activity
19932005
most cited3D Hydrodynamic Simulations of Relativistic Extragalactic Jets

69 citations · 346 across the 16 of their papers we have counts for

collaborators

16 papers

gr-qc2005★ 5 cited

General Relativistic Decompression of Binary Neutron Stars During Dynamic Inspiral

Mark Miller

We investigate the dynamic stability of inspiraling neutron stars by performing multiple-orbit numerical relativity simulations of the binary neutron star inspiral process. By intr…

gr-qc2005★ 35 cited

Accuracy requirements for the calculation of gravitational waveforms from coalescing compact binaries in numerical relativity

Mark Miller

I discuss the accuracy requirements on numerical relativity calculations of inspiraling compact object binaries whose extracted gravitational waveforms are to be used as templates…

gr-qc2003★ 67 cited

Towards a Realistic Neutron Star Binary Inspiral: Initial Data and Multiple Orbit Evolution in Full General Relativity

Mark Miller, Philip Gressman, Wai-Mo Suen

This paper reports on our effort in modeling realistic astrophysical neutron star binaries in general relativity. We analyze under what conditions the conformally flat quasiequilib…

gr-qc2003★ 19 cited

On the Circular Orbit Approximation for Binary Compact Objects In General Relativity

Mark Miller

One often-used approximation in the study of binary compact objects (i.e., black holes and neutron stars) in general relativity is the instantaneously circular orbit assumption. Th…

gr-qc2003★ 1 cited

Towards a Realistic Neutron Star Binary Inspiral

Mark Miller, Wai-Mo Suen

An approach to general relativity based on conformal flatness and quasiequilibrium (CFQE) assumptions has played an important role in the study of the inspiral dynamics and in prov…

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…