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clustering from HSC, LSST, and Roman • Development of cosmological simulations incorporating primordial non-Gaussianity (PNG) • Construction of cosmological emulators for cluster observables, including
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to be involved in academic activities of the High-Energy-Theory group (https://www.phys.sinica.edu.tw/group_hep_theory_en.php ) and encouraged to collaborate and interact with other research groups in
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supervisor. Possible present or future connections to his research are appreciated. Structure of the Research Group The group usually consists of around two MSc students, two PhD students, and two
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, including structural, diffusion, and resting-state functional MRI data, while additional multimodal datasets are currently being collected (including neuroimaging, actigraphy, electroretinography
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programme without teaching duties; it belongs to the research group of Ulrich Menne who acts as supervisor. Possible present or future connections to his research are appreciated. Structure of the research
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the initial conditions of the Big Bang to the formation of the large-scale structure in the late universe (and many things in between). The center contains both groups focussing on theoretical research and
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Sinica are possible, which add an individual research budget and may increase the salary for exceptional candidates. Successful candidates are encouraged to collaborate and interact with other research
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, Condensed Matter Theory , Nanoscience , Nonlinear and Complex Systems , Quantum many-body structure and their manipulation , Statistical physics Appl Deadline: 2026/03/31 11:59PM (posted 2025/08/27, listed