Publications

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188 Publications visible to you, out of a total of 188

Abstract

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Authors: Richard Miller, Marco Ajello, Katie Auchettl, John Beacom, Peter Bloser, Adam Burrows, Anna Frebel, Chris Fryer, Dieter Hartmann, Peter Hoeflich, Aimee Hungerford, Mark Leising, Laura Lopez, Peter Milne, Patrick Peplowski, Friedrich Roepke, Daniel Scolnic, Ivo Seitenzahl, Lih-Sin The, C. Alex Young, LOX Team

Date Published: 1st Apr 2022

Publication Type: InProceedings

Abstract

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Authors: R. Andrassy, J. Higl, H. Mao, M. Mocák, D. G. Vlaykov, W. D. Arnett, I. Baraffe, S. W. Campbell, T. Constantino, P. V. F. Edelmann, T. Goffrey, T. Guillet, F. Herwig, R. Hirschi, L. Horst, G. Leidi, C. Meakin, J. Pratt, F. Rizzuti, F. K. Röpke, P. Woodward

Date Published: 1st Mar 2022

Publication Type: Journal

Abstract

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Authors: F. Lach, F. P. Callan, S. A. Sim, F. K. Röpke

Date Published: 1st Mar 2022

Publication Type: Journal

Abstract

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Authors: Theodoros Soultanis, Andreas Bauswein, Nikolaos Stergioulas

Date Published: 1st Feb 2022

Publication Type: Journal

Abstract

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Authors: F. Lach, F. P. Callan, D. Bubeck, F. K. Röpke, S. A. Sim, M. Schrauth, S. T. Ohlmann, M. Kromer

Date Published: 1st Feb 2022

Publication Type: Journal

Abstract

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Authors: Umberto Battino, Claudia Lederer-Woods, Claudia Travaglio, Friedrich Konrad Röpke, Brad Gibson

Date Published: 2022

Publication Type: Journal

Abstract (Expand)

This thesis presents multidimensional hydrodynamic simulations of stellar interiors with a focus on dynamical phenomena at low Mach numbers using the Seven-League Hydro (SLH) code. A better understanding of these phenomena is crucial to improve the modeling of stellar evolution. It is demonstrated that suitable numerical methods are required to avoid that numerical artifacts and spurious dissipation dominate the actual physical flow. Three-dimensional simulations of convective helium shell burning are used to measure the entrainment of mass into the convective region. This aids the parametrization of entrainment in one-dimensional evolution calculations. Furthermore, the excitation of waves by core convection is simulated and the results are analyzed regarding their physical plausibility and agreement with observations. These simulations demonstrate that the current set of numerical methods used by the SLH code is promising regarding future, more realistic simulations of astrophysical flows.

Author: Leonhard Horst

Date Published: 10th Dec 2021

Publication Type: Doctoral Thesis

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