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dc.contributor.authorKainulainen, Kimmo
dc.contributor.authorNurmi, Sami
dc.contributor.authorSchiappacasse, Enrico D.
dc.contributor.authorYanagida, Tsutomu T.
dc.date.accessioned2022-01-10T07:24:41Z
dc.date.available2022-01-10T07:24:41Z
dc.date.issued2021
dc.identifier.citationKainulainen, K., Nurmi, S., Schiappacasse, E. D., & Yanagida, T. T. (2021). Can primordial black holes as all dark matter explain fast radio bursts?. <i>Physical Review D</i>, <i>104</i>(12), Article 123033. <a href="https://doi.org/10.1103/PhysRevD.104.123033" target="_blank">https://doi.org/10.1103/PhysRevD.104.123033</a>
dc.identifier.otherCONVID_103768061
dc.identifier.urihttps://jyx.jyu.fi/handle/123456789/79253
dc.description.abstractPrimordial black holes (PBHs) are one of the most interesting nonparticle dark matter (DM) candidates. They may explain all the DM content in the Universe in the mass regime from about 10−14 M⊙ to 10−11 M⊙. We study PBHs as the source of fast radio bursts (FRBs) via magnetic reconnection in the event of collisions between them and neutron stars (NSs) in galaxies. We investigate the energy loss of PBHs during PBH-NS encounters to model their capture by NSs. To an order-of-magnitude estimation, we conclude that the parameter space of PBHs being all DM is accidentally consistent with that to produce FRBs with a rate which is the order of the observed FRB rate.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherAmerican Physical Society (APS)
dc.relation.ispartofseriesPhysical Review D
dc.rightsIn Copyright
dc.titleCan primordial black holes as all dark matter explain fast radio bursts?
dc.typearticle
dc.identifier.urnURN:NBN:fi:jyu-202201101032
dc.contributor.laitosFysiikan laitosfi
dc.contributor.laitosDepartment of Physicsen
dc.type.urihttp://purl.org/eprint/type/JournalArticle
dc.description.reviewstatuspeerReviewed
dc.relation.issn2470-0010
dc.relation.numberinseries12
dc.relation.volume104
dc.type.versionpublishedVersion
dc.rights.copyright© 2021 American Physical Society
dc.rights.accesslevelopenAccessfi
dc.relation.grantnumber318319
dc.subject.ysokosmologia
dc.subject.ysopimeä aine
dc.subject.ysomustat aukot
dc.format.contentfulltext
jyx.subject.urihttp://www.yso.fi/onto/yso/p7160
jyx.subject.urihttp://www.yso.fi/onto/yso/p14101
jyx.subject.urihttp://www.yso.fi/onto/yso/p18360
dc.rights.urlhttp://rightsstatements.org/page/InC/1.0/?language=en
dc.relation.doi10.1103/PhysRevD.104.123033
dc.relation.funderSuomen Akatemiafi
dc.relation.funderAcademy of Finlanden
jyx.fundingprogramAkatemiahanke, SAfi
jyx.fundingprogramAcademy Project, AoFen
jyx.fundinginformationThis work was supported by the Academy of Finland Grant No. 318319. T. T. Y. is supported in part by the China Grant for Talent Scientific Start-Up Project and the JSPS Grant-in-Aid for Scientific Research Grants No. 16H02176, No. 17H02878, and No. 19H05810 and by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan.


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