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TABLE I. Summary. b is the density at bounce, the maximum characteristic GW strain hchar;max is at a distance of 10 kpc, and Egw is the energy emitted in GWs. Values for E20Apb include GW emission from late-time 3D dynamics.
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Journal Article
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DOI
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3D collapse of rotating stellar iron cores in general relativity including deleptonization and a nuclear equation of state.
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Christian D. Ott
1
,
Harald Dimmelmeier
1
,
Andreas Marek
1
,
Hans-Thomas Janka
1
,
Ian Hawke
1
,
Burkhard Zink
1
,
Erik Schnetter
1
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+3 more
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Institutions (1)
Max Planck Society
1
29 Jun 2007
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Physical Review Letters