Details
Original language | English |
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Article number | 131101 |
Journal | Physical review letters |
Volume | 112 |
Issue number | 13 |
Publication status | Published - 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.
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In: Physical review letters, Vol. 112, No. 13, 131101, 04.04.2014.
Research output: Contribution to journal › Article › Research › peer review
}
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 -