Searches for gravitational waves associated with pulsar glitches using a coherent network algorithm

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dc.creatorHayama, Kazuhiro
dc.creatorDesai, Shantanu
dc.creatorMohanty, Soumya D.
dc.creatorRakhmanov, Malik
dc.creatorSummerscales, Tiffany
dc.creatorYoshida, Sanichiro
dc.date2008-07-25
dc.date.accessioned2026-07-07T11:45:04Z
dc.date.available2026-07-07T11:45:04Z
dc.descriptionPulsar glitches are a potential source of gravitational waves for current and future interferometric gravitational wave detectors. Some pulsar glitch events were observed by radio and X-ray telescopes during the fifth LIGO science run. It is expected that glitches from these same pulsars should also be seen in the future. We carried out Monte Carlo simulations to estimate the sensitivity of possible gravitational wave signals associated with a pulsar glitch using a coherent network analysis method. We show the detection efficiency and evaluate the reconstruction accuracy of gravitational waveforms using a matched filter analysis on the estimated gravitational waveforms from the coherent analysis algorithm.
dc.descriptionsubmitted to CQG
dc.identifierhttps://arxiv.org/abs/0807.3983
dc.identifierhttp://arxiv.org/abs/0807.3983
dc.identifierClass.Quant.Grav.25:184016,2008
dc.identifierdoi:10.1088/0264-9381/25/18/184016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201767
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSearches for gravitational waves associated with pulsar glitches using a coherent network algorithm
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