Merging Neutron Stars and Black Holes as Sources of Gamma-Ray Bursts and   Heavy Elements
  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. 
H.-Th. Janka (MPI f. Astrophysik), M. Ruffert (Univ. of Edinburgh), T.   Eberl (MPI f. Astrophysik)