Showing 1–20 of 62 results
/ Date/ Name
May 6, 2010Binary Neutron Stars in Quasi-equilibriumMay 20, 2005Black hole-neutron star binaries in general relativity: effects of neutron star spinSep 15, 2006Quasiequilibrium sequences of black-hole--neutron-star binaries in general relativityMar 30, 2005Merger of binary neutron stars with realistic equations of state in full general relativityOct 26, 2007Relativistic black hole-neutron star binaries in quasiequilibrium: effects of the black hole excision boundary conditionJul 25, 2002Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. III. Identical and different mass stars with gamma=2Jan 19, 2007Quasiequilibrium black hole-neutron star binaries in general relativityOct 3, 2014Quasiequilibrium sequences of binary neutron stars undergoing dynamical scalarizationMar 6, 2006Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringingAug 9, 2010Gravitational waves from nonspinning black hole-neutron star binaries: dependence on equations of stateFeb 3, 2009Gravitational waves from black hole-neutron star binaries I: Classification of waveformsSep 8, 2020Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture frameworkDec 2, 2004The final phase of inspiral of neutron stars: realistic equations of stateDec 14, 2007Fully General Relativistic Simulations of Black Hole-Neutron Star MergersMar 28, 2008General relativistic simulations of magnetized binary neutron star mergersMar 12, 2004Collision dynamics of two barchan dunes simulated by a simple modelJun 22, 2015High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burstOct 2, 2013Coalescence of binary neutron stars in a scalar-tensor theory of gravitySep 10, 1998Irrotational and Incompressible Ellipsoids in the First Post-Newtonian Approximation of General RelativityJul 2, 1998Gravitational radiation from corotating binary neutron stars of incompressible fluid in the first post-Newtonian approximation of general relativity