output
20022008
most citedThumbs up? Sentiment Classification using Machine Learning Techniques

2.2k citations

Showing 2007 · gr-qcShow all

7 papers · 2 filters

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-qc2007175 cited

Using Full Information When Computing Modes of Post-Newtonian Waveforms From Inspiralling Compact Binaries in Circular Orbit

Lawrence E. Kidder

The increasing sophistication and accuracy of numerical simulations of compact binaries (especially binary black holes) presents the opportunity to test the regime in which post-Ne…

gr-qc200721 cited

Numerical Simulations of Oscillating Soliton Stars: Excited States in Spherical Symmetry and Ground State Evolutions in 3D

Jayashree Balakrishna, Ruxandra Bondarescu, Gregory Daues +1

Excited state soliton stars are studied numerically for the first time. The stability of spherically symmetric S-branch excited state oscillatons under radial perturbations is inve…

gr-qc20073 cited

Finite Mirror Effects in Advanced Interferometric Gravitational Wave Detectors

Andrew P. Lundgren, Ruxandra Bondarescu, David Tsang +1

Thermal noise is expected to be the dominant source of noise in the most sensitive frequency band of second generation ground based gravitational wave detectors. Reshaping the beam…

gr-qc200763 cited

Can Gravity Probe B usefully constrain torsion gravity theories?

Eanna E. Flanagan, Eran Rosenthal

In most theories of gravity involving torsion, the source for torsion is the intrinsic spin of matter. Since the spins of fermions are normally randomly oriented in macroscopic bod…

gr-qc200750 cited

A generalization of Ryan's theorem: probing tidal coupling with gravitational waves from nearly circular, nearly equatorial, extreme-mass-ratio inspirals

Chao Li, Geoffrey Lovelace

Extreme-mass-ratio inspirals (EMRIs) and intermediate-mass-ratio inspirals (IMRIs)--binaries in which a stellar-mass object spirals into a massive black hole or other massive, comp…