activity
19972008
most citedInitial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method

99 citations · 164 across the 3 of their papers we have counts for

collaborators
Showing gr-qcShow all

6 papers · 1 filter

gr-qc200822 cited

Ineffectiveness of Padé resummation techniques in post-Newtonian approximations

Abdul H. Mroué, Lawrence E. Kidder, Saul A. Teukolsky

We test the resummation techniques used in developing Padé and Effective One Body (EOB) waveforms for gravitational wave detection. Convergence tests show that Padé approximants of…

gr-qc200899 cited

Initial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method

Francois Foucart, Lawrence E. Kidder, Harald P. Pfeiffer +1

We present a new numerical scheme to solve the initial value problem for black hole-neutron star binaries. This method takes advantage of the flexibility and fast convergence of a…

gr-qc200743 cited

High accuracy simulations of Kerr tails: coordinate dependence and higher multipoles

Manuel Tiglio, Lawrence Kidder, Saul Teukolsky

We investigate the late time behavior of a scalar field on a fixed Kerr background using a 2+1 dimensional pseudospectral evolution code. We compare evolutions of pure axisymmetric…

gr-qc1999

An Efficient Method for Fully Relativistic Simulations of Coalescing Binary Neutron Stars

Walter Landry, Saul A. Teukolsky

The merger of two neutron stars has been proposed as a source of gamma-ray bursts, r-process elements, and detectable gravitational waves. Extracting information from observations…

gr-qc1998

Hot, Rotating Disks In General Relativity: Collisionless Equilibrium Models

A. Katrin Schenk, Stuart L. Shapiro, Saul A. Teukolsky

We present a method for constructing equilibrium disks with net angular momentum in general relativity. The method solves the relativistic Vlasov equation coupled to Einstein's equ…

gr-qc1997

Binary Neutron Stars in Quasi-Equilibrium Circular Orbit: A Fully Relativistic Treatment

Thomas W. Baumgarte, Stuart L. Shapiro, Gregory B. Cook +2

We present a numerical scheme that solves the initial value problem in full general relativity for a binary neutron star in quasi-equilibrium. While Newtonian gravity allows for a…