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Coalescence of black hole-neutron star binaries
We review the current status of general relativistic studies for the coalescence of black hole-
neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi …
neutron star (BH-NS) binaries. First, procedures for a solution of BH-NS binaries in quasi …
Astrophysical smooth particle hydrodynamics
The paper presents a detailed review of the smooth particle hydrodynamics (SPH) method
with particular focus on its astrophysical applications. We start by introducing the basic ideas …
with particular focus on its astrophysical applications. We start by introducing the basic ideas …
Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts,<? format?> and quasinormal mode ringing
Three-dimensional simulations for the merger of binary neutron stars are performed in the
framework of full general relativity. We pay particular attention to the black hole formation …
framework of full general relativity. We pay particular attention to the black hole formation …
Neutrino signatures and the neutrino-driven wind in binary neutron star mergers
L Dessart, CD Ott, A Burrows, S Rosswog… - The Astrophysical …, 2008 - iopscience.iop.org
We present VULCAN/2D multigroup flux-limited-diffusion radiation-hydrodynamics
simulations of binary neutron star mergers, using the Shen equation of state, covering≳ 100 …
simulations of binary neutron star mergers, using the Shen equation of state, covering≳ 100 …
Merger of binary neutron stars with realistic equations of state in full general relativity
We present numerical results of three-dimensional simulations for the merger of binary
neutron stars in full general relativity. Hybrid equations of state are adopted to mimic realistic …
neutron stars in full general relativity. Hybrid equations of state are adopted to mimic realistic …
High-resolution calculations of merging neutron stars—II. Neutrino emission
The remnant resulting from the merger of two neutron stars produces neutrinos in copious
amounts. In this paper we present the neutrino emission results obtained via Newtonian …
amounts. In this paper we present the neutrino emission results obtained via Newtonian …
Relativistic neutron star merger simulations with non-zero temperature equations of state-I. Variation of binary parameters and equation of state
An extended set of binary neutron star (NS) merger simulations is performed with an
approximative treatment of general relativity to systematically investigate the influence of the …
approximative treatment of general relativity to systematically investigate the influence of the …
An overview of gravitational-wave sources
C Cutler, KS Thorne - General Relativity and Gravitation, 2002 - World Scientific
AN OVERVIEW OF GRAVITATIONAL-WAVE SOURCES CURT CUTLER Max Planck Institute for
Gravitational Physics, 14476 Golm, Germany KIP S. Page 1 AN OVERVIEW OF …
Gravitational Physics, 14476 Golm, Germany KIP S. Page 1 AN OVERVIEW OF …
Merger of binary neutron stars of unequal mass in full general relativity
We present results of three dimensional numerical simulations of the merger of unequal-
mass binary neutron stars in full general relativity. A Γ-law equation of state P=(Γ− 1) ρ ɛ is …
mass binary neutron stars in full general relativity. A Γ-law equation of state P=(Γ− 1) ρ ɛ is …
Coalescing neutron stars-A step towards physical models-III. Improved numerics and different neutron star masses and spins
In this paper we present a compilation of results from our most advanced neutron star
merger simulations. Special aspects of these models were refered to in earlier publications …
merger simulations. Special aspects of these models were refered to in earlier publications …