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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/113040
Title: 
Search for Gravitational Waves Associated with gamma-ray Bursts Detected by the Interplanetary Network
Author(s): 
Institution: 
  • CALTECH
  • Louisiana State Univ
  • Univ Salerno
  • Complesso Univ Monte S Angelo
  • Univ Florida
  • LIGO Livingston Observ
  • Cardiff Univ
  • Univ Sannio Benevento
  • INFN
  • Max Planck Inst Gravitat Phys
  • Nikhef
  • MIT
  • Instituto Nacional de Pesquisas Espaciais (INPE)
  • Tata Inst Fundamental Res
  • Syracuse Univ
  • Univ Wisconsin Milwaukee
  • Leibniz Univ Hannover
  • Univ Siena
  • Stanford Univ
  • University of Mississippi
  • Calif State Univ Fullerton
  • Ist Nazl Fis Nucl
  • Univ Birmingham
  • Max Planck Inst Gravitat phys
  • Montana State Univ
  • European Gravitat Observ EGO
  • Hanford Observ
  • Univ Glasgow
  • Univ Paris Diderot
  • Columbia University
  • Univ Pisa
  • CAMK PAN
  • Warsaw Univ
  • Univ Genoa
  • Moscow MV Lomonosov State Univ
  • Univ Paris 11
  • NASA
  • Univ Western Australia
  • Radboud Univ Nijmegen
  • Univ Nice Sophia Antipolis
  • Univ Rennes 1
  • Univ Savoie
  • Washington State Univ
  • Inter Univ Ctr Astron & Astrophys
  • Kyoto Univ
  • Univ Urbino
  • Univ Oregon
  • Univ Paris 06
  • Vrije Univ Amsterdam
  • University of Maryland
  • Univ Massachusetts Amherst
  • Univ Lyon
  • Univ Illes Balears
  • Univ Naples Federico II
  • Univ Toronto
  • Tsinghua Univ
  • University of Michigan
  • Natl Tsing Hua Univ
  • Charles Sturt Univ
  • Caltech CaRT
  • Pusan Natl Univ
  • Australian Natl Univ
  • Carleton Coll
  • Univ Roma Tor Vergata
  • Univ Roma La Sapienza
  • Univ Brussels
  • Sonoma State Univ
  • George Washington Univ
  • Univ Cambridge
  • Univ Minnesota
  • Univ Texas Brownsville
  • Univ Sheffield
  • RMKI
  • Argentinian Gravitat Wave Grp
  • Univ Trent
  • NW Univ
  • Montclair State Univ
  • Penn State Univ
  • Eotvos Lorand Univ
  • Univ Perugia
  • HSIC
  • Embry Riddle Aeronaut Univ
  • Seoul Natl Univ
  • Perimeter Inst Theoret Phys
  • Amer Univ
  • Coll William & Mary
  • Univ Adelaide
  • Raman Res Inst
  • Korea Inst Sci & Technol Informat
  • Bialystok Univ
  • Univ Southampton
  • IISER TVM
  • Inst Phys Appl
  • Hanyang Univ
  • NCBJ
  • IM PAN
  • Inst Plasma Res
  • Univ Melbourne
  • Monash Univ
  • Univ Strathclyde
  • Louisiana Tech University
  • CNRS
  • Univ Camerino
  • S Univ & A& M Coll
  • IISER Kolkata
  • Natl Inst Mat Sci
  • Hobart & William Smith Coll
  • RRCAT
  • Univ W Scotland
  • Inst Astron
  • Indian Inst Technol
  • Universidade Estadual Paulista (UNESP)
  • Andrews Univ
  • Trinity Univ
  • University of Washington
  • Rochester Inst Technol
  • SE Louisiana Univ
  • Abilene Christian Univ
  • AF Ioffe Phys Tech Inst
  • Univ Toulouse
  • Univ Alabama Huntsville
  • Univ Calif Berkeley
  • CRESST
  • Univ Space Res Assoc
  • INAF IASF Bologna
  • St Petersburg State Polytechn Univ
  • Los Alamos Natl Lab
  • Saitama Univ
  • Max Planck Inst f extraterrest Phys
ISSN: 
0031-9007
Sponsorship: 
  • Australian Research Council
  • International Science Linkages program of the Commonwealth of Australia
  • Council of Scientific and Industrial Research of India
  • Istituto Nazionale di Fisica Nucleare of Italy
  • Spanish Ministerio de Economia y Competitividad
  • Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears
  • Netherlands Organisation for Scientific Research
  • Polish Ministry of Science and Higher Education
  • FOCUS Programme of Foundation for Polish Science
  • Royal Society
  • Scottish Funding Council
  • Scottish Universities Physics Alliance
  • National Aeronautics and Space Administration
  • Carnegie Trust
  • Leverhulme Trust
  • David and Lucile Packard Foundation
  • Research Corporation
  • Alfred P. Sloan Foundation
  • NASA
  • Russian Space Agency
  • RFBR
Sponsorship Process Number: 
  • NASANNX06AI36G
  • NASANNX08AB84G
  • NASANNX08AZ85G
  • NASANNX09AV61G
  • NASANNX10AR12G
  • NASANNG06GI89G
  • NASANNX07AJ65G
  • NASANNX08AN23G
  • NASANNX09AO97G
  • NASANNX10AI23G
  • NASANNG06GE69G
  • NASANNX07AQ22G
  • NASANNX08AC90G
  • NASANNX08AX95G
  • NASANNX09AR28G
  • RFBR12-02-00032-a
  • RFBR13-02-12017-ofi_m
Abstract: 
We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M(circle dot)c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
Issue Date: 
30-Jun-2014
Citation: 
Physical Review Letters. College Pk: Amer Physical Soc, v. 113, n. 1, 14 p., 2014.
Time Duration: 
14
Publisher: 
Amer Physical Soc
Source: 
http://dx.doi.org/10.1103/PhysRevLett.113.011102
URI: 
Access Rights: 
Acesso restrito
Type: 
outro
Source:
http://repositorio.unesp.br/handle/11449/113040
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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