Merging Neutron Stars and Black Holes as Sources of Gamma-Ray Bursts and Heavy Elements

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dc.creatorJanka, H. -Th.
dc.creatorRuffert, M.
dc.creatorEberl, T.
dc.date1998-10-05
dc.date.accessioned2026-07-07T02:28:12Z
dc.date.available2026-07-07T02:28:12Z
dc.descriptionHydrodynamic simulations were performed of the dynamical phase of the merging of binary neutron stars (NS-NS) and of neutron star black hole binaries (NS-BH), using the physical nuclear equation of state of Lattimer and Swesty (1991) and taking into account the emission of gravitational waves and neutrinos.
dc.description4 pages, 4 ps figures, submitted to Editions Frontieres (France), Nuclei in the Cosmos V
dc.identifierhttps://arxiv.org/abs/astro-ph/9810057
dc.identifierhttp://arxiv.org/abs/astro-ph/9810057
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13024
dc.subjectAstrophysics
dc.titleMerging Neutron Stars and Black Holes as Sources of Gamma-Ray Bursts and Heavy Elements
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