (1)
- multichannel Raman spectroscopy (1)
- multidimensional fractional diffusion equation (1)
- multilayer graphene deformation (1)
- multiple (1)
- multiplicative noise (1)
- mushroom instability (1)
- myosin II (1)
- nano-object motion (1)
- nanoclusters (1)
- nanofiber (1)
- nanoplate capacitor (1)
- nanoscale energy transports (1)
- nanoscale friction and thermal noise (1)
- nanoscale heat transfer (1)
- nanoscale modeling (1)
- nanostructured metal surface (1)
- nanostructures (1)
- naphthalenediimide (1)
- narrow escape problem (1)
- natriuretic peptide system (1)
- natural disasters (1)
- natural resources (biological and non-biological) (1)
- near-ambient pressure X-ray photoelectron spectroscopy (1)
- near-ambient pressure x-ray photoelectron spectroscopy (1)
- nebulae: general (1)
- negative thermal expansion (1)
- network (1)
- network dynamics (1)
- network reconstruction (1)
- neural (1)
- neural synchonization (1)
- neutron (1)
- neutron powder diffraction (1)
- neutron resonance spin-echo spectroscopy (1)
- neutron spin-echo (1)
- neutron star mergers (1)
- neutron stars (1)
- neutrophils (1)
- noise in biochemical signalling (1)
- non-Gaussian (1)
- non-Gaussian diffusion (1)
- non-Gaussian distribution (1)
- non-Gaussian probability (1)
- non-Gaussianity (1)
- non-Langevin reduction factors (1)
- non-Markovian dynamics (1)
- non-contact heat transfer (1)
- non-destructive evaluation (1)
- non-equilibrium steady state (1)
- non-ergodicity (1)
- non-exponential relaxation (1)
- non-exponential statistics (1)
- non-extensive statistics (1)
- non-geminate recombination (1)
- non-halogenated solvents (1)
- non-integer dimension (1)
- non-local field theory (1)
- non-radiative interface recombination (1)
- non-radiative recombination (1)
- non-thermal-pulsars (1)
- nonadaptive evolution (1)
- nondestructive testing (1)
- nonequilibrium (1)
- nonequilibrium electrodynamics of nanosystems (1)
- nonequilibrium physics (1)
- nonequilibrium stationary state (1)
- nonlinear dynamical systems (1)
- nonlinear frequency conversion (1)
- nonlinear lattice (1)
- nonlinear microscopy (1)
- nonlinear time series analysis (1)
- nonlinear waves (1)
- nonlocal coupled oscillators (1)
- nonradiative losses (1)
- nonstationary diffusivity (1)
- nonsymmetric linear-systems (1)
- novae (1)
- nucleation (1)
- nucleobase (1)
- nucleobases (1)
- number (1)
- numerical ice modeling (1)
- numerical schemes (1)
- numerical simulations (1)
- observations (1)
- observatory (1)
- ocean-atmosphere energy exchange (1)
- onset (1)
- opacity (1)
- open cluster and associations: individual: Quintuplet (1)
- open clusters and associations: individual (Cl Bochum 10, Cl Bochum 11, Cl Collinder 228, Cl Trumpler 14, Cl Trumpler 15, Cl Trumpler 16) (1)
- open clusters and associations: individual (NGC 602) (1)
- open clusters and associations: individual (Trumpler 16) (1)
- open clusters and associations: individual: (1)
- open clusters and associations: individual: Quintuplet (1)
- open clusters and associations: individual: Trapezium cluster (1)
- open quantum system (1)
- open quantum systems (1)
- open-circuit voltage decay (1)
- optical feedback (1)
- optical fiber bundle (1)
- optical hole burning (1)
- optical interconnections (1)
- optical pump (1)
- optical pump - X-ray probe spectroscopy (1)
- optical pump X-ray probe (1)
- optical simulations (1)
- optical spectroscopy (1)
- optical tomography (1)
- option pricing (1)
- opto-mechanical stresses (1)
- optomechanical forces (1)
- optoplasmonic (1)
- organic (1)
- organic field-effect transistors (1)
- organic interfaces (1)
- organic light-emitting diode (1)
- organic semiconductors; (1)
- organic solar cell (1)
- organic thermoelectrics (1)
- organohalide lead perovskites (1)
- orientation (1)
- orientation approaches (1)
- orientation of azobenzenes in polymer brushes (1)
- origins (1)
- oscillator populations (1)
- osmotic-pressure (1)
- osteoporosis (1)
- outflows X-rays: binaries (1)
- outflows; (1)
- overdamped brownian systems (1)
- oxidation state (1)
- oxygen plasma (1)
- oxygen quenching (1)
- oxygen torus (1)
- oxygen/Ag(111) (1)
- p-type (1)
- packaging (1)
- parameter (1)
- parameter inference (1)
- partial synchronization (1)
- particle morphology (1)
- particle physics - cosmology connection (1)
- particles (1)
- passivation (1)
- path integration (1)
- patient immobilization (1)
- patterning glass microfiber (1)
- patterns (1)
- pause hiatus (1)
- peak load (1)
- pedagogical content knowledge (1)
- pedagogical content knowledge (PCK) (1)
- pedagogical reasoning (1)
- percolation threshold (1)
- performance assessment (1)
- period doubling (1)
- periodically poled material (1)
- perovskite (1)
- perovskite semiconductors (1)
- perovskites (1)
- persistence (1)
- perturbation approach (1)
- perturbation theory (1)
- phase approximation (1)
- phase diagram (1)
- phase diffusion (1)
- phase field model (1)
- phase grating (1)
- phase lag (1)
- phase oscillator (1)
- phase oscillators (1)
- phase purity (1)
- phase response curve (1)
- phase-transition boundary (1)
- phonon (1)
- phonon dispersion relations (1)
- phospholipid membranes (1)
- phosphonic acid (1)
- photo-chemical pathways (1)
- photo-isomerization kinetics (1)
- photo-sensitive surfactant (1)
- photocontrol (1)
- photodissociation region (PDR) (1)
- photoelectrochemistry (1)
- photoexcited hole transfer (1)
- photofragmentation (1)
- photoisomerization (1)
- photometric (1)
- photon recycling (1)
- photon statistics (1)
- photonic bandgap (1)
- photonic crystal fibers (1)
- photophysics (1)
- photosensitive brushes (1)
- photosensitive polymer films (1)
- photosensitive polymers (1)
- photosensitive soft objects (1)
- photosphere (1)
- photostability (1)
- photoswitches (1)
- photosynthesis (1)
- photothermal conversion (1)
- physical activity (1)
- physical hydrogels (1)
- physics (1)
- physics education (1)
- picosecond ultrasonics (1)
- piezoelectric measurements (1)
- piezoelectric nanogenerator (PENG) (1)
- piezoelectric polymers (1)
- piezoelectricity-polarization relation (1)
- pitch angle distributions (1)
- pitch angle scattering (1)
- planar lightwave circuit (1)
- planare Lichtwellenleiter (1)
- planet (1)
- planetary (1)
- planetary nebulae (1)
- planetary nebulae: general; (1)
- planetary nebulae: individual (A30 and A78) (1)
- planetary nebulae: individual (A30) (1)
- planetary nebulae: individual (A78) (1)
- planetary nebulae: individual: Abell 48 (1)
- planetary nebulae: individual: Hen 2-84 (1)
- planetary nebulae: individual: IC4406 (1)
- planetary nebulae: individual: NGC40 (1)
- planetary nebulae: individual: PN G029.0+00.4 (1)
- planetary nebulae: individual: Stingray nebula (Henize 3-1357) (1)
- planetary nebulae: individual: SwSt1 (1)
- planets (1)
- planets and (1)
- planets and satellites (1)
- planets and satellites: composition (1)
- planets and satellites: detection (1)
- planets and satellites: dynamical evolution and stability (1)
- planets and satellites: gaseous (1)
- planets and satellites: individual: AU Mic b (1)
- planets and satellites: individual: Jupiter (1)
- plasma flows (1)
- plasma pressure (1)
- plasmasphere (1)
- plasmaspheric plume (1)
- plasmonics (1)
- pnCCD (1)
- polarized radiation (1)
- policies (1)
- politics (1)
- poly (acrylic acid, sodium salt) (1)
- poly(gamma-benzyl L-glutamate) (1)
- poly(heptazine imide) (1)
- poly(vinylidenefluoride-trifluoroethylene) P(VDF-TrFE) (1)
- polyelectrolyte layer (1)
- polyelectrolytes (1)
- polyethylene naphthalate (PEN) (1)
- polymer ferroelectrets (1)
- polymer films (1)
- polymer translocation (1)
- polymer-foam films (1)
- polymer:fullerene bulk heterojunction (1)
- polymerase chain reaction (PCR) (1)
- polypropylene (1)
- polypyrrole (1)
- polytetrafluoroethylene (1)
- polytetrafluoroethylene (PTFE) (1)
- polyurethanes (1)
- populations (1)
- pore orientation (1)
- porphyrin (1)
- position control (1)
- positioning (1)
- posttranslational protein translocation (1)
- potential ene rgy surface (1)
- potential landscape (1)
- power conversion efficiency (1)
- power law and power-law breakdown (1)
- power spectral density (1)
- power spectrum (1)
- practicum (1)
- pre-main sequence stars (1)
- pre-service teachers (1)
- predator-prey model (1)
- prediction (1)
- preferred orientation (1)
- pressure (1)
- principal stress components (1)
- printed electroacoustic thin-film transducers (1)
- printing (1)
- probabilistic inference (1)
- process (1)
- process inference (1)
- process monitoring (1)
- projections (1)
- prominences (1)
- propagating surface plasmons (1)
- proper motion (1)
- proteasome (1)
- protein folding (1)
- protein translocation (1)
- proteins (1)
- protonation (1)
- protons (1)
- protostars (1)
- pulsars : individual (PSR J2021+3651) (1)
- pulsars: individual (PSR J0633+1746, Geminga) (1)
- pulsars: individual (PSR J1023+0038) (1)
- pulsars: individual (PSR J1907+0602) (1)
- pulsars: individual (PSR J2032+4127) (1)
- pulsars: individual (PSR J2032+4127, VER J2032+414, MAGIC J2032+4127) (1)
- pulsars: individual: 4U0114+65 (1)
- pulsars: individual: B0531+21 (1)
- pulsars: individual: LS V+22 25 (1)
- pulsars: individual: PSR B0656+14 (1)
- pulsars: individual: PSR B1259-63 (1)
- pulsars: individual: SXP 1062 (1)
- pulsars: individual: SXP1062 (1)
- pulsars: individual: rho Ophiuchi A (1)
- pulse compression (1)
- pulse front matching (1)
- pulse shortening (1)
- pure aluminium (1)
- purification (1)
- pyroelectric polymers (1)
- pyroelectricity (1)
- quality (1)
- quantum (1)
- quantum batteries (1)
- quantum correlations (1)
- quantum effects (1)
- quantum electrodynamics (1)
- quantum eraser (1)
- quantum gas (1)
- quantum gases (1)
- quantum gravity (1)
- quantum mechanics (1)
- quantum optics (1)
- quantum phase transition (1)
- quantum regression theorem (1)
- quasar: absorption line (1)
- quasars: (1)
- quasars: emission lines (1)
- quasars: individual (PKS 0405-123) (1)
- quasars: individual (SDSS J092447.36+485242.8, SDSS J110155.74+105302.3) (1)
- quasars: individual (SDSS J142253.31-000149) (1)
- quasars: individual (SDSS J213748+001220, SDSS J215200+062516) (1)
- quasars: individual: 3C 279 (1)
- quasars: individual: HE 0027-1836 (1)
- quasars: individual: HE 2217-2818 (1)
- quasars: individual: HS 1549+1919 (1)
- quasars: individual: LBQS 0302-0018 (1)
- quasars: individual: LBQS 0302-0019 (1)
- quasars: individual: PKS 0208-512 (1)
- quasars: individual: PKS 1510-089 (1)
- quasars: individual: PKS1127-145 (1)
- quasars: individual: QSO 0347-383 (1)
- quasars: supermassive black holes (1)
- quasi-Fermi level (1)
- quasi-free-standing graphene (1)
- quasi-particle interaction (1)
- quasi-particles (1)
- quasi-periodic oscillation (1)
- quasi-steady-state photoinduced absorptions (1)
- quenching (1)
- quorum sensing (1)
- r and K selection (1)
- radiation belt (1)
- radiation belt electrons (1)
- radiation belt forecasts (1)
- radiation pressure (1)
- radiation: dynamics (1)
- radiative limit (1)
- radio continuum: ISM (1)
- radio continuum: galaxies (1)
- radio continuum: general (1)
- radiography (1)
- random copolymer (1)
- random processes (1)
- random search process (1)
- random search processes (1)
- random walk (1)
- random-walk (1)
- random-walks (1)
- rare earth (1)
- rare events (1)
- ratchets (1)
- rate constants (1)
- rate of (1)
- rays: stars (1)
- reaction cascade (1)
- reaction rate constants (1)
- reaction-advection-diffusion equation (1)
- reaction-diffusion models (1)
- reaction-diffusion system (1)
- reactions (1)
- reanalysis (1)
- recombination losses (1)
- recombinations (1)
- recrystallization (1)
- rectification (1)
- recurrence (1)
- recurrence plot (1)
- refined consensus model (RCM) (1)
- reflected Brownian motion (1)
- reflecting boundary conditions (1)
- reflection (1)
- regular planar architecture (1)
- relationships (1)
- relative total electron content (1)
- relativistic electron precipitation (1)
- relaxation dynamics (1)
- relaxor-ferroelectric polymers (1)
- remanent polarisation (1)
- remodelers (1)
- repercussion resonance (1)
- repertory grid (1)
- reproduction (1)
- resetting (1)
- residual stress analysis (1)
- resolution matrix (1)
- resonances (1)
- resonant X-ray scattering (1)
- resonant inelastic X-ray scattering (1)
- resonant inelastic x-ray scattering (1)
- return migration (1)
- reversible binding (1)
- ribosome assembly (1)
- ring (1)
- ring current electrons (1)
- ring current model (1)
- river dynamics on glacial timescales (1)
- river floods (1)
- rock (1)
- rotation curves of galaxies (1)
- rotational diffusion (1)
- roughness (1)
- royal soc chemistry (1)
- run and tumble (1)
- sagittal X-ray diffraction (1)
- satellites: atmospheres (1)
- scalar fields (1)
- scanning tunneling microscopy (1)
- scanning tunneling spectroscopy (1)
- school (1)
- school internship (1)
- science park (1)
- science teaching (1)
- screen (1)
- screen-printed (1)
- sea level (1)
- sea-level (1)
- sea-level change (1)
- search dynamics (1)
- search efficiency (1)
- search optimization (1)
- seasonal cyclone activity forecasts (1)
- segmentations (1)
- seismogenic zone (1)
- selective bond cleavage (1)
- selective contact (1)
- self-assembled monolayers (1)
- self-organisation (1)
- self-similarity (1)
- self-sustained activity (1)
- self-sustained oscillations (1)
- semiconducting polymers (1)
- semiconductor lasers (1)
- sensing skin (1)
- seperation (1)
- sequence-controlled polymers (1)
- shear layers (1)
- shell-like geometries (1)
- shifts (1)
- shock (1)
- signal processing (1)
- silica-on-silicon (1)
- silicon (1)
- silicone based dielectric elastomer actuators (1)
- silicone-based dielectric elastomer actuators (1)
- silver (1)
- silver nanoslits (1)
- simulation model (1)
- simulations (1)
- single chain folding (1)
- single particle tracking (1)
- single trajectories (1)
- single trajectory analysis (1)
- single-cell analysis (1)
- single-file diffusion (1)
- single-file motion (1)
- single-molecule (1)
- single-particle tracking (1)
- single-stranded-dna (1)
- single-trajectory analysis (1)
- sintering (1)
- skutterudite (1)
- small molecules (1)
- small ring systems (1)
- soft X-ray (1)
- soft X-ray absorption (1)
- soft X-ray beamline (1)
- soft X-ray spectroscopy (1)
- soft elastomeric capacitor (1)
- soft electrical connections (1)
- soft electro-active materials (1)
- soft matter (1)
- software: data analysis (1)
- software: simulations (1)
- solar chromosphere (1)
- solar coronal mass ejections (1)
- solar filament eruptions (1)
- solar storm (1)
- solar wind dependence (1)
- solid-state nanopores (1)
- solitary wave (1)
- soliton (1)
- solubility test (1)
- solvation (1)
- solvent vapor annealing (1)
- space charge (1)
- space mission (1)
- space-charge and polarization profiles (1)
- space-charge effects (1)
- space-dependent diffusivity (1)
- space-time fractional diffusion equation (1)
- spacing (1)
- spark plasma (1)
- spatial (1)
- spatial localization (1)
- spatial poisson distribution (1)
- spatiotemporal phenomena (1)
- special quasirandom structure (1)
- spectral triple (1)
- spectroelectrochemistry (1)
- spectrometry (1)
- spectroscopic (1)
- spectroscopic - astronomical databases (1)
- spin coating (1)
- spin foam models (1)
- spin glass (1)
- spin state (1)
- spin- and angle-resolved photoemission (1)
- spin-crossover (1)
- spin-dependent forces (1)
- spin-orbit coupling (1)
- spin-related factors (1)
- spin-resolved (1)
- spiro-OMeTAD (1)
- splitting (1)
- spontaneous emission (1)
- spontaneous parametric down conversion (1)
- spontaneous parametric down-conversion (1)
- spread F (1)
- stability (1)
- stability analysis (1)
- stable water isotopes (1)
- standard (1)
- star formation (1)
- star interactions (1)
- stars : Wolf-Rayet (1)
- stars : atmospheres (1)
- stars : early-type (1)
- stars : evolution (1)
- stars : individual : xi Per (1)
- stars : individual : zeta Oph (1)
- stars : individual : zeta Ori (1)
- stars : individual : zeta Pup (1)
- stars : mass-loss (1)
- stars : winds, outflows (1)
- stars evolution (1)
- stars: Wolf (1)
- stars: Wolft-Rayet (1)
- stars: binaries (1)
- stars: binaries: spectroscopic (1)
- stars: carbon (1)
- stars: circumstellar matter (1)
- stars: early type (1)
- stars: early-typeP (1)
- stars: earlytype (1)
- stars: horizontal branch (1)
- stars: individual ( KIC 8462852) (1)
- stars: individual (1A 0535+262) (1)
- stars: individual (AH Cep, CW Cep) (1)
- stars: individual (Cyg OB2 12) (1)
- stars: individual (Delta Ori) (1)
- stars: individual (HD 54879) (1)
- stars: individual (HD 93250, HD 93129A, HD 93403, HD 93205, HD 93343, QZ Car, SS73 24, FO 15, Cl Trumpler 16 22, CPD-59 2610, HD 93501) (1)
- stars: individual (LS I+61 degrees 303, VER J0240+612) (1)
- stars: individual (MT91 213) (1)
- stars: individual (PHL 457, EQ Psc) (1)
- stars: individual (QV Nor, 4U1538+52) (1)
- stars: individual (Sanduleak 183) (1)
- stars: individual (delta Ori A) (1)
- stars: individual (mu Col) (1)
- stars: individual (zeta Oph, BD+43 degrees 3654) (1)
- stars: individual (zeta Pup) (1)
- stars: individual (zetaPup) (1)
- stars: individual: 1FGL J1018.6-5856 (1)
- stars: individual: 4U1700-37 (1)
- stars: individual: AM CVn (1)
- stars: individual: AU Mic (1)
- stars: individual: CPD-28 degrees 2561 (1)
- stars: individual: CPD-57 degrees 3509 (1)
- stars: individual: DGCVn-gamma rays: stars (1)
- stars: individual: EC 22536-5304 (1)
- stars: individual: Feige 46 (1)
- stars: individual: GALEX J015054.4+310745 (1)
- stars: individual: HD 137366 (1)
- stars: individual: HD 164492C (1)
- stars: individual: HD 23478 (1)
- stars: individual: HD 345439 (1)
- stars: individual: HD 54879 (1)
- stars: individual: HD 63425 (1)
- stars: individual: HD 66665 (1)
- stars: individual: HD 93129A (1)
- stars: individual: HD142301 (1)
- stars: individual: HR 5907 (1)
- stars: individual: HR 7355 (1)
- stars: individual: Hen 3-1383 (1)
- stars: individual: K2-133 (1)
- stars: individual: LP 358-499 (1)
- stars: individual: LP 40-365 (1)
- stars: individual: LS 2883 (1)
- stars: individual: PG 1610+062 (1)
- stars: individual: R 145 (1)
- stars: individual: RE 0457-281 (1)
- stars: individual: RE 0503-289 (1)
- stars: individual: Rho Ophiuchi (1)
- stars: individual: SAO 244567 (1)
- stars: individual: SMC AB 6 (1)
- stars: individual: V1298 Tau (1)
- stars: individual: WD0402+607 (1)
- stars: individual: WD1751+106 (1)
- stars: individual: WD2134+125 (1)
- stars: individual: WR 134 (1)
- stars: individual: WR 137 (1)
- stars: individual: WR 138 (1)
- stars: individual: WR 148 (1)
- stars: individual: WR 6 (1)
- stars: individual: WR 7 (1)
- stars: individual: X1908+075 (1)
- stars: individual: [MA93] 1393 (1)
- stars: individual: beta CMa (1)
- stars: individual: epsilon CMa (1)
- stars: individual: gamma(2) Vel (1)
- stars: individual: red clump stars (1)
- stars: individual: xi Persei (1)
- stars: individual: zeta Ophiuchi (1)
- stars: kinematics (1)
- stars: luminosity function, mass function (1)
- stars: magnetars (1)
- stars: oscillations (including pulsations) (1)
- stars: statistics (1)
- stars: subdwarfs (1)
- stars: variables: RR Lyrae (1)
- static-pressure dependence (1)
- stationarity (1)
- stationary stochastic process (1)
- steady‐ state photoconductance (1)
- steel and concrete structures (1)
- stellar content (1)
- stellar coronal mass ejections (1)
- stilbene oxide (1)
- stimuli-responsive structured polymer films (1)
- stochastic dynamics (1)
- stochastic model (1)
- stochastic particle dynamics (theory) (1)
- stochastic process (1)
- stochastic quench (1)
- stochastic resonance (1)
- stochastics (1)
- strain gauges (1)
- strain monitoring (1)
- strain sensors (1)
- strain-free lattice (1)
- stratosphere (1)
- stratospheric polar vortex (1)
- stress exponent (1)
- stress recovery (1)
- stress-relaxation (1)
- stretchability (1)
- stretchable electronics (1)
- stretchable sensor (1)
- stretching (1)
- structure analysis (1)
- structure of water (1)
- structure-property (1)
- structured polynucleotides (1)
- stuck-at faults (1)
- sub-T-g relaxations (1)
- subduction zone (1)
- subgrain structure (1)
- subseasonal predictions (1)
- substitution system (1)
- sudden stratosphere warming (1)
- sun (1)
- superdiffusion and (1)
- superluminescent diodes (1)
- supernovae : individual (CTB 87) (1)
- supernovae: individual (G0.9+0.1) (1)
- supernovae: individual: HESS J1818-154 (1)
- supersymmetry and cosmology (1)
- supply chains (1)
- supply network (1)
- supramolecular chemistry (1)
- surface Brillouin zone (SBZ) (1)
- surface acoustic waves (1)
- surface band bending (1)
- surface charge (1)
- surface charge stability (1)
- surface cracks (1)
- surface deformation (1)
- surface hopping (1)
- surface morphology (1)
- surface photovoltage (1)
- surface plasm on polaritons (1)
- surface plasmon (1)
- surface reactivity (1)
- surface recombination (1)
- surface reconstruction (1)
- surface states (1)
- surface tension (1)
- surface wetting (1)
- surface-enhanced infrared absorption spectroscopy (1)
- surface-relief gratings (1)
- surface-roughened (1)
- surfactant (1)
- surfactants (1)
- susceptibility (1)
- synchrotron X-ray refraction (1)
- synchrotron imaging (1)
- synchrotron x-ray refraction radiography (SXRR) (1)
- synthetic extruded cordierite (1)
- systems biology (1)
- systems subjected to parameter drift (1)
- table-top sources (1)
- tandem solar cells (1)
- tau proteins (1)
- teacher education (1)
- teacher professional development (1)
- teaching practice (1)
- techniques: Image processing (1)
- techniques: high angular resolution (1)
- telegrapher's equation (1)
- telescopes (1)
- telluride (1)
- tellurium (1)
- temperature fluctuation (1)
- terahertz waves (1)
- ternary (1)
- ternary blends (1)
- the Weibel instability (1)
- the sun (1)
- thermal barrier coatings (1)
- thermal conductivity (1)
- thermal stability (1)
- thermal stimulation of (1)
- thermal-convection (1)
- thermally enhanced actuators (1)
- thermally stimulated depolarization current (1)
- thermo-acoustic ultrasound emitter (1)
- thermoactivational spectroscopy (1)
- thermodynamic control (1)
- thermodynamic efficiency (1)
- thermodynamic length (1)
- thermodynamics (1)
- thermoelectric materials (1)
- thermoelectric properties (1)
- thermoelectrics (1)
- theta neurons (1)
- thickness insensitive active layers (1)
- thin film (1)
- thin film devices (1)
- thin-film actuators (1)
- thin-film solar cells (1)
- thin-films (1)
- thiophene (1)
- thiouracil (1)
- thomas graham house (1)
- threshold voltages (1)
- time (1)
- time interval reproduction (1)
- time series analysis (1)
- time-averaged mean squared displacement (1)
- time-domain astronomy (1)
- time-fractional Schrödinger equation (1)
- time-resolved (1)
- time-resolved X-ray probing (1)
- time-resolved photoemission (1)
- timing resilient design (1)
- tipping cascade (1)
- tipping elements (1)
- tipping interactions (1)
- tipping point (1)
- tissue engineering (1)
- tissue growth (1)
- tomography (1)
- tomography (XCT) (1)
- topological community (1)
- topologically associated domains (1)
- tracking (1)
- trade shocks (1)
- tranfer excited-state (1)
- transducer (1)
- transfer dynamics (1)
- transfer function (1)
- transient absorption spectroscopy (1)
- transient grating spectroscopy (1)
- transient spectroscopy (1)
- transit migration (1)
- transition metal complexes (1)
- transition radiation (1)
- transparent conductors (1)
- transport layer (1)
- transport layers (1)
- transport properties (1)
- transports (1)
- transversal instabilities (1)
- traveling waves (1)
- triaxial residual stresses (1)
- triple-axis spectroscopy (1)
- triple-cation perovskite (1)
- triplet excited states (1)
- tubular-channel polymer systems (1)
- tunnel barrier (1)
- tunneling (1)
- turbulence control (1)
- turbulent transport (1)
- twisted state (1)
- two beam interferometry (1)
- ultracold atoms (1)
- ultrafast (1)
- ultrafast molecular dynamics (1)
- ultrafast optics (1)
- ultrafast phenomena (1)
- ultrafast photoacoustics (1)
- ultrafast photochemistry (1)
- ultrafast spectroscopy (1)
- ultrafast x-ray diffraction (1)
- ultrarelativistic electrons (1)
- ultraviolet photoelectron spectroscopy (1)
- ultraviolet: general (1)
- uniform spatial arrangement (1)
- up-down states (1)
- upconversion (1)
- upconversion nanoparticles (1)
- vacuum fields (1)
- valence band (VB) (1)
- valence band maximum (VBM) (1)
- van Hove correlation (1)
- van alien probes (1)
- van allen probes (RBSP) (1)
- van allen probes; (1)
- van der Waals interaction (1)
- variability (1)
- variances (1)
- verb (1)
- verb simulations; (1)
- vibration monitoring (1)
- vibrational resonance (1)
- vibrational spectroscopy (1)
- vinylidenefluoride (VDF)-based polymers (1)
- vinylidenefluoride(VDF)-based polymers (1)
- virtual observatory tools (1)
- viscoelastic effects and anomalous diffusion (1)
- viscoelasticity and memory effects (1)
- viscosity (1)
- visibility (1)
- walks (1)
- water (1)
- water diffusion in the brain (1)
- water ice (1)
- water reduction reactions (1)
- water-interface (1)
- water-methane films (1)
- wave particle interaction (1)
- wave-particle dualism (1)
- wave-particle interactions (1)
- waveguides (1)
- wavelength (1)
- wearable (1)
- wearable electronics (1)
- weather (1)
- weather extremes (1)
- whispering gallery modes (1)
- wide-bandgap (1)
- winter circulation (1)
- x-ray diffraction (1)
- x-ray free-electron lasers (1)
- x-ray photoemission (1)
- x-ray spectroscopies and phenomena (1)
- x-ray-absorption (1)
- young star clusters (1)
- youth (1)
- zebrafish (1)
- Überschwemmungen (1)
- иперболический аттрактор (1)
- оллективная динамика (1)
- синхронизация (1)
Institute
- Institut für Physik und Astronomie (4728) (remove)
Comb-like geometric constraints leading to emergence of the time-fractional Schrödinger equation
(2021)
This paper presents an overview over several examples, where the comb-like geometric constraints lead to emergence of the time-fractional Schrodinger equation. Motion of a quantum object on a comb structure is modeled by a suitable modification of the kinetic energy operator, obtained by insertion of the Dirac delta function in the Laplacian. First, we consider motion of a free particle on two- and three-dimensional comb structures, and then we extend the study to the interacting cases. A general form of a nonlocal term, which describes the interactions of the particle with the medium, is included in the Hamiltonian, and later on, the cases of constant and Dirac delta potentials are analyzed. At the end, we discuss the case of non-integer dimensions, considering separately the case of fractal dimension between one and two, and the case of fractal dimension between two and three. All these examples show that even though we are starting with the standard time-dependent Schrodinger equation on a comb, the time-fractional equation for the Green's functions appears, due to these specific geometric constraints.
We present the discovery of a new double-detonation progenitor system consisting of a hot subdwarf B (sdB) binary with a white dwarf companion with a P (orb) = 76.34179(2) minutes orbital period. Spectroscopic observations are consistent with an sdB star during helium core burning residing on the extreme horizontal branch. Chimera light curves are dominated by ellipsoidal deformation of the sdB star and a weak eclipse of the companion white dwarf. Combining spectroscopic and light curve fits, we find a low-mass sdB star, M (sdB) = 0.383 +/- 0.028 M (circle dot) with a massive white dwarf companion, M (WD) = 0.725 +/- 0.026 M (circle dot). From the eclipses we find a blackbody temperature for the white dwarf of 26,800 K resulting in a cooling age of approximate to 25 Myr whereas our MESA model predicts an sdB age of approximate to 170 Myr. We conclude that the sdB formed first through stable mass transfer followed by a common envelope which led to the formation of the white dwarf companion approximate to 25 Myr ago. Using the MESA stellar evolutionary code we find that the sdB star will start mass transfer in approximate to 6 Myr and in approximate to 60 Myr the white dwarf will reach a total mass of 0.92 M (circle dot) with a thick helium layer of 0.17 M (circle dot). This will lead to a detonation that will likely destroy the white dwarf in a peculiar thermonuclear supernova. PTF1 J2238+7430 is only the second confirmed candidate for a double-detonation thermonuclear supernova. Using both systems we estimate that at least approximate to 1% of white dwarf thermonuclear supernovae originate from sdB+WD binaries with thick helium layers, consistent with the small number of observed peculiar thermonuclear explosions.
The study addresses the question, if observed changes in terms of Arctic-midlatitude linkages during winter are driven by Arctic Sea ice decline alone or if the increase of global sea surface temperatures plays an additional role. We compare atmosphere-only model experiments with ECHAM6 to ERA-Interim Reanalysis data. The model sensitivity experiment is implemented as a set of four combinations of sea ice and sea surface temperature boundary conditions. Atmospheric circulation regimes are determined and evaluated in terms of their cyclone and blocking characteristics and changes in frequency during winter. As a prerequisite, ECHAM6 reproduces general features of circulation regimes very well. Tropospheric changes induced by the change of boundary conditions are revealed and further impacts on the large-scale circulation up into the stratosphere are investigated. In early winter, the observed increase of atmospheric blocking in the region between Scandinavia and the Urals are primarily related to the changes in sea surface temperatures. During late winter, we f nd a weakened polar stratospheric vortex in the reanalysis that further impacts the troposphere. In the model sensitivity study a climatologically weakened polar vortex occurs only if sea ice is reduced and sea surface temperatures are increased together. This response is delayed compared to the reanalysis. The tropospheric response during late winter is inconclusive in the model, which is potentially related to the weak and delayed response in the stratosphere. The model experiments do not reproduce the connection between early and late winter as interpreted from the reanalysis. Potentially explaining this mismatch, we identify a discrepancy of ECHAM6 to reproduce the weakening of the stratospheric polar vortex through blocking induced upward propagation of planetary waves.
We consider a system of noninteracting particles on a line with initial positions distributed uniformly with density ? on the negative half-line. We consider two different models: (i) Each particle performs independent Brownian motion with stochastic resetting to its initial position with rate r and (ii) each particle performs run -and-tumble motion, and with rate r its position gets reset to its initial value and simultaneously its velocity gets randomized. We study the effects of resetting on the distribution P(Q, t) of the integrated particle current Q up to time t through the origin (from left to right). We study both the annealed and the quenched current distributions and in both cases, we find that resetting induces a stationary limiting distribution of the current at long times. However, we show that the approach to the stationary state of the current distribution in the annealed and the quenched cases are drastically different for both models. In the annealed case, the whole distribution P-an(Q, t) approaches its stationary limit uniformly for all Q. In contrast, the quenched distribution P-qu(Q, t) attains its stationary form for Q < Q(crit)(t), while it remains time dependent for Q > Q(crit)(t). We show that Q(crit)(t) increases linearly with t for large t. On the scale where Q <; Q(crit)(t), we show that P-qu(Q, t) has an unusual large deviation form with a rate function that has a third-order phase transition at the critical point. We have computed the associated rate functions analytically for both models. Using an importance sampling method that allows to probe probabilities as tiny as 10-14000, we were able to compute numerically this nonanalytic rate function for the resetting Brownian dynamics and found excellent agreement with our analytical prediction.
We present a detailed spectroscopic and timing analysis of X-ray observations of the bright pulsar PSR B0656+14. The observations were obtained simultaneously with eROSITA and XMM-Newton during the calibration and performance verification phase of the Spektrum-Roentgen-Gamma mission (SRG). The analysis of the 100 ks deep observation of eROSITA is supported by archival observations of the source, including XMM-Newton, NuSTAR, and NICER. Using XMM-Newton and NICER, we first established an X-ray ephemeris for the time interval 2015 to 2020, which connects all X-ray observations in this period without cycle count alias and phase shifts. The mean eROSITA spectrum clearly reveals an absorption feature originating from the star at 570 eV with a Gaussian sigma of about 70 eV that was tentatively identified in a previous long XMM-Newton observation. A second previously discussed absorption feature occurs at 260-265 eV and is described here as an absorption edge. It could be of atmospheric or of instrumental origin. These absorption features are superposed on various emission components that are phenomenologically described here as the sum of hot (120 eV) and cold (65 eV) blackbody components, both of photospheric origin, and a power law with photon index Gamma = 2 from the magnetosphere. We created energy-dependent light curves and phase-resolved spectra with a high signal-to-noise ratio. The phase-resolved spectroscopy reveals that the Gaussian absorption line at 570 eV is clearly present throughout similar to 60% of the spin cycle, but it is otherwise undetected. Likewise, its parameters were found to be dependent on phase. The visibility of the line strength coincides in phase with the maximum flux of the hot blackbody. If the line originates from the stellar surface, it nevertheless likely originates from a different location than the hot polar cap. We also present three families of model atmospheres: a magnetized atmosphere, a condensed surface, and a mixed model. They were applied to the mean observed spectrum, whose continuum fit the observed data well. The atmosphere model, however, predicts distances that are too short. For the mixed model, the Gaussian absorption may be interpreted as proton cyclotron absorption in a field as high as 10(14) G, which is significantly higher than the field derived from the moderate observed spin-down.
Perovskite semiconductors are an attractive option to overcome the limitations of established silicon based photovoltaic (PV) technologies due to their exceptional opto-electronic properties and their successful integration into multijunction cells. However, the performance of single- and multijunction cells is largely limited by significant nonradiative recombination at the perovskite/organic electron transport layer junctions. In this work, the cause of interfacial recombination at the perovskite/C-60 interface is revealed via a combination of photoluminescence, photoelectron spectroscopy, and first-principle numerical simulations. It is found that the most significant contribution to the total C-60-induced recombination loss occurs within the first monolayer of C-60, rather than in the bulk of C-60 or at the perovskite surface. The experiments show that the C-60 molecules act as deep trap states when in direct contact with the perovskite. It is further demonstrated that by reducing the surface coverage of C-60, the radiative efficiency of the bare perovskite layer can be retained. The findings of this work pave the way toward overcoming one of the most critical remaining performance losses in perovskite solar cells.
Thanks to dedicated long-term missions like Voyager and GOES over the past 50 years, much insight has been gained on the activity of our Sun, the solar wind, its interaction with the interstellar medium, and, thus, about the formation, the evolution, and the structure of the heliosphere. Additionally, with the help of multi-wavelength observations by the Hubble Space Telescope, Kepler, and TESS, we not only were able to detect a variety of extrasolar planets and exomoons but also to study the characteristics of their host stars, and thus became aware that other stars drive bow shocks and astrospheres. Although features like, e.g., stellar winds, could not be measured directly, over the past years several techniques have been developed allowing us to indirectly derive properties like stellar mass-loss rates and stellar wind speeds, information that can be used as direct input to existing astrospheric modeling codes. In this review, the astrospheric modeling efforts of various stars will be presented. Starting with the heliosphere as a benchmark of astrospheric studies, investigating the paleo-heliospheric changes and the Balmer H alpha projections to 1 pc, we investigate the surroundings of cool and hot stars, but also of more exotic objects like neutron stars. While pulsar wind nebulae (PWNs) might be a source of high-energy galactic cosmic rays (GCRs), the astrospheric environments of cool and hot stars form a natural shield against GCRs. Their modulation within these astrospheres, and the possible impact of turbulence, are also addressed. This review shows that all of the presented modeling efforts are in excellent agreement with currently available observations.
Energetic charged particles trapped in planetary radiation belts are hazardous to spacecraft. Planned missions to iron-rich asteroids with possible strong remanent magnetic fields require an assessment of trapped particles energies. Using laboratory measurements of iron meteorites, we estimate the largest possible asteroid magnetic moment. Although weak compared to moments of planetary dynamos, the small body size may yield strong surface fields. We use hybrid simulations to confirm the formation of a magnetosphere with an extended quasi-dipolar region. However, the short length scale of the field implies that energetic particle motion would be nonadiabatic, making existing radiation belt theories not applicable. Our idealized particle simulations demonstrate that chaotic motions lead to particle loss at lower energies than those predicted by adiabatic theory, which may explain the energies of transiently trapped particles observed at Mercury, Ganymede, and Earth. However, even the most magnetized asteroids are unlikely to stably trap hazardous particles.
Massive stars that become stripped of their hydrogen envelope through binary interaction or winds can be observed either as Wolf-Rayet stars, if they have optically thick winds, or as transparent-wind stripped-envelope stars. We approximate their evolution through evolutionary models of single helium stars, and compute detailed model grids in the initial mass range 1.5-70 M. for metallicities between 0.01 and 0.04, from core helium ignition until core collapse. Throughout their lifetimes some stellar models expose the ash of helium burning. We propose that models that have nitrogen-rich envelopes are candidate WN stars, while models with a carbon-rich surface are candidate WC stars during core helium burning, and WO stars afterwards. We measure the metallicity dependence of the total lifetimes of our models and the duration of their evolutionary phases. We propose an analytic estimate of the wind's optical depth to distinguish models of Wolf-Rayet stars from transparent-wind stripped-envelope stars, and find that the luminosity ranges at which WN-, WC-, and WO-type stars can exist is a strong function of metallicity. We find that all carbon-rich models produced in our grids have optically thick winds and match the luminosity distribution of observed populations. We construct population models and predict the numbers of transparent-wind stripped-envelope stars and Wolf-Rayet stars, and derive their number ratios at different metallicities. We find that as metallicity increases, the number of transparent-wind stripped-envelope stars decreases and the number of Wolf-Rayet stars increases. At high metallicities WC- and WO-type stars become more common. We apply our population models to nearby galaxies, and find that populations are more sensitive to the transition luminosity between Wolf-Rayet stars and transparent-wind helium stars than to the metallicity-dependent mass loss rates.
The bimolecular recombination characteristics of conjugated polymer poly[(4,4'-bis(2-ethylhexyl)dithieno[3,2-b:2',3'-d]silole)-2,6-diyl-alt-(2,5-bis 3-tetradecylthiophen-2-y1 thiazolo 5,4-d thiazole)-2,5diy1] (PDTSiTTz) blended with the fullerene series PC60BM, ICMA, ICBA, and ICTA have been investigated using microsecond and femtosecond transient absorption spectroscopy, in conjunction with electroluminescence measurements and ambient photoemission spectroscopy. The non-Langevin polymer PDTSiTTz allows an inspection of intrinsic bimolecular recombination rates uninhibited by diffusion, while the low oscillator strengths of fullerenes allow polymer features to dominate, and we compare our results to those of the well-known polymer Si-PCPDTBT. Using mu s-TAS, we have shown that the trap -limited decay dynamics of the PDTSiTTz polaron becomes progressively slower across the fullerene series, while those of Si-PCPDTBT are invariant. Electroluminescence measurements showed an unusual double peak in pristine PDTSiTTz, attributed to a low energy intragap charge transfer state, likely interchain in nature. Furthermore, while the pristine PDTSiTTz showed a broad, low-intensity density of states, the ICBA and ICTA blends presented a virtually identical DOS to Si-PCPDTBT and its blends. This has been attributed to a shift from a delocalized, interchain highest occupied molecular orbital (HOMO) in the pristine material to a dithienosilole-centered HOMO in the blends, likely a result of the bulky fullerenes increasing interchain separation. This HOMO localization had a side effect of progressively shifting the polymer HOMO to shallower energies, which was correlated with the observed decrease in bimolecular recombination rate and increased "trap" depth. However, since the density of tail states remained the same, this suggests that the traditional viewpoint of "trapping" being dominated by tail states may not encompass the full picture and that the breadth of the DOS may also have a strong influence on bimolecular recombination.
We present observations with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope of seven compact low-mass star-forming galaxies at redshifts, z, in the range 0.3161-0.4276, with various O3Mg2 = [O III] lambda 5007/Mg II lambda 2796+2803 and Mg-2 = Mg II lambda 2796/Mg II lambda 2803 emission-line ratios. We aim to study the dependence of leaking Lyman continuum (LyC) emission on the characteristics of Mg ii emission together with the dependencies on other indirect indicators of escaping ionizing radiation. LyC emission with escape fractions f(esc)(LyC) = 3.1-4.6 per cent is detected in four galaxies, whereas only 1 sigma upper limits of f(esc)(LyC) in the remaining three galaxies were derived. A strong narrow Ly alpha emission line with two peaks separated by V-sep similar to 298-592 km s(-1) was observed in four galaxies with detected LyC emission and very weak Ly alpha emission is observed in galaxies with LyC non-detections. Our new data confirm the tight anticorrelation between f(esc)(LyC) and V-sep found for previous low-redshift galaxy samples. V-sep remains the best indirect indicator of LyC leakage among all considered indicators. It is found that escaping LyC emission is detected predominantly in galaxies with Mg-2 greater than or similar to 1.3. A tendency of an increase of f(esc)(LyC) with increasing of both the O3Mg2 and Mg-2 is possibly present. However, there is substantial scatter in these relations not allowing their use for reliable prediction of f(esc)(LyC).
Multijunction solar cells can overcome the fundamental efficiency limits of single-junction devices. The bandgap tunability of metal halide perovskite solar cells renders them attractive for multijunction architectures(1). Combinations with silicon and copper indium gallium selenide (CIGS), as well as all-perovskite tandem cells, have been reported(2-5). Meanwhile, narrow-gap non-fullerene acceptors have unlocked skyrocketing efficiencies for organic solar cells(6,7). Organic and perovskite semiconductors are an attractive combination, sharing similar processing technologies. Currently, perovskite-organic tandems show subpar efficiencies and are limited by the low open-circuit voltage (V-oc) of wide-gap perovskite cells(8) and losses introduced by the interconnect between the subcells(9,10). Here we demonstrate perovskite-organic tandem cells with an efficiency of 24.0 per cent (certified 23.1 per cent) and a high V-oc of 2.15 volts. Optimized charge extraction layers afford perovskite subcells with an outstanding combination of high V-oc and fill factor. The organic subcells provide a high external quantum efficiency in the near-infrared and, in contrast to paradigmatic concerns about limited photostability of non-fullerene cells(11), show an outstanding operational stability if excitons are predominantly generated on the non-fullerene acceptor, which is the case in our tandems. The subcells are connected by an ultrathin (approximately 1.5 nanometres) metal-like indium oxide layer with unprecedented low optical/electrical losses. This work sets a milestone for perovskite-organic tandems, which outperform the best p-i-n perovskite single junctions(12) and are on a par with perovskite-CIGS and all-perovskite multijunctions(13).
A combinatorial study of the effect of in-mixing of various guests on the thermoelectric properties of the host workhorse polymer poly[2,5-bis(3-tetradecylthiophen-2-yl)thieno[3,2-b]thiophene] (PBTTT) is presented. Specifically, the composition and thickness for doped films of PBTTT blended with different polymers are varied. Some blends at guest weight fractions around 10-15% exhibit up to a fivefold increase in power factor compared to the reference material, leading to zT values around 0.1. Spectroscopic analysis of the charge-transfer species, structural characterization using grazing-incidence wide-angle X-ray scattering, differential scanning calorimetry, Raman, and atomic force microscopy, and Monte Carlo simulations are employed to determine that the key to improved performance is for the guest to promote long-range electrical connectivity and low disorder, together with similar highest occupied molecular orbital levels for both materials in order to ensure electronic connectivity are combined.
We present proper motion (PM) measurements within the central region of the Large Magellanic Cloud (LMC), using near-infrared data from the VISTA survey of the Magellanic Cloud system (VMC). This work encompasses 18 VMC tiles covering a total sky area of similar to 28 deg(2). We computed absolute stellar PMs from multiepoch observations in the K-s filter over time baselines between similar to 12 and 47 months. Our final catalogue contains similar to 6322 000 likely LMC member stars with derived PMs. We employed a simple flat-rotating disc model to analyse and interpret the PM data. We found a stellar centre of rotation (alpha(0) = 79.95 degrees(+0.22)(-0.23), delta(0) = -69.31 degrees(+0.12)(-0.11)) that is in agreement with that resulting from Hubble Space Telescope data. The inferred viewing angles of the LMC disc (i = 33.5 degrees(+1.2)(-1.3), Theta = 129.8 degrees(+1.9)(-1.9)) are in good agreement with values from the literature but suggest a higher inclination of the central parts of the LMC. Our data confirm a higher rotation amplitude for the young (less than or similar to 0.5 Gyr) stars compared to the intermediate-age/old (greater than or similar to 1 Gyr) population, which can be explained by asymmetric drift. We constructed spatially resolved velocity maps of the intermediate-age/old and young populations. Intermediate-age/old stars follow elongated orbits parallel to the bar's major axis, providing first observational evidence for x(1) orbits within the LMC bar. In the innermost regions, the motions show more chaotic structures. Young stars show motions along a central filamentary bar structure.
Simulating the space weather in the AU Mic system: stellar winds and extreme coronal mass ejections
(2022)
Two close-in planets have been recently found around the M-dwarf flare star AU Microscopii (AU Mic). These Neptune-sized planets (AU Mic b and c) seem to be located very close to the so-called "evaporation valley" in the exoplanet population, making this system an important target for studying atmospheric loss on exoplanets. This process, while mainly driven by high-energy stellar radiation, will be strongly mediated by the space environment surrounding the planets. Here we present an investigation of this last area, performing 3D numerical modeling of the quiescent stellar wind from AU Mic, as well as time-dependent simulations describing the evolution of a highly energetic coronal mass ejection (CME) event in this system. Observational constraints on the stellar magnetic field and properties of the eruption are incorporated in our models. We carry out qualitative and quantitative characterizations of the stellar wind, the emerging CMEs, as well as the expected steady and transient conditions along the orbit of both exoplanets. Our results predict extreme space weather for AU Mic and its planets. This includes sub-Alfvenic regions for the large majority of the exoplanet orbits, very high dynamic and magnetic pressure values in quiescence (varying within 10(2)-10(5) times the dynamic pressure experienced by Earth), and an even harsher environment during the passage of any escaping CME associated with the frequent flaring observed in AU Mic. These space weather conditions alone pose an immense challenge for the survival of exoplanetary atmospheres (if any) in this system.
When two initially thermal many-body systems start to interact strongly, their transient states quickly become non-Gibbsian, even if the systems eventually equilibrate. To see beyond this apparent lack of structure during the transient regime, we use a refined notion of thermality, which we call g-local. A system is g-locally thermal if the states of all its small subsystems are marginals of global thermal states. We numerically demonstrate for two harmonic lattices that whenever the total system equilibrates in the long run, each lattice remains g-locally thermal at all times, including the transient regime. This is true even when the lattices have long-range interactions within them. In all cases, we find that the equilibrium is described by the generalized Gibbs ensemble, with three-dimensional lattices requiring special treatment due to their extended set of conserved charges. We compare our findings with the well-known two-temperature model. While its standard form is not valid beyond weak coupling, we show that at strong coupling it can be partially salvaged by adopting the concept of a g-local temperature.
Core-collapse supernova remnants are structures of the interstellar medium (ISM) left behind the explosive death of most massive stars ( ?40 M-?). Since they result in the expansion of the supernova shock wave into the gaseous environment shaped by the star's wind history, their morphology constitutes an insight into the past evolution of their progenitor star. Particularly, fast-mo ving massiv e stars can produce asymmetric core-collapse superno va remnants. We inv estigate the mixing of materials in core-collapse supernova remnants generated by a moving massive 35 M-? star, in a magnetized ISM. Stellar rotation and the wind magnetic field are time-dependently included into the models which follow the entire evolution of the stellar surroundings from the zero-age main-sequence to 80 kyr after the supernova explosion. It is found that very little main-sequence material is present in remnants from moving stars, that the Wolf-Rayet wind mixes very efficiently within the 10 kyr after the explosion, while the red supergiant material is still unmixed by 30 per cent within 50 kyr after the supernova. Our results indicate that the faster the stellar motion, the more complex the internal organization of the supernova remnant and the more ef fecti ve the mixing of ejecta therein. In contrast, the mixing of stellar wind material is only weakly affected by progenitor motion, if at all.
This review discusses picosecond ultrasonics experiments using ultrashort hard x-ray probe pulses to extract the transient strain response of laser-excited nanoscopic structures from Bragg-peak shifts. This method provides direct, layer-specific, and quantitative information on the picosecond strain response for structures down to few-nm thickness. We model the transient strain using the elastic wave equation and express the driving stress using Gruneisen parameters stating that the laser-induced stress is proportional to energy density changes in the microscopic subsystems of the solid, i.e., electrons, phonons and spins. The laser-driven strain response can thus serve as an ultrafast proxy for local energy-density and temperature changes, but we emphasize the importance of the nanoscale morphology for an accurate interpretation due to the Poisson effect. The presented experimental use cases encompass ultrathin and opaque metal-heterostructures, continuous and granular nanolayers as well as negative thermal expansion materials, that each pose a challenge to established all-optical techniques.
The NGC 346 young stellar system and associated N66 giant H ii region in the Small Magellanic Cloud are the nearest example of a massive star-forming event in a low metallicity (Z approximate to 0.2Z (circle dot)) galaxy. With an age of less than or similar to 3 Myr this system provides a unique opportunity to study relationships between massive stars and their associated H ii region. Using archival data, we derive a total H alpha luminosity of L(H alpha) = 4.1 x 10(38) erg s(-1) corresponding to an H-photoionization rate of 3 x 10(50) s(-1). A comparison with a predicted stellar ionization rate derived from the more than 50 known O-stars in NGC 346, including massive stars recently classified from Hubble Space Telescope far-ultraviolet (FUV) spectra, indicates an approximate ionization balance. Spectra obtained with SALT suggest the ionization structure of N66 could be consistent with some leakage of ionizing photons. Due to the low metallicity, the FUV luminosity from NGC 346 is not confined to the interstellar cloud associated with N66. Ionization extends through much of the spatial extent of the N66 cloud complex, and most of the cloud mass is not ionized. The stellar mass estimated from nebular L(H alpha) appears to be lower than masses derived from the census of resolved stars which may indicate a disconnect between the formation of high and low mass stars in this region. We briefly discuss implications of the properties of N66 for studies of star formation and stellar feedback in low metallicity environments.
The unmixed debris of Gaia-Sausage/Enceladus in the form of a pair of halo stellar overdensities
(2022)
In the first billion years after its formation, the galaxy underwent several mergers with dwarf satellites of various masses. The debris of Gaia-Sausage/Enceladus (GSE), the galaxy responsible for the last significant merger of the Milky Way, dominates the inner halo and has been suggested to be the progenitor of both the Hercules-Aquila Cloud (HAC) and Virgo Overdensity (VOD). We combine SEGUE, APOGEE, Gaia, and StarHorse distances to characterize the chemodynamical properties and verify the link between HAC, VOD, and GSE. We find that the orbital eccentricity distributions of the stellar overdensities and GSE are comparable. We also find that they have similar, strongly peaked, metallicity distribution functions, reinforcing the hypothesis of common origin. Furthermore, we show that HAC and VOD are indistinguishable from the prototypical GSE population within all chemical-abundance spaces analyzed. All these evidences combined provide a clear demonstration that the GSE merger is the main progenitor of the stellar populations found within these halo overdensities.