TY  - JOUR
A1  - Troll, Günter
A1  - Beim Graben, Peter
T1  - Zipfs law is not a consequence of the central limit theorem
Y1  - 1998
ER  - 
TY  - JOUR
A1  - Blasius, Bernd
A1  - Toenjes, Ralf
T1  - Zipf's Law in the popularity distribution of chess openings
N2  - We perform a quantitative analysis of extensive chess databases and show that the frequencies of opening moves are distributed according to a power law with an exponent that increases linearly with the game depth, whereas the pooled distribution of all opening weights follows Zipf's law with universal exponent. We propose a simple stochastic process that is able to capture the observed playing statistics and show that the Zipf law arises from the self-similar nature of the game tree of chess. Thus, in the case of hierarchical fragmentation the scaling is truly universal and independent of a particular generating mechanism. Our findings are of relevance in general processes with composite decisions.
Y1  - 2009
UR  - http://prl.aps.org/
U6  - https://doi.org/10.1103/Physrevlett.103.218701
SN  - 0031-9007
ER  - 
TY  - JOUR
A1  - Lange, Ilja
A1  - Reiter, Sina
A1  - Kniepert, Juliane
A1  - Piersimoni, Fortunato
A1  - Paetzel, Michael
A1  - Hildebrandt, Jana
A1  - Brenner, Thomas J. K.
A1  - Hecht, Stefan
A1  - Neher, Dieter
T1  - Zinc oxide modified with benzylphosphonic acids as transparent electrodes in regular and inverted organic solar cell structures
JF  - Applied physics letters
N2  - An approach is presented to modify the work function of solution-processed sol-gel derived zinc oxide (ZnO) over an exceptionally wide range of more than 2.3 eV. This approach relies on the formation of dense and homogeneous self-assembled monolayers based on phosphonic acids with different dipole moments. This allows us to apply ZnO as charge selective bottom electrodes in either regular or inverted solar cell structures, using poly(3-hexylthiophene): phenyl-C71-butyric acid methyl ester as the active layer. These devices compete with or even surpass the performance of the reference on indium tin oxide/poly(3,4-ethylenedioxythiophene) polystyrene sulfonate. Our findings highlight the potential of properly modified ZnO as electron or hole extracting electrodes in hybrid optoelectronic devices. (C) 2015 AIP Publishing LLC.
Y1  - 2015
U6  - https://doi.org/10.1063/1.4916182
SN  - 0003-6951
SN  - 1077-3118
VL  - 106
IS  - 11
PB  - American Institute of Physics
CY  - Melville
ER  - 
TY  - JOUR
A1  - Rosenhahn, Axel
A1  - Finlay, John A.
A1  - Pettit, Michala E.
A1  - Ward, Andy
A1  - Wirges, Werner
A1  - Gerhard, Reimund
A1  - Callow, Maureen E.
A1  - Grunze, Michael
A1  - Callow, James A.
T1  - Zeta potential of motile spores of the green alga Ulva linza and the influence of electrostatic interactions on spore settlement and adhesion strength
N2  - The zeta potential of the motile spores of the green alga (seaweed) Ulva linza was quantified by video microscopy in combination with optical tweezers and determined to be -19.3ñ1.1 mV. The electrostatic component involved in the settlement and adhesion of spores was studied using electret surfaces consisting of PTFE and bearing different net charges. As the surface chemistry remains the same for differently charged surfaces, the experimental results isolate the influence of surface charge and thus electrostatic interactions. Ulva spores were demonstrated to have a reduced tendency to settle on negatively charged surfaces and when they did settle the adhesion strength of settled spores was lower than with neutral or positively charged surfaces. These observations can be ascribed to electrostatic interactions.
Y1  - 2009
UR  - http://biointerphases.org/
U6  - https://doi.org/10.1116/1.3110182
SN  - 1559-4106
ER  - 
TY  - JOUR
A1  - Cioni, Maria-Rosa L.
A1  - Bekki, Kenji
A1  - Girardi, Leo
A1  - de Grijs, Richard
A1  - Irwin, Mike J.
A1  - Ivanov, Valentin D.
A1  - Marconi, Marcella
A1  - Oliveira, Joana M.
A1  - Piatti, Andres E.
A1  - Ripepi, Vincenzo
A1  - van Loon, Jacco Th.
T1  - XVII. Proper motions of the Small Magellanic Cloud and the Milky Way globular cluster 47 Tucanae
JF  - Physical review : E, Statistical, nonlinear and soft matter physics
N2  - Aims. In this study we use multi-epoch near-infrared observations from the VISTA survey of the Magellanic Cloud system (VMC) to measure the proper motions of different stellar populations in a tile of 1.5 deg2 in size in the direction of the Galactic globular cluster 47 Tuc. We obtain the proper motion of the cluster itself, of the Small Magellanic Cloud (SMC), and of the field Milky Way stars.

Methods. Stars of the three main stellar components are selected according to their spatial distributions and their distributions in colour−magnitude diagrams. Their average coordinate displacement is computed from the difference between multiple Ks-band observations for stars as faint as Ks = 19 mag. Proper motions are derived from the slope of the best-fitting line among ten VMC epochs over a time baseline of ~1 yr. Background galaxies are used to calibrate the absolute astrometric reference frame.

Results. The resulting absolute proper motion of 47 Tuc is (μαcos(δ), μδ) = (+7.26 ± 0.03, −1.25 ± 0.03) mas yr-1. This measurement refers to about 35 000 sources distributed between 10′ and 60′ from the cluster centre. For the SMC we obtain (μαcos(δ), μδ) = (+1.16 ± 0.07, −0.81 ± 0.07) mas yr-1 from about 5250 red clump and red giant branch stars. The absolute proper motion of the Milky Way population in the line of sight (l = 305.9, b = −44.9) of this VISTA tile is (μαcos(δ), μδ) = (+10.22 ± 0.14, −1.27 ± 0.12) mas yr-1 and has been calculated from about 4000 sources. Systematic uncertainties associated with the astrometric reference system are 0.18 mas yr-1. Thanks to the proper motion we detect 47 Tuc stars beyond its tidal radius.
KW  - proper motions
KW  - surveys
KW  - Magellanic Clouds
KW  - globular clusters: individual: 47 Tucanae
Y1  - 2016
U6  - https://doi.org/10.1051/0004-6361/201527004
SN  - 1432-0746
VL  - 586
SP  - 67
EP  - 75
PB  - EDP Sciences
CY  - Les Ulis
ER  - 
TY  - JOUR
A1  - Sanjurjo-Ferrrin, G.
A1  - Torrejon, J. M.
A1  - Postnov, K.
A1  - Oskinova, Lida
A1  - Rodes-Roca, J. J.
A1  - Bernabeu, Guillermo
T1  - XMM-Newton spectroscopy of the accreting magnetar candidate 4U0114+65
JF  - Astronomy and astrophysics : an international weekly journal
N2  - Methods. We analysed the energy-resolved light curve and the time-resolved X-ray spectra provided by the EPIC cameras on board XMM-Newton. We also analysed the first high-resolution spectrum of this source provided by the Reflection Grating Spectrometer. Results. An X-ray pulse of 9350 +/- 160 s was measured. Comparison with previous measurements confirms the secular spin up of this source. We successfully fit the pulse-phase-resolved spectra with Comptonisation models. These models imply a very small (r similar to 3 km) and hot (kT similar to 2-3 keV) emitting region and therefore point to a hot spot over the neutron star (NS) surface as the most reliable explanation for the X-ray pulse. The long NS spin period, the spin-up rate, and persistent X-ray emission can be explained within the theory of quasi-spherical settling accretion, which may indicate that the magnetic field is in the magnetar range. Thus, 4U0114+65 could be a wind-accreting magnetar. We also observed two episodes of low luminosity. The first was only observed in the low-energy light curve and can be explained as an absorption by a large over-dense structure in the wind of the B1 supergiant donor. The second episode, which was deeper and affected all energies, may be due to temporal cessation of accretion onto one magnetic pole caused by non-spherical matter capture from the structured stellar wind. The light curve displays two types of dips that are clearly seen during the high-flux intervals. The short dips, with durations of tens of seconds, are produced through absorption by wind clumps. The long dips, in turn, seem to be associated with the rarefied interclump medium. From the analysis of the X-ray spectra, we found evidence of emission lines in the X-ray photoionised wind of the B1Ia donor. The Fe K alpha line was found to be highly variable and much weaker than in other X-ray binaries with supergiant donors. The degree of wind clumping, measured through the covering fraction, was found to be much lower than in supergiant donor stars with earlier spectral types. Conclusions. The XMM-Newton spectroscopy provided further support for the magnetar nature of the neutron star in 4U0114+65. The light curve presents dips that can be associated with clumps and the interclump medium in the stellar wind of the mass donor.
KW  - X-rays: binaries
KW  - stars: winds, outflows
KW  - pulsars: individual: 4U0114+65
Y1  - 2017
U6  - https://doi.org/10.1051/0004-6361/201630119
SN  - 1432-0746
VL  - 606
SP  - 4039
EP  - 4042
PB  - EDP Sciences
CY  - Les Ulis
ER  - 
TY  - JOUR
A1  - Ignace, Richard
A1  - Oskinova, Lida
A1  - Brown, John C.
T1  - XMM-Newton Observations of the Nitrogen-Rich Wolf-Rayet star WR1
N2  - We present XMM-Newton results for the X-ray spectrum from the N-rich Wolf-Rayet (WR) star WR 1. The EPIC instrument was used to obtain a medium-resolution spectrum. The following features characterize this spectrum: (a) significant emission "bumps" appear that are coincident with the wavelengths of typical strong lines, such as Mg XI, Si XIII and S XV; (b) little emission is detected above 4 keV, in contrast to recent reports of a hard component in the stars WR 6 and WR 110 which are of similar subtype; and (c) evidence for sulfur K-edge absorption at about 2.6 keV, which could only arise from absorption of X-rays by the ambient stellar wind. The lack of hard emission in our dataset is suggestive that WR 1 may truly be a single star, thus representing the first detailed X-ray spectrum that isolates the WR wind alone (in contrast to colliding wind zones). Although the properties of the S-edge are not well-constrained by our data, it does appear to be real, and its detection indicates that at least some of the hot gas in WR 1 must reside interior to the radius of optical depth unity for the total absorptive opacity at the energy of the edge.
Y1  - 2003
ER  - 
TY  - JOUR
A1  - Sidoli, Lara
A1  - Sguera, Vito
A1  - Esposito, Paolo
A1  - Oskinova, Lida
A1  - Polletta, Maria del Carmen
T1  - XMM-Newton discovery of very high obscuration in the candidate Supergiant Fast X-ray Transient AX J1714.1-3912
JF  - Monthly notices of the Royal Astronomical Society
N2  - We have analysed an archival XMM-Newton EPIC observation that serendipitously covered the sky position of a variable X-ray source AX J1714.1-3912, previously suggested to be a Supergiant Fast X-ray Transient (SFXT). During the XMM-Newton observation the source is variable on a timescale of hundred seconds and shows two luminosity states, with a flaring activity followed by unflared emission, with a variability amplitude of a factor of about 50. We have discovered an intense iron emission line with a centroid energy of 6.4 keV in the power law-like spectrum, modified by a large absorption (N-H similar to 10(24) cm(-2)), never observed before from this source. This X-ray spectrum is unusual for an SFXT, but resembles the so-called 'highly obscured sources', high mass X-ray binaries (HMXBs) hosting an evolved B[e] supergiant companion (sgB[e]). This might suggest that AX J1714.1-3912 is a new member of this rare type of HMXBs, which includes IGR J16318-4848 and CI Camelopardalis. Increasing this small population of sources would be remarkable, as they represent an interesting short transition evolutionary stage in the evolution of massive binaries. Nevertheless, AX J1714.1-3912 appears to share X-ray properties of both kinds of HMXBs (SFXT versus sgB[e] HMXB). Therefore, further investigations of the companion star are needed to disentangle the two hypothesis.
KW  - X-rays: binaries
KW  - X-rays: individual: AX J1714.1-3912
Y1  - 2022
U6  - https://doi.org/10.1093/mnras/stac691
SN  - 0035-8711
SN  - 1365-2966
VL  - 512
IS  - 2
SP  - 2929
EP  - 2935
PB  - Oxford Univ. Press
CY  - Oxford
ER  - 
TY  - JOUR
A1  - Reiche, Jürgen
A1  - Barberka, Thomas Andreas
A1  - Janietz, Dietmar
A1  - Hofmann, Dieter
A1  - Pietsch, Ullrich
A1  - Brehmer, Ludwig
T1  - X-ray structure investigation and computer modelling of Langmuir-Blodgett films formed from disc-shaped pentaalkines
Y1  - 1994
ER  - 
TY  - JOUR
A1  - Miedema, P. S.
A1  - Mitzner, Rolf
A1  - Ganschow, S.
A1  - Föhlisch, Alexander
A1  - Beye, Martin
T1  - X-ray spectroscopy on the active ion in laser crystals
JF  - Physical chemistry, chemical physics : a journal of European Chemical Societies
N2  - The active ions in typical laser crystals were studied with Resonant Inelastic X-ray Scattering (RIXS) and Partial Fluorescence Yield X-ray Absorption (PFY-XAS) spectroscopies as solid state model systems for dilute active centers. We analyzed Ti3+ and Cr3+ in alpha-Al2O3:Ti3+ and LiCaAlF6:Cr3+, respectively. The comparison of experimental data with semi-empirical multiplet calculations provides insights into the electronic structure and shows how measured crystal field energies are related across different spectroscopies.
Y1  - 2017
U6  - https://doi.org/10.1039/c7cp03026f
SN  - 1463-9076
SN  - 1463-9084
VL  - 19
SP  - 21800
EP  - 21806
PB  - Royal Society of Chemistry
CY  - Cambridge
ER  - 
TY  - JOUR
A1  - Pietsch, Ullrich
A1  - Barberka, Thomas Andreas
A1  - Geue, Thomas
A1  - Stömmer, Ralph
T1  - X-ray scattering from thin organic films and multilayers
Y1  - 1997
ER  - 
TY  - THES
A1  - Stömmer, Ralph
T1  - X-ray scattering from silicon surfaces and thin oxides on silicon substrates
Y1  - 1998
ER  - 
TY  - JOUR
A1  - Stömmer, Ralph
A1  - Göbel, H.
A1  - Hub, W.
A1  - Pietsch, Ullrich
T1  - X-ray scattering from silicon surfaces
Y1  - 1998
ER  - 
TY  - THES
A1  - Baumbach, Tilo
T1  - X-Ray scattering by periodic nanostructures
Y1  - 2000
ER  - 
TY  - JOUR
A1  - Pietsch, Ullrich
A1  - Tsirelson, Vladimir G.
A1  - Gorfan, S. V.
T1  - X-ray scattering amplitude of an atom in a permanent external electric field
Y1  - 2003
ER  - 
TY  - JOUR
A1  - Pietsch, Ullrich
A1  - Kubowicz, Stephan
A1  - Thünemann, Andreas F.
A1  - Geue, Thomas
A1  - Watson, M. D.
A1  - Tchebotareva, N.
A1  - Müllen, K.
T1  - X-ray reflectivity study of an amphiphilic hex-peri-hexabenzocoronene at a structured silicon wafer surface
Y1  - 2003
ER  - 
TY  - JOUR
A1  - Geue, Thomas
A1  - Henneberg, Oliver
A1  - Pietsch, Ullrich
T1  - X-ray reflectivity from sinusoidal surface relief gratings
Y1  - 2002
SN  - 0023-4753
ER  - 
TY  - JOUR
A1  - Pietsch, Ullrich
T1  - X-ray reflectivity from sinusoidal surface relief gratings
Y1  - 2002
ER  - 
TY  - JOUR
A1  - Poloucek, P.
A1  - Pietsch, Ullrich
A1  - Geue, Thomas
A1  - Symietz, Christian
A1  - Brezesinski, Gerald
T1  - X-ray reflectivity analysis of thin complex Langmuir-Blodgett films
Y1  - 2001
ER  - 
TY  - JOUR
A1  - Giewekemeyer, K.
A1  - Krueger, S. P.
A1  - Kalbfleisch, S.
A1  - Bartels, Meike
A1  - Beta, Carsten
A1  - Salditt, T.
T1  - X-ray propagation microscopy of biological cells using waveguides as a quasipoint source
JF  - Physical review : A, Atomic, molecular, and optical physics
N2  - We have used x-ray waveguides as highly confining optical elements for nanoscale imaging of unstained biological cells using the simple geometry of in-line holography. The well-known twin-image problem is effectively circumvented by a simple and fast iterative reconstruction. The algorithm which combines elements of the classical Gerchberg-Saxton scheme and the hybrid-input-output algorithm is optimized for phase-contrast samples, well-justified for imaging of cells at multi-keV photon energies. The experimental scheme allows for a quantitative phase reconstruction from a single holographic image without detailed knowledge of the complex illumination function incident on the sample, as demonstrated for freeze-dried cells of the eukaryotic amoeba Dictyostelium discoideum. The accessible resolution range is explored by simulations, indicating that resolutions on the order of 20 nm are within reach applying illumination times on the order of minutes at present synchrotron sources.
Y1  - 2011
U6  - https://doi.org/10.1103/PhysRevA.83.023804
SN  - 1050-2947
VL  - 83
IS  - 2
PB  - American Physical Society
CY  - College Park
ER  -