 |
Journal articles
Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run
B.P. Abbott
T. Adams
1
R. Bonnand
1
D. Buskulic
1
M. Ducrot
1
V. Germain
1
R. Gouaty
1
N. Letendre
1
F. Marion
1
A. Masserot
1
B. Mours
1
L. Rolland
1
D. Verkindt
1
M. Was
1
M. Yvert
1
François Bondu
2
M. Boër
3
G. Bogaert
3
A. Brillet
3
F. Cleva
3
J.-P. Coulon
3
J.-D. Fournier
3
H. Heitmann
3
F. Kéfélian
3
N. Man
3
L. Martinelli
3
D. Meacher
3
M. Merzougui
3
M. Pichot
3
T. Regimbau
3
M. Turconi
3
J.-Y. Vinet
3
L.-W. Wei
3
F. Marion 1
Author
A. Masserot 1
Author
B. Mours 1
Author
L. Rolland 1
Author IdHAL : loic-rolland arXiv : https://arxiv.org/a/Loic Rolland ORCID : https://orcid.org/0000-0003-0589-9687
D. Verkindt 1
Author IdHAL : didier-verkindt VIAF : https://viaf.org/viaf/450144782737535668452 arXiv : http://arxiv.org/a/verkindt_d_1 IdRef : https://www.idref.fr/188902783 ORCID : https://orcid.org/0000-0003-4344-7227
M. Was 1
Author IdHAL : michalwas ORCID : https://orcid.org/0000-0002-1890-1128
M. Yvert 1
Author
François Bondu 2
Author IdHAL : francois-bondu ResearcherId : http://www.researcherid.com/rid/A-2071-2012 ORCID : https://orcid.org/0000-0001-6487-5197
M. Boër 3
Author
G. Bogaert 3
Author IdHAL : gilles-bogaert ORCID : https://orcid.org/0000-0003-2507-3866
A. Brillet 3
Author
F. Cleva 3
Author
J.-P. Coulon 3
Author
J.-D. Fournier 3
Author
H. Heitmann 3
Author
F. Kéfélian 3
Author IdHAL : fabien-kefelian ORCID : https://orcid.org/0000-0001-9870-6850
L.-W. Wei 3
Author
1
LAPP - Laboratoire d'Annecy de Physique des Particules (9 Chemin de Bellevue - BP 110 - 74941 Annecy-le-Vieux CEDEX - France - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- USMB [Université de Savoie] [Université de Chambéry] - Université Savoie Mont Blanc (27, rue Marcoz - 73000 Chambéry - France)
- CNRS - Centre National de la Recherche Scientifique : UMR5814 (France)
2
IPR - Institut de Physique de Rennes (Bâtiment 11A , B, C, E – 10B
263 av. Général Leclerc
35042 Rennes cedex FRANCE - France)
- UR1 - Université de Rennes 1 (2 rue du Thabor - CS 46510 - 35065 Rennes cedex - France)
- UNIV-RENNES - Université de Rennes (France)
- CNRS - Centre National de la Recherche Scientifique : UMR6251 (France)
3
ARTEMIS - Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (Bd de l'Observatoire BP 4229 06304 NICE CEDEX 4 - France)
- UNS - Université Nice Sophia Antipolis (... - 2019) (Parc Valrose - BP 2135 - 06103 Nice cedex 2 - France)
- COMUE UCA - COMUE Université Côte d'Azur (2015 - 2019) (Parc Valrose, 28 avenue Valrose 06108 Nice Cedex 2 - France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- Observatoire de la Côte d'Azur (France)
- UCA - Université Côte d'Azur (Parc Valrose, 28 avenue Valrose 06108 Nice Cedex 2 - France)
- COMUE UCA - COMUE Université Côte d'Azur (2015 - 2019) (Parc Valrose, 28 avenue Valrose 06108 Nice Cedex 2 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7250 (France)
- UCA - Université Côte d'Azur (Parc Valrose, 28 avenue Valrose 06108 Nice Cedex 2 - France)
Abstract : A wide variety of astrophysical and cosmological sources are expected to contribute to a stochastic gravitational-wave background. Following the observations of GW150914 and GW151226, the rate and mass of coalescing binary black holes appear to be greater than many previous expectations. As a result, the stochastic background from unresolved compact binary coalescences is expected to be particularly loud. We perform a search for the isotropic stochastic gravitational-wave background using data from Advanced LIGO's first observing run. The data display no evidence of a stochastic gravitational-wave signal. We constrain the dimensionless energy density of gravitational waves to be $\Omega_0<1.7\times 10^{-7}$ with 95% confidence, assuming a flat energy density spectrum in the most sensitive part of the LIGO band (20-86 Hz). This is a factor of ~33 times more sensitive than previous measurements. We also constrain arbitrary power-law spectra. Finally, we investigate the implications of this search for the background of binary black holes using an astrophysical model for the background.
Document type :
Journal articles
Complete list of metadata
http://hal.in2p3.fr/in2p3-01412187
Contributor : Claudine Bombar <>
Submitted on : Thursday, December 8, 2016 - 10:12:31 AM
Last modification on : Wednesday, March 31, 2021 - 1:59:47 PM
Contributor : Claudine Bombar <>
Submitted on : Thursday, December 8, 2016 - 10:12:31 AM
Last modification on : Wednesday, March 31, 2021 - 1:59:47 PM
Links full text
Identifiers
- HAL Id : in2p3-01412187, version 1
- ARXIV : 1612.02029
- DOI : 10.1103/PhysRevLett.118.121101
- PUBMED : 28388180
Collections
IN2P3 | CNRS | LAPP | UNIV-SAVOIE | UNICE | ARTEMIS | OCA | IPR | UNIV-RENNES1 | UR1-UFR-SPM | IPR-OP | OSUR | INSU | UNIV-COTEDAZUR | UNIV-RENNES | UGA
Citation
B.P. Abbott, T. Adams, R. Bonnand, D. Buskulic, M. Ducrot, et al.. Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run. Physical Review Letters, American Physical Society, 2017, 118 (12), pp.121101. ⟨10.1103/PhysRevLett.118.121101⟩. ⟨in2p3-01412187⟩
Metrics
Record views