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19922007
most citedThree-dimensional general relativistic hydrodynamics II: long-term dynamics of single relativistic stars

202 citations · 322 across the 10 of their papers we have counts for

collaborators

10 papers

gr-qc2007★ 38 cited

A post-Newtonian diagnosis of quasiequilibrium configurations of neutron star-neutron star and neutron star-black hole binaries

Emanuele Berti, Sai Iyer, Clifford M. Will

We use a post-Newtonian diagnostic tool to examine numerically generated quasiequilibrium initial data sets for non-spinning double neutron star and neutron star-black hole binary…

gr-qc2006★ 20 cited

Eccentricity content of binary black hole initial data

Emanuele Berti, Sai Iyer, Clifford M. Will

Using a post-Newtonian diagnostic tool developed by Mora and Will, we examine numerically generated quasiequilibrium initial data sets that have been used in recently successful nu…

gr-qc2005★ 12 cited

Computational Relativistic Astrophysics With Adaptive Mesh Refinement: Testbeds

Edwin Evans, Sai Iyer, Erik Schnetter +4

We have carried out numerical simulations of strongly gravitating systems based on the Einstein equations coupled to the relativistic hydrodynamic equations using adaptive mesh ref…

gr-qc2003★ 5 cited

Head-on/Near Head-on Collisions of Neutron Stars With a Realistic EOS

Edwin Evans, A. Gopakumar, Philip Gressman +4

It has been conjectured that in head-on collisions of neutron stars (NSs), the merged object would not collapse promptly even if the total mass is higher than the maximum stable ma…

gr-qc2001★ 202 cited

Three-dimensional general relativistic hydrodynamics II: long-term dynamics of single relativistic stars

J. Font, T. Goodale, S. Iyer +6

This is the second in a series of papers on the construction and validation of a three-dimensional code for the solution of the coupled system of the Einstein equations and of the…

gr-qc2000★ 6 cited

Padé approximants for truncated post-Newtonian neutron star models

Anshu Gupta, A. Gopakumar, Bala R. Iyer +1

Padé approximants to truncated post-Newtonian neutron star models are constructed. The Padé models converge faster to the general relativistic (GR) solution than the truncated post…