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Early sensitivity to prosodic phrase boundary cues: Behavioral evidence from German-learning infants
(2023)
This dissertation seeks to shed light on the relation of phrasal prosody and developmental speech perception in German-learning infants. Three independent empirical studies explore the role of acoustic correlates of major prosodic boundaries, specifically pitch change, final lengthening, and pause, in infant boundary perception. Moreover, it was examined whether the sensitivity to prosodic phrase boundary markings changes during the first year of life as a result of perceptual attunement to the ambient language (Aslin & Pisoni, 1980).
Using the headturn preference procedure six- and eight-month-old monolingual German-learning infants were tested on their discrimination of two different prosodic groupings of the same list of coordinated names either with or without an internal IPB after the second name, that is, [Moni und Lilli] [und Manu] or [Moni und Lilli und Manu]. The boundary marking was systematically varied with respect to single prosodic cues or specific cue combinations.
Results revealed that six- and eight-month-old German-learning infants successfully detect the internal prosodic boundary when it is signaled by all the three main boundary cues pitch change, final lengthening, and pause. For eight-, but not for six-month-olds, the combination of pitch change and final lengthening, without the occurrence of a pause, is sufficient. This mirrors an adult-like perception by eight-months (Holzgrefe-Lang et al., 2016). Six-month-olds detect a prosodic phrase boundary signaled by final lengthening and pause. The findings suggest a developmental change in German prosodic boundary cue perception from a strong reliance on the pause cue at six months to a differentiated sensitivity to the more subtle cues pitch change and final lengthening at eight months. Neither for six- nor for eight-month-olds the occurrence of pitch change or final lengthening as single cues is sufficient, similar to what has been observed for adult speakers of German (Holzgrefe-Lang et al., 2016).
The present dissertation provides new scientific knowledge on infants’ sensitivity to individual prosodic phrase boundary cues in the first year of life. Methodologically, the studies are pathbreaking since they used exactly the same stimulus materials – phonologically thoroughly controlled lists of names – that have also been used with adults (Holzgrefe-Lang et al., 2016) and with infants in a neurophysiological paradigm (Holzgrefe-Lang, Wellmann, Höhle, & Wartenburger, 2018), allowing for comparisons across age (six/ eight months and adults) and method (behavioral vs. neurophysiological methods). Moreover, materials are suited to be transferred to other languages allowing for a crosslinguistic comparison. Taken together with a study with similar French materials (van Ommen et al., 2020) the observed change in sensitivity in German-learning infants can be interpreted as a language-specific one, from an initial language-general processing mechanism that primarily focuses on the presence of pauses to a language-specific processing that takes into account prosodic properties available in the ambient language. The developmental pattern is discussed as an interplay of acoustic salience, prosodic typology (prosodic regularity) and cue reliability.
In X-ray computed tomography (XCT), an X-ray beam of intensity I0 is transmitted through an object and its attenuated intensity I is measured when it exits the object. The attenuation of the beam depends on the attenuation coefficients along its path. The attenuation coefficients provide information about the structure and composition of the object and can be determined through mathematical operations that are referred to as reconstruction.
The standard reconstruction algorithms are based on the filtered backprojection (FBP) of the measured data. While these algorithms are fast and relatively simple, they do not always succeed in computing a precise reconstruction, especially from under-sampled data.
Alternatively, an image or volume can be reconstructed by solving a system of linear equations. Typically, the system of equations is too large to be solved but its solution can be approximated by iterative methods, such as the Simultaneous Iterative Reconstruction Technique (SIRT) and the Conjugate Gradient Least Squares (CGLS).
This dissertation focuses on the development of a novel iterative algorithm, the Direct Iterative Reconstruction of Computed Tomography Trajectories (DIRECTT). After its reconstruction principle is explained, its performance is assessed for real parallel- and cone-beam CT (including under-sampled) data and compared to that of other established algorithms. Finally, it is demonstrated how the shape of the measured object can be modelled into DIRECTT to achieve even better reconstruction results.
Investment control has experienced a considerable increase in importance in M&A transactions, as it has been constantly adapted to real economic conditions and successively tightened. The result is a partially inconsistent review regime that contains value contradictions and creates legal uncertainties. In a comprehensive approach, this doctoral thesis analyzes the problems of the current investment control regime and states concrete reform proposals.
In der vorliegenden Arbeit liegt der Fokus auf jungen russischsprachigen Jüdinnen und Juden, deren Eltern in den 90er Jahren des 20 Jahrhunderts nach Deutschland eingewandert sind. Im Rahmen dieser Studie wird der Bildungsweg dieser MigrantInnengruppe und deren Erfahrungen in Deutschland aus der biographischen Perspektive nachvollzogen. Der Fokus wird insbesondere auf die biographischen Lebenserfahrungen gelegt, d.h. die allgemeinen Lebensumstände, Hürden und Schwierigkeiten, die die jungen russischsprachigen Jüdinnen und Juden in Deutschland überwinden mussten, um auf ihrem Bildungsweg an ihr Ziel zu kommen. Des Weiteren werden die Rolle des sozialen Umfelds auf die Auswahl ihres Bildungsweges sowie ihre Zugehörigkeit und ihr Beitrag zur deutschen Gesellschaft beleuchtet. Ein weiteres Hauptaugenmerk dieser Arbeit liegt auf den gesellschaftlichen, politischen und familiären Rahmenbedingungen, die den BiographInnen den Zugang zum Bildungsweg ermöglichten.
Die in der Arbeit formulierten Forschungsfragen wurden mithilfe der interpretativen Sozialforschung, genauer, der fallrekonstruktiven Auswertung nach Gabriele Rosenthal beantwortet.
Über den biographischen Verlauf der Lebensgeschichte der jungen russischsprachigen Jüdinnen und Juden wurde deutlich, dass die BiographInnen in die säkulare Gesellschaft gehen müssen, um ihren Bildungsweg erfolgreich zu gestalten. Dort erfahren sie einen sehr starken Antisemitismus und sind diesem schutzlos ausgeliefert. Bei allen drei Interviewten wurde diese Erfahrung in der Schule gemacht, an einem Ort, an dem sie Schutz erfahren sollten. Diesen Anfeindungen begegneten sie auf unterschiedliche Weise und sie entwickelten verschiedene Handlungsstrategien. Einige BiographInnen setzen sich auf der intellektuellen Ebene bewusst damit auseinander, andere wiederum versuchen, nicht hinzuschauen und es zu ignorieren.
Des Weiteren wurde als Resultat der Untersuchung in einigen Fällen ein übereinstimmendes, in anderen ein nicht übereinstimmendes Passungsverhältnis zwischen elterlichen Vorstellungen und den Bildungswegen der jungen russischsprachigen Jüdinnen und Juden gefunden.
Cosmic rays (CRs) constitute an important component of the interstellar medium (ISM) of galaxies and are thought to play an essential role in governing their evolution. In particular, they are able to impact the dynamics of a galaxy by driving galactic outflows or heating the ISM and thereby affecting the efficiency of star-formation. Hence, in order to understand galaxy formation and evolution, we need to accurately model this non-thermal constituent of the ISM. But except in our local environment within the Milky Way, we do not have the ability to measure CRs directly in other galaxies. However, there are many ways to indirectly observe CRs via the radiation they emit due to their interaction with magnetic and interstellar radiation fields as well as with the ISM.
In this work, I develop a numerical framework to calculate the spectral distribution of CRs in simulations of isolated galaxies where a steady-state between injection and cooling is assumed. Furthermore, I calculate the non-thermal emission processes arising from the modelled CR proton and electron spectra ranging from radio wavelengths up to the very high-energy gamma-ray regime.
I apply this code to a number of high-resolution magneto-hydrodynamical (MHD) simulations of isolated galaxies, where CRs are included. This allows me to study their CR spectra and compare them to observations of the CR proton and electron spectra by the Voyager-1 satellite and the AMS-02 instrument in order to reveal the origin of the measured spectral features.
Furthermore, I provide detailed emission maps, luminosities and spectra of the non-thermal emission from our simulated galaxies that range from dwarfs to Milk-Way analogues to starburst galaxies at different evolutionary stages. I successfully reproduce the observed relations between the radio and gamma-ray luminosities with the far-infrared (FIR) emission of star-forming (SF) galaxies, respectively, where the latter is a good tracer of the star-formation rate. I find that highly SF galaxies are close to the limit where their CR population would lose all of their energy due to the emission of radiation, whereas CRs tend to escape low SF galaxies more quickly. On top of that, I investigate the properties of CR transport that are needed in order to match the observed gamma-ray spectra.
Furthermore, I uncover the underlying processes that enable the FIR-radio correlation (FRC) to be maintained even in starburst galaxies and find that thermal free-free-emission naturally explains the observed radio spectra in SF galaxies like M82 and NGC 253 thus solving the riddle of flat radio spectra that have been proposed to contradict the observed tight FRC.
Lastly, I scrutinise the steady-state modelling of the CR proton component by investigating for the first time the influence of spectrally resolved CR transport in MHD simulations on the hadronic gamma-ray emission of SF galaxies revealing new insights into the observational signatures of CR transport both spectrally and spatially.