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The Transient Gravitational-Wave Sky

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arxiv 1305.0816 v1 pith:463YJN4M submitted 2013-05-03 gr-qc astro-ph.COastro-ph.HE

Nils Andersson , John Baker , Kris Belczynski , Sebastiano Bernuzzi , Emanuele Berti , Laura Cadonati , Pablo Cerda-Duran , James Clark
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Marc Favata Lee Samuel Finn Chris Fryer Bruno Giacomazzo Jose Antonio Gonzalez Martin Hendry Ik Siong Heng Stefan Hild Nathan Johnson-McDaniel Peter Kalmus Sergei Klimenko Shiho Kobayashi Kostas Kokkotas Pablo Laguna Luis Lehner Janna Levin Steve Liebling Andrew MacFadyen Ilya Mandel Szabolcs Marka Zsuzsa Marka David Neilsen Paul O'Brien Rosalba Perna Harald Pfeiffer Jocelyn Read Christian Reisswig Carl Rodriguez Max Ruffert Erik Schnetter Antony Searle Peter Shawhan Deirdre Shoemaker Alicia Soderberg Ulrich Sperhake Patrick Sutton Nial Tanvir Michal Was Stan Whitcomb
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classification gr-qcastro-ph.COastro-ph.HE
keywords gravitational-wavetransientunderstandingwillanalysisastrophysicscataclysmicchallenge
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Interferometric detectors will very soon give us an unprecedented view of the gravitational-wave sky, and in particular of the explosive and transient Universe. Now is the time to challenge our theoretical understanding of short-duration gravitational-wave signatures from cataclysmic events, their connection to more traditional electromagnetic and particle astrophysics, and the data analysis techniques that will make the observations a reality. This paper summarizes the state of the art, future science opportunities, and current challenges in understanding gravitational-wave transients.

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Cited by 1 Pith paper

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  1. kiloHertz gravitational waves from binary neutron star remnants: time-domain model and constraints on extreme matter

    gr-qc 2019-08 conditional novelty 7.0 of 10

    A phase-coherent time-domain model for kilohertz postmerger gravitational waves from neutron star remnants is introduced, with injection studies indicating postmerger detection at SNR around 8.5 and radius constraints...

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