Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run

(LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration)

Research output: Contribution to journalArticlepeer-review

136 Scopus citations

Abstract

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks, and, for the first time, kink-kink collisions. A template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension Gμ as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models. Additionally, we develop and test a third model that interpolates between these two models. Our results improve upon the previous LIGO-Virgo constraints on Gμ by 1 to 2 orders of magnitude depending on the model that is tested. In particular, for the one-loop distribution model, we set the most competitive constraints to date: Gμ≲4×10-15. In the case of cosmic strings formed at the end of inflation in the context of grand unified theories, these results challenge simple inflationary models.

Original languageEnglish
Article number241102
JournalPhysical Review Letters
Volume126
Issue number24
DOIs
StatePublished - 18 Jun 2021
Externally publishedYes

Funding

FundersFunder number
Council of Scientific and Industrial Research, India
Ministry of Human Resource Development
Australian Research Council
ICTP South American Institute for Fundamental Research
National Research Foundation of Korea
Narodowe Centrum Nauki
Scottish Universities Physics Alliance
National Science Foundation
Conselleria d’Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana
Science and Technology Facilities Council
Scottish Funding Council
Actions de Recherche Concertées
Ministry of Science and Technology, Taiwan
French Lyon Institute of Origins
Leverhulme Trust
Science and Engineering Research Board
Generalitat de Catalunya
Instituto Nazionale di Fisica Nucleare
Department of Science and Technology, Ministry of Science and Technology, India
Centre National de la Recherche Scientifique
Max-Planck-Gesellschaft
Canada Foundation for Innovation
Kavli Foundation
Nemzeti Kutatási Fejlesztési és Innovációs Hivatal
KISTI-GSDC
European Commission
Russian Foundation for Basic Research
U.S. Department of Energy
Brazilian Ministry of Science, Technology, and Innovations
Agencia Estatal de Investigación
Natural Sciences and Engineering Research Council of Canada
Research Grants Council, University Grants Committee
Russian Science Foundation
Advanced Technology Center
Fundacja na rzecz Nauki Polskiej
Hungarian Scientific Research Fund
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Fonds De La Recherche Scientifique - FNRS
Royal Society
Universitat de les Illes Balears
European Regional Development Fund
Fonds Wetenschappelijk Onderzoek—Vlaanderen
University of Tokyo
Netherlands Organization for Scientific Research for the construction and operation of the Virgo detector
Istituto Nazionale di Fisica Nucleare
Ministry of Education, Culture, Sports, Science and Technology
National Natural Science Foundation of China
Academia SinicaAS-CDA-105-M06
Japan Society for the Promotion of Science18K03630, 17H06133, JP17H06361, JP17H06364, 18H01224, JP17H06358
Fundação para a Ciência e a TecnologiaIncentivo/SAU/LA0001/2013

    Fingerprint

    Dive into the research topics of 'Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run'. Together they form a unique fingerprint.

    Cite this