S
Simon Scheidegger
Researcher at University of Lausanne
Publications - 40
Citations - 959
Simon Scheidegger is an academic researcher from University of Lausanne. The author has contributed to research in topics: Neutrino & Gravitational wave. The author has an hindex of 15, co-authored 39 publications receiving 822 citations. Previous affiliations of Simon Scheidegger include University of Zurich & Hoover Institution.
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The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
TL;DR: In this paper, the authors present the analysis of an extensive series of 3D MHD core-collapse simulations, which are launched from a 15 solar mass progenitor, a spherically symmetric effective general relativistic potential, and a neutrino parametrisation scheme which is accurate until about 5ms postbounce.
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The influence of model parameters on the prediction of gravitational wave signals from stellar core collapse
TL;DR: In this article, the effects of the equation of state, the initial rotation rate, and both the toroidal and the poloidal magnetic fields on the GW signature were investigated in an extensive series of three-dimensional magnetohydrodynamical core-collapse simulations.
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Gravitational waves from 3D MHD core collapse simulations
TL;DR: In this article, the Lattimer-Swesty equation of state for hot, dense matter and a neutrino parametrisation scheme were used to simulate core collapse supernova.
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Using Adaptive Sparse Grids to Solve High-Dimensional Dynamic Models
Johannes Brumm,Simon Scheidegger +1 more
TL;DR: This work presents a flexible and scalable method for computing global solutions of high‐dimensional stochastic dynamic models, combining distributed and shared memory parallelization paradigms, and thus permits an efficient use of high-performance computing architectures.
Journal ArticleDOI
Gravitational waves from 3D MHD core collapse simulations
TL;DR: In this paper, the Lattimer-Swesty equation of state for hot, dense matter and a neutrino parametrisation scheme were used to simulate core collapse supernova.