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Exploring the relativistic regime with Newtonian hydrodynamics: an improved effective gravitational potential for supernova simulations

MPS-Authors
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Marek,  A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Dimmelmeier,  H.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Janka,  H.-Th.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Müller,  E.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Buras,  R.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Marek, A., Dimmelmeier, H., Janka, H.-T., Müller, E., & Buras, R. (2006). Exploring the relativistic regime with Newtonian hydrodynamics: an improved effective gravitational potential for supernova simulations. Astronomy & Astrophysics, 445(1), 273-289. doi:10.1051/0004-6361:20052840.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-B042-9
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