Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors

Research output: Contribution to journalArticleResearchpeer review

Authors

  • The LIGO Scientific Collaboration

Research Organisations

External Research Organisations

  • LIGO Laboratory
  • Louisiana State University
  • Laboratoire d'Annecy-le-Vieux de Physique des Particules LAPP
  • Istituto Nazionale di Fisica Nucleare (INFN)
  • Cardiff University
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • National Institute for Subatomic Physics (Nikhef)
  • Washington State University Spokane
  • Carson College of Business
  • Syracuse University
  • University of Birmingham
  • Caltech CaRT
  • University of Western Australia
  • Crawley Hospital
  • University of Mississippi
  • Hanyang University
  • Seoul National University
  • Massachusetts Institute of Technology
  • California State University Fullerton
  • Tsinghua University
  • Embry Riddle Aeronautical University
  • Australian National University
  • Canberra Hospital
  • University of Michigan
  • Universite de Nice-Sophia Antipolis
  • University of Wisconsin Milwaukee
View graph of relations

Details

Original languageEnglish
Article number131101
JournalPhysical review letters
Volume112
Issue number13
Publication statusPublished - 4 Apr 2014

Abstract

Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.

Cite this

Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors. / The LIGO Scientific Collaboration.
In: Physical review letters, Vol. 112, No. 13, 131101, 04.04.2014.

Research output: Contribution to journalArticleResearchpeer review

The LIGO Scientific Collaboration. Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors. Physical review letters. 2014 Apr 4;112(13):131101. doi: 10.1103/PhysRevLett.112.131101
The LIGO Scientific Collaboration. / Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors. In: Physical review letters. 2014 ; Vol. 112, No. 13.
Download
@article{4411c862923a4d8688a6c975bd410312,
title = "Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors",
abstract = "Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.",
author = "{The LIGO Scientific Collaboration} and J Aasi and J Abadie and Abbott, {B P} and R Abbott and T Abbott and Abernathy, {M R} and T Accadia and F Acernese and C Adams and T Adams and Adhikari, {R X} and C Affeldt and M Agathos and N Aggarwal and B Allen and S Ast and S Bose and Brown, {D D} and Brown, {D D} and F Br{\"u}ckner and Y Chen and Danilishin, {S L} and K Danzmann and A Dietz and Fricke, {T T} and M Hanke and M Heurs and F Kawazoe and Lee, {H K} and Lee, {H K} and J Lee and J Lee and H Liu and Y Liu and K Loew and H L{\"u}ck and T Nguyen and J Poeld and J Sanders and M Shaltev and H Vahlbruch and M Wang and X Wang and A Wanner and L-W Wei and B Willke and H Wittel and H Yang and L Zhang and Zhu, {X J}",
year = "2014",
month = apr,
day = "4",
doi = "10.1103/PhysRevLett.112.131101",
language = "English",
volume = "112",
journal = "Physical review letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "13",

}

Download

TY - JOUR

T1 - Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors

AU - The LIGO Scientific Collaboration

AU - Aasi, J

AU - Abadie, J

AU - Abbott, B P

AU - Abbott, R

AU - Abbott, T

AU - Abernathy, M R

AU - Accadia, T

AU - Acernese, F

AU - Adams, C

AU - Adams, T

AU - Adhikari, R X

AU - Affeldt, C

AU - Agathos, M

AU - Aggarwal, N

AU - Allen, B

AU - Ast, S

AU - Bose, S

AU - Brown, D D

AU - Brown, D D

AU - Brückner, F

AU - Chen, Y

AU - Danilishin, S L

AU - Danzmann, K

AU - Dietz, A

AU - Fricke, T T

AU - Hanke, M

AU - Heurs, M

AU - Kawazoe, F

AU - Lee, H K

AU - Lee, H K

AU - Lee, J

AU - Lee, J

AU - Liu, H

AU - Liu, Y

AU - Loew, K

AU - Lück, H

AU - Nguyen, T

AU - Poeld, J

AU - Sanders, J

AU - Shaltev, M

AU - Vahlbruch, H

AU - Wang, M

AU - Wang, X

AU - Wanner, A

AU - Wei, L-W

AU - Willke, B

AU - Wittel, H

AU - Yang, H

AU - Zhang, L

AU - Zhu, X J

PY - 2014/4/4

Y1 - 2014/4/4

N2 - Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.

AB - Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising observational signature. In this Letter we present a search for GWs from cosmic string cusps in data collected by the LIGO and Virgo gravitational wave detectors between 2005 and 2010, with over 625 days of live time. We find no evidence of GW signals from cosmic strings. From this result, we derive new constraints on cosmic string parameters, which complement and improve existing limits from previous searches for a stochastic background of GWs from cosmic microwave background measurements and pulsar timing data. In particular, if the size of loops is given by the gravitational backreaction scale, we place upper limits on the string tension Gμ below 10(-8) in some regions of the cosmic string parameter space.

U2 - 10.1103/PhysRevLett.112.131101

DO - 10.1103/PhysRevLett.112.131101

M3 - Article

C2 - 24745400

VL - 112

JO - Physical review letters

JF - Physical review letters

SN - 0031-9007

IS - 13

M1 - 131101

ER -

By the same author(s)