Zobrazeno 1 - 10
of 778
pro vyhledávání: '"Horst, L."'
Autor:
Andrassy, R., Higl, J., Mao, H., Mocák, M., Vlaykov, D. G., Arnett, W. D., Baraffe, I., Campbell, S. W., Constantino, T., Edelmann, P. V. F., Goffrey, T., Guillet, T., Herwig, F., Hirschi, R., Horst, L., Leidi, G., Meakin, C., Pratt, J., Rizzuti, F., Roepke, F. K., Woodward, P.
Publikováno v:
A&A 659, A193 (2022)
Our ability to predict the structure and evolution of stars is in part limited by complex, 3D hydrodynamic processes such as convective boundary mixing. Hydrodynamic simulations help us understand the dynamics of stellar convection and convective bou
Externí odkaz:
http://arxiv.org/abs/2111.01165
Publikováno v:
A&A 653, A55 (2021)
Context. Multidimensional hydrodynamic simulations of convection in stellar interiors are numerically challenging, especially for flows at low Mach numbers. Methods. We explore the benefits of using a low-Mach hydrodynamic flux solver and demonstrate
Externí odkaz:
http://arxiv.org/abs/2107.02199
Autor:
Bijlsma, M.W., Citroen, J., van Geel, B.M., Groeneveld, N.S., Heckenberg, S.G.B., Jellema, K., Kester, M.I., Killestein, J., Mook, B.B., Resok, Y.C., Olie, S.E., Staal, S.L., Titulaer, M.J., van Veen, K.E.B., van Zeggeren, I.E., Pennartz, C.J., ter Horst, L., van de Beek, D., Brouwer, M.C.
Publikováno v:
In Journal of Hospital Infection March 2024 145:99-105
Publikováno v:
In Safety Science February 2024 170
Autor:
Edelmann, P. V. F., Horst, L., Berberich, J. P., Andrassy, R., Higl, J., Leidi, G., Klingenberg, C., Roepke, F. K.
Publikováno v:
A&A 652, A53 (2021)
Accurate simulations of flows in stellar interiors are crucial to improving our understanding of stellar structure and evolution. Because the typically slow flows are merely tiny perturbations on top of a close balance between gravity and the pressur
Externí odkaz:
http://arxiv.org/abs/2102.13111
Autor:
Bowman, D. M., Burssens, S., Simón-Díaz, S., Edelmann, P. V. F., Rogers, T. M., Horst, L., Roepke, F. K., Aerts, C.
Publikováno v:
A&A 640, A36 (2020)
Context. Massive stars are predicted to excite internal gravity waves (IGWs) by turbulent core convection and from turbulent pressure fluctuations in their near-surface layers. These IGWs are extremely efficient at transporting angular momentum and c
Externí odkaz:
http://arxiv.org/abs/2006.03012
Autor:
Horst, L., Edelmann, P. V. F., Andrassy, R., Roepke, F. K., Bowman, D. M., Aerts, C., Ratnasingam, R. P.
Publikováno v:
A&A 641, A18 (2020)
Context. Recent, nonlinear simulations of wave generation and propagation in full-star models have been carried out in the anelastic approximation using spectral methods. Although it makes long time steps possible, this approach excludes the physics
Externí odkaz:
http://arxiv.org/abs/2006.03011
Publikováno v:
In Safety Science May 2023 161
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When electrons are confined in two dimensions and subjected to strong magnetic fields, the Coulomb interactions between them become dominant and can lead to novel states of matter such as fractional quantum Hall liquids. In these liquids electrons li
Externí odkaz:
http://arxiv.org/abs/0910.2763