0000000000761976

AUTHOR

J.-y. Vinet

showing 5 related works from this author

GW190521: A Binary Black Hole Merger with a Total Mass of 150  M⊙

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

AstronomyGeneral Physics and Astronomydetector: networkAstrophysicsGravitational waves; Binary black holes Intermediate mass black holes01 natural sciencesGeneral Relativity and Quantum Cosmologygravitational waves; black holesGW190521 BBHIntermediate mass black holesLIGO10. No inequalityQCQBSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPAIR-INSTABILITYSettore FIS/05Physicsstatistical analysis: BayesianSupernovaPhysical SciencesPhysique des particules élémentaires[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodBinary black holes Intermediate mass black holesgr-qcPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Physics and Astronomy(all)Gravitation and AstrophysicsGravitational wavespair-instabilitySettore FIS/05 - Astronomia e AstrofisicaBinary black holeBinary black holesNeutron starsgravitational wavessupernova0103 physical sciences010306 general physicsLuminosity distanceSTFCGW190521Science & Technology9. Industry and infrastructureGravitational wavegravitational radiationRCUKblack hole: massgravitational waves black holegravitational radiation detectorLIGORedshiftBlack holewave: modelVIRGOblack hole: binaryIntermediate-mass black holegravitational radiation: emissionBBH[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Constraining the p -Mode– g -Mode Tidal Instability with GW170817

2019

We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the binary to internal modes of the stars, accelerating the gravitational-wave driven inspiral. We model the impact of this instability on the phasing of the gravitational wave signal using three parameters per star: An overall amplitude, a saturation frequency, and a spectral index. Incorporating these additional parameters, we compute the Bayes factor (lnB!pgpg) comparing our p-g model to a standard one. We find that the observed signal is consistent with waveform models that neglect p-g effects, with lnB!pgpg=…

Physics010308 nuclear & particles physicsGravitational waveGeneral Physics and AstronomyBreaking wave7. Clean energy01 natural sciencesInstabilityComputational physicsNeutron starStarsAmplitude13. Climate action0103 physical sciencesWaveformExtreme value theory010303 astronomy & astrophysicsPhysical Review Letters
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The advanced Virgo longitudinal control system for the O2 observing run

2020

Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During …

neutron star: binaryPhysics::Instrumentation and DetectorsAstronomycavity: opticalSuspended optical cavities01 natural sciencesGravitational wave detectorsoff-lineGravitational wave detectors; Interferometer; Suspended optical cavities; Control loopsControl loopSuspended optical cavitieLIGOInterferometer010303 astronomy & astrophysicsdetectorsSettore FIS/01Physics[PHYS]Physics [physics]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsGravitational wave detectors Interferometer Suspended optical cavities Control loopsGravitational wave detectorUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradecontrol systemGravitational wavelongitudinalAstrophysics::High Energy Astrophysical PhenomenainterferometerAstrophysics::Cosmology and Extragalactic Astrophysicscontrol loops; gravitational wave detectors; interferometer; suspended optical cavitiesgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescence0103 physical sciencesControl loops[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and AstrophysicssensitivityLIGOgravitational radiation detectordetector: sensitivityNeutron star* Automatic Keywords *VIRGOblack hole: binaryControl systemgravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

2014

Made available in DSpace on 2022-04-29T07:21:49Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-11-17 We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of …

MECHANISMPhysics and Astronomy (miscellaneous)AstrophysicsFOLLOW-UP OBSERVATIONSASTROPHYSICAL SOURCESIceCubeneutrinoDetection of gravitational waveGravitational waves neutrinoObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCLIGO Scientific CollaborationQBPhysicsGAMMA-RAY BURSTS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYNuclear and High Energy Physics; Physics and Astronomy (miscellaneous)NEUTRINOSNeutrino detectorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoSENSITIVITYGIANT FLARENuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]95.85.RyMUON NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATIONGravitational wavesGeneral Relativity and Quantum CosmologyINSTABILITIESSettore FIS/05 - Astronomia e AstrofisicaCORE-COLLAPSE SUPERNOVAE[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530SDG 7 - Affordable and Clean EnergyCORE-COLLAPSEDETECTOR/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyGravitational wave95.85.SzMAGNETIZED NEUTRON-STARS[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyTRANSIENTS95.85.Sz; 95.85.RyRELATIVISTIC STARSLIGOPhysics and Astronomy[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma-ray burstEMISSIONEnergy (signal processing)
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Search for GW signals associated with GRBs

2021

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38x10^-6^ (modeled) and 3.1x10^-4^ (unmodeled). We do not find any significant evidence for gravitational-wave signals assoc…

Astrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyGamma ray burstsGravitational wavesCosmologyobservational astronomyGamma ray astronomyGamma-ray burstsAstrophysical ProcessesNatural Sciences
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