Published August 5, 2022 | Version Published + Supplemental Material + Submitted
Journal Article Open

Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO's and Advanced Virgo's Third Observing Run

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Abstract

We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M_⊙ and 1.0 M_⊙ in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend our previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio q ≥ 0.1. We do not report any gravitational-wave candidates. The most significant trigger has a false alarm rate of 0.14 yr⁻¹. This implies an upper limit on the merger rate of subsolar binaries in the range [220 − 24200] Gpc⁻³ yr⁻¹, depending on the chirp mass of the binary. We use this upper limit to derive astrophysical constraints on two phenomenological models that could produce subsolar-mass compact objects. One is an isotropic distribution of equal-mass primordial black holes. Using this model, we find that the fraction of dark matter in primordial black holes in the mass range 0.2 M_⊙ < m_(PBH) < 1.0 M_⊙ is f_(PBH) ≡ Ω_(PBH)/Ω_(DM) ≲ 6%. This improves existing constraints on primordial black hole abundance by a factor of ∼3. The other is a dissipative dark matter model, in which fermionic dark matter can collapse and form black holes. The upper limit on the fraction of dark matter black holes depends on the minimum mass of the black holes that can be formed: the most constraining result is obtained at M_(min) = 1 M_⊙, where f_(DBH) ≡ Ω_(DBH)/Ω_(DM) ≲ 0.003%. These are the first constraints placed on dissipative dark models by subsolar-mass analyses.

Additional Information

© 2022 American Physical Society. (Received 1 October 2021; revised 18 March 2022; accepted 7 June 2022; published 5 August 2022) This material is based upon work supported by NSF's LIGO Laboratory which is a major facility fully funded by the National Science Foundation. The authors also gratefully acknowledge the support of the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Netherlands Organization for Scientific Research (NWO), for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigación, the Vicepresidència i Conselleria d'Innovació, Recerca i Turisme and the Conselleria d'Educació i Universitat del Govern de les Illes Balears, the Conselleria d'Innovació, Universitats, Ciència i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the European Union—European Regional Development Fund; Foundation for Polish Science (FNP), the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concertées (ARC) and Fonds Wetenschappelijk Onderzoek—Vlaanderen (FWO), Belgium, the Paris Íle-de-France Region, the National Research, Development and Innovation Office Hungary (NKFIH), the National Research Foundation of Korea, the Natural Science and Engineering Research Council Canada, Canadian Foundation for Innovation (CFI), the Brazilian Ministry of Science, Technology, and Innovations, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan, the United States Department of Energy, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, INFN, and CNRS for provision of computational resources. Funding for this project was provided by the Charles E. Kaufman Foundation of The Pittsburgh Foundation and the Institute for Computational and Data Sciences at Penn State. This article has been assigned the document number LIGO-P2100163-v8.

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Submitted - 2109.12197.pdf

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Additional details

Identifiers

Eprint ID
116166
DOI
10.1103/physrevlett.129.061104
Resolver ID
CaltechAUTHORS:20220808-223925000

Funding

Science and Technology Facilities Council (STFC)
Australian Research Council
Istituto Nazionale di Fisica Nucleare (INFN)
Centre National de la Recherche Scientifique (CNRS)
Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)
Council of Scientific and Industrial Research (India)
Department of Science and Technology (India)
Science and Engineering Research Board (SERB)
Ministry of Education (India)
Agencia Estatal de Investigación
Ministerio de Ciencia e Innovación (MICINN)
Conselleria d'Educació i Universitat del Govern de les Illes Balears
Generalitat Valenciana Conselleria de Innovación, Universidades, Ciencia y Sociedad Digital
Generalitat de Catalunya
National Science Centre (Poland)
European Regional Development Fund
Foundation for Polish Science
Swiss National Science Foundation (SNSF)
Russian Foundation for Basic Research
Russian Science Foundation
European Commission
Royal Society
Scottish Funding Council
Scottish Universities Physics Alliance
Hungarian Scientific Research Fund (OTKA)
Institut des Origines de Lyon
Fonds de la Recherche Scientifique (FNRS)
Fonds Wetenschappelijk Onderzoek (FWO)
Conseil Régional, Île-de-France
National Research, Development and Innovation Office (Hungary)
National Research Foundation of Korea
Natural Sciences and Engineering Research Council of Canada (NSERC)
Canada Foundation for Innovation
International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)
Research Grants Council of Hong Kong
National Natural Science Foundation of China
Leverhulme Trust
Ministry of Science and Technology (Taipei)
Department of Energy (DOE)
Kavli Foundation
Charles E. Kaufman Foundation
Pittsburgh Foundation
Pennsylvania State University
Max Planck Society
Conselleria de Fons Europeus
Research Corporation
Vicepresidència i Conselleria d'Innovació, Recerca i Turisme
State of Niedersachsen/Germany
Ministry of Human Resource Development (India)

Dates

Created
2022-08-11
Created from EPrint's datestamp field
Updated
2023-03-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
LIGO , Astronomy Department , TAPIR , Physics Department , Physics Department
Other Numbering System Name
LIGO Document
Other Numbering System Identifier
P2100163-v8