14.2k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR1.2k papers
- California Institute of TechnologyUS1k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR744 papers
- University of CambridgeGB676 papers
- University College LondonGB641 papers
- University of TorontoCA603 papers
- National Institute for AstrophysicsIT595 papers
- Sapienza University of RomeIT578 papers
- Stanford UniversityUS550 papers
- European Southern ObservatoryCL540 papers
- Jet Propulsion LaboratoryUS533 papers
- University of ManchesterGB523 papers
8 papers · 2 filters
Gravitational waves from black hole binary inspiral and merger: The span of third post-Newtonian effective-one-body templates
Thibault Damour, Bala R. Iyer, Piotr Jaranowski +1
We extend the description of gravitational waves emitted by binary black holes during the final stages of inspiral and merger by introducing in the third post-Newtonian (3PN) effec…
Finite-Range Gravity and Its Role in Gravitational Waves, Black Holes and Cosmology
Stanislav V. Babak, L. P. Grishchuk
Theoretical considerations of fundamental physics, as well as certain cosmological observations, persistently point out to permissibility, and maybe necessity, of macroscopic modif…
A comparison of search templates for gravitational waves from binary inspiral - 3.5PN update
Thibault Damour, Bala R. Iyer, B. S. Sathyaprakash
Phasing formulas in a recent paper of ours' (Phys. Rev. D 63, 044023-1 (2001) are updated taking into account the recent 3.5PN results. Some misprints in the published version of t…
Approximating the inspiral of test bodies into Kerr black holes
Kostas Glampedakis, Scott A. Hughes, Daniel Kennefick
We present a new approximate method for constructing gravitational radiation driven inspirals of test-bodies orbiting Kerr black holes. Such orbits can be fully described by a semi…
Zoom & Whirl: Eccentric equatorial orbits around spinning black holes and their evolution under gravitational radiation reaction
Kostas Glampedakis, Daniel Kennefick
We study eccentric equatorial orbits of a test-body around a Kerr black hole under the influence of gravitational radiation reaction. We have adopted a well established two-step ap…
Computational Resources to Filter Gravitational Wave Data with P-approximant Templates
Edward K. Porter
The prior knowledge of the gravitational waveform from compact binary systems makes matched filtering an attractive detection strategy. This detection method involves the filtering…
Celestial mechanics in Kerr spacetime
Wolfram Schmidt
The dynamical parameters conventionally used to specify the orbit of a test particle in Kerr spacetime are the energy , the axial component of the angular momentum, , and…
The Early Universe Odyssey With Gravitational Waves
L. P. Grishchuk
This contribution summarizes some recent work on gravitational-wave astronomy and, especially, on the generation and detection of relic gravitational waves. We begin with a brief d…