Showing 1–14 of 14 results
/ Date/ Name
Jul 19, 2013Prompt merger collapse and the maximum mass of neutron starsJan 15, 2002Illustrating Stability Properties of Numerical Relativity in ElectrodynamicsSep 10, 2001A numerical testbed for singularity excision in moving black hole spacetimesMay 8, 1999Constructing a Mass-Current Radiation-Reaction Force For Numerical SimulationsSep 30, 2008Equilibrium initial data for moving puncture simulations: The stationary 1+log slicingMay 8, 1998Stability of coalescing binary stars against gravitational collapse: hydrodynamical simulationsSep 30, 1997Gravitational wave extraction and outer boundary conditions by perturbative matchingJul 28, 1999Implementing fully relativistic hydrodynamics in three dimensionsNov 12, 2004The Moment of Inertia of the Binary Pulsar J0737-3039A: Constraining the Nuclear Equation of StateDec 8, 1997Waveform propagation in black hole spacetimes: evaluating the quality of numerical solutionsMay 10, 1997The Stability of Relativistic Neutron Stars in Binary OrbitApr 8, 1997Binary Neutron Stars in General Relativity: Quasi-Equilibrium ModelsNov 26, 1997Boosted three-dimensional black-hole evolutions with singularity excisionSep 11, 1997General Relativistic Models of Binary Neutron Stars in Quasiequilibrium