output
19962026
most citedObservation of Gravitational Waves from a Binary Black Hole Merger

14.2k citations

Showing 2009 · gr-qcShow all

24 papers · 2 filters

gr-qc2009★ 43 cited

All Vacuum Near-Horizon Geometries in -dimensions with Commuting Rotational Symmetries

Stefan Hollands, Akihiro Ishibashi

We explicitly construct all stationary, non-static, extremal near horizon geometries in dimensions that satisfy the vacuum Einstein equations, and that have commuting rot…

gr-qc2009★ 625 cited

Inspiral-merger-ringdown waveforms for black-hole binaries with non-precessing spins

P. Ajith, M. Hannam, S. Husa +9

We present the first analytical inspiral-merger-ringdown gravitational waveforms from binary black holes (BBHs) with non-precessing spins, that is based on a description of the lat…

gr-qc2009★ 10 cited

Current status of gravitational-wave observations

Stephen Fairhurst, Gianluca M Guidi, Patrice Hello +2

The first generation of gravitational wave interferometric detectors has taken data at, or close to, their design sensitivity. This data has been searched for a broad range of grav…

gr-qc2009★ 151 cited

A stochastic template placement algorithm for gravitational wave data analysis

Ian Harry, Bruce Allen, B. S. Sathyaprakash

This paper presents an algorithm for constructing matched-filter template banks in an arbitrary parameter space. The method places templates at random, then removes those which are…

gr-qc2009★ 139 cited

X-Pipeline: An analysis package for autonomous gravitational-wave burst searches

Patrick J. Sutton, Gareth Jones, Shourov Chatterji +8

Autonomous gravitational-wave searches -- fully automated analyses of data that run without human intervention or assistance -- are desirable for a number of reasons. They are nece…

gr-qc2009★ 184 cited

Triangulation of gravitational wave sources with a network of detectors

Stephen Fairhurst

There is significant benefit to be gained by pursuing multi-messenger astronomy with gravitational wave and electromagnetic observations. In order to undertake electromagnetic foll…

gr-qc2009★ 646 cited

Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors

Alessandra Buonanno, Bala Iyer, Evan Ochsner +2

The two-body dynamics in general relativity has been solved perturbatively using the post-Newtonian (PN) approximation. The evolution of the orbital phase and the emitted gravitati…

gr-qc2009★ 29 cited

Detecting relics of a thermal gravitational wave background in the early Universe

W. Zhao, D. Baskaran, P. Coles

A thermal gravitational wave background can be produced in the early Universe if a radiation dominated epoch precedes the usual inflationary stage. This background provides a uniqu…

gr-qc2009★ 17 cited

Stable indications of relic gravitational waves in Wilkinson Microwave Anisotropy Probe data and forecasts for the Planck mission

W. Zhao, D. Baskaran, L. P. Grishchuk

The relic gravitational waves (gw) are the cleanest probe of the violent times in the very early history of the Universe. They are expected to leave signatures in the observed cosm…

gr-qc2009★ 55 cited

Status of NINJA: the Numerical INJection Analysis project

Benjamin Aylott, John G. Baker, William D. Boggs +74

The 2008 NRDA conference introduced the Numerical INJection Analysis project (NINJA), a new collaborative effort between the numerical relativity community and the data analysis co…

gr-qc2009★ 100 cited

Einstein@Home search for periodic gravitational waves in early S5 LIGO data

LIGO Scientific Collaboration

This paper reports on an all-sky search for periodic gravitational waves from sources such as deformed isolated rapidly-spinning neutron stars. The analysis uses 840 hours of data…

gr-qc2009★ 122 cited

Search for Gravitational Waves from Low Mass Compact Binary Coalescence in 186 Days of LIGO's fifth Science Run

The LIGO Scientific Collaboration

We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35 Msun, using LIGO observations between November 14, 2006 and May 18, 2…

gr-qc2009★ 48 cited

Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

The LIGO Scientific Collaboration, B. Abbott

According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for exa…

gr-qc2009

Search for gravitational-wave bursts in the first year of the fifth LIGO science run

LIGO Scientific Collaboration, B. P. Abbott

We present the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64-2000 Hz frequency range in data collected by the LIGO detectors during the first…

gr-qc2009★ 12 cited

Response of a spaceborne gravitational wave antenna to solar oscillations

A. G. Polnarev, I. W. Roxburgh, D. Baskaran

We investigate the possibility of observing very small amplitude low frequency solar oscillations with the proposed laser interferometer space antenna (LISA). For frequencies b…

gr-qc2009★ 9 cited

Some Uncomfortable Thoughts on the Nature of Gravity, Cosmology, and the Early Universe

L P Grishchuk

A specific theoretical framework is important for designing and conducting an experiment, and for interpretation of its results. The field of gravitational physics is expanding, an…

gr-qc2009★ 46 cited

Template banks to search for compact binaries with spinning components in gravitational wave data

Chris Van Den Broeck, Duncan A. Brown, Thomas Cokelaer +5

Gravitational waves from coalescing compact binaries are one of the most promising sources for detectors such as LIGO, Virgo and GEO600. If the components of the binary posess sign…

gr-qc2009★ 42 cited

Search for High Frequency Gravitational Wave Bursts in the First Calendar Year of LIGO's Fifth Science Run

LIGO Scientific Collaboration, B. Abbott

We present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIG…

gr-qc2009★ 21 cited

Searching for gravitational-wave signals emitted by eccentric compact binaries using a non-eccentric template bank: implications for ground-based detectors

T Cokelaer, D Pathak

Most of the inspiralling compact binaries are expected to be circularized by the time their gravitational-wave signals enter the frequency band of ground-based detectors such as LI…

gr-qc2009★ 876 cited

Physics, Astrophysics and Cosmology with Gravitational Waves

B. S. Sathyaprakash, B. F. Schutz

Gravitational wave detectors are already operating at interesting sensitivity levels, and they have an upgrade path that should result in secure detections by 2014. We review the p…

gr-qc2009★ 26 cited

Limits on high-frequency gravitational wave background from its interplay with large scale magnetic fields

M. S. Pshirkov, D. Baskaran

In this work, we analyze the implications of graviton to photon conversion in the presence of large scale magnetic fields. We consider the magnetic fields associated with galaxy cl…

gr-qc2009★ 11 cited

Searching for binary coalescences with inspiral templates: Detection and parameter estimation

Benjamin Farr, Stephen Fairhurst, B. S. Sathyaprakash

There has been remarkable progress in numerical relativity recently. This has led to the generation of gravitational waveform signals covering what has been traditionally termed th…

gr-qc2009★ 140 cited

Testing gravitational-wave searches with numerical relativity waveforms: Results from the first Numerical INJection Analysis (NINJA) project

Benjamin Aylott, John G. Baker, William D. Boggs +74

The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave data analysis communities. The purpose…

gr-qc2009★ 146 cited

Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data

LIGO Scientific Collaboration, B. Abbott

We have searched for gravitational waves from coalescing low mass compact binary systems with a total mass between 2 and 35 Msun and a minimum component mass of 1 Msun using data f…