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20012004
most citedA Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Space-Time

302 citations · 583 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2004★ 68 cited

The Influence of Quark Matter at High Densities on Binary Neutron Star Mergers

R. Oechslin, K. Uryū, G. Poghosyan +1

We consider the influence of potential quark matter existing at high densities in neutron star interiors on gravitational waves (GW) emitted in a binary neutron star merger event.…

astro-ph2002★ 69 cited

The Neutrino Signal in Stellar Core Collapse and Postbounce Evolution

M. Liebendoerfer, A. Mezzacappa, O. E. B. Messer +3

General relativistic multi-group and multi-flavor Boltzmann neutrino transport in spherical symmetry adds a new level of detail to the numerical bridge between microscopic nuclear…

astro-ph2002★ 302 cited

A Finite Difference Representation of Neutrino Radiation Hydrodynamics in Spherically Symmetric General Relativistic Space-Time

M. Liebendoerfer, O. E. B. Messer, A. Mezzacappa +3

We present an implicit finite difference representation for general relativistic radiation hydrodynamics in spherical symmetry. Our code, Agile-Boltztran, solves the Boltzmann tran…

astro-ph2002

The importance of neutrino opacities for the accretion luminosity in spherically symmetric supernova models

M. Liebendoerfer, O. E. B. Messer, A. Mezzacappa +3

Based on general relativistic three-flavor Boltzmann neutrino transport, we compare simulations of the postbounce evolution for five different stellar progenitors with 13 and 20 so…

gr-qc2001★ 144 cited

Conformally Flat Smoothed Particle Hydrodynamics: Application to Neutron Star Mergers

Roland Oechslin, Stephan Rosswog, Friederich-Karl Thielemann

We present a new 3D SPH code which solves the general relativistic field + hydrodynamics equations in the conformally flat approximation. Several test cases are considered to test…