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Article: Has LIGO detected primordial black hole dark matter? - tidal disruption in binary black hole formation

TitleHas LIGO detected primordial black hole dark matter? - tidal disruption in binary black hole formation
Authors
Keywordsblack hole physics
dark matter
gravitational waves
quasars
supermassive black holes
Issue Date2020
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/1674-4527/
Citation
Research in Astronomy and Astrophysics, 2020, v. 20 n. 11, p. article no. 185 How to Cite?
AbstractThe frequent detection of binary mergers of ~30 M⊙ black holes (BHs) by the Laser Interferometer Gravitational-Wave Observatory (LIGO) rekindled researchers' interest in primordial BHs (PBHs) being dark matter (DM). In this work, we investigated PBHs distributed as DM with a monochromatic mass of 30 M⊙ and examined the encounter-capture scenario of binary formation, where the densest central region of DM halo dominates. Thus, we paid special attention to the tidal effect by the supermassive black hole (SMBH) present. In doing so, we discovered a necessary tool called loss zone that complements the usage of loss cone. We found that the tidal effect is not prominent in affecting binary formation, which also turned out to be insufficient in explaining the totality of LIGO's event rate estimation, especially due to a microlensing event constraining the DM fraction in PBH at the mass of interest from near unity to an order smaller. Meanwhile, an early-universe binary formation scenario proves so prevailing that the LIGO signal in turn constrains the PBH fraction below one percent. Thus, people should put more faith in alternative PBH windows and other DM candidates.
Persistent Identifierhttp://hdl.handle.net/10722/295262
ISSN
2023 Impact Factor: 1.8
2023 SCImago Journal Rankings: 0.641
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorGAO, Y-
dc.contributor.authorZhang, XJ-
dc.contributor.authorSu, M-
dc.date.accessioned2021-01-11T13:57:37Z-
dc.date.available2021-01-11T13:57:37Z-
dc.date.issued2020-
dc.identifier.citationResearch in Astronomy and Astrophysics, 2020, v. 20 n. 11, p. article no. 185-
dc.identifier.issn1674-4527-
dc.identifier.urihttp://hdl.handle.net/10722/295262-
dc.description.abstractThe frequent detection of binary mergers of ~30 M⊙ black holes (BHs) by the Laser Interferometer Gravitational-Wave Observatory (LIGO) rekindled researchers' interest in primordial BHs (PBHs) being dark matter (DM). In this work, we investigated PBHs distributed as DM with a monochromatic mass of 30 M⊙ and examined the encounter-capture scenario of binary formation, where the densest central region of DM halo dominates. Thus, we paid special attention to the tidal effect by the supermassive black hole (SMBH) present. In doing so, we discovered a necessary tool called loss zone that complements the usage of loss cone. We found that the tidal effect is not prominent in affecting binary formation, which also turned out to be insufficient in explaining the totality of LIGO's event rate estimation, especially due to a microlensing event constraining the DM fraction in PBH at the mass of interest from near unity to an order smaller. Meanwhile, an early-universe binary formation scenario proves so prevailing that the LIGO signal in turn constrains the PBH fraction below one percent. Thus, people should put more faith in alternative PBH windows and other DM candidates.-
dc.languageeng-
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/1674-4527/-
dc.relation.ispartofResearch in Astronomy and Astrophysics-
dc.rightsResearch in Astronomy and Astrophysics. Copyright © Institute of Physics Publishing Ltd.-
dc.rightsThis is an author-created, un-copyedited version of an article published in [insert name of journal]. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at http://dx.doi.org/[insert DOI].-
dc.subjectblack hole physics-
dc.subjectdark matter-
dc.subjectgravitational waves-
dc.subjectquasars-
dc.subjectsupermassive black holes-
dc.titleHas LIGO detected primordial black hole dark matter? - tidal disruption in binary black hole formation-
dc.typeArticle-
dc.identifier.emailSu, M: mengsu84@hku.hk-
dc.identifier.authoritySu, M=rp02150-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1088/1674-4527/20/11/185-
dc.identifier.scopuseid_2-s2.0-85097243399-
dc.identifier.hkuros320825-
dc.identifier.volume20-
dc.identifier.issue11-
dc.identifier.spagearticle no. 185-
dc.identifier.epagearticle no. 185-
dc.identifier.isiWOS:000593527600001-
dc.publisher.placeUnited Kingdom-

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