The gravitational wave burst signal from core collapse of rotating stars

We present results from detailed general relativistic simulations of stellar core collapse to a proto-neutron star, using two different microphysical nonzero-temperature nuclear equations of state as well as an approximate description of deleptonization during the collapse phase. Investigating a wid...

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Veröffentlicht in:	arXiv.org 2008-08
Hauptverfasser:	Dimmelmeier, Harald, Ott, Christian D, Marek, Andreas, Hans-Thomas, Janka
Format:	Artikel
Sprache:	eng
Schlagworte:	Computer simulation Data analysis Differential rotation Dynamic stability Equations of state Gravitation Gravitational collapse Gravitational waves Mathematical models Model accuracy Morphology Neutron stars Neutrons Peak frequency Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Stars Stellar rotation Supernovae
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