Merging Neutron Stars and Black Holes as Sources of Gamma-Ray Bursts and Heavy Elements
arXiv:astro-ph/9810057
Abstract
Hydrodynamic 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.
4 pages, 4 ps figures, submitted to Editions Frontieres (France), Nuclei in the Cosmos V