Can primordial black holes as all dark matter explain fast radio bursts?
| dc.contributor.author | Kainulainen, Kimmo | |
| dc.contributor.author | Nurmi, Sami | |
| dc.contributor.author | Schiappacasse, Enrico D. | |
| dc.contributor.author | Yanagida, Tsutomu T. | |
| dc.date.accessioned | 2022-01-10T07:24:41Z | |
| dc.date.available | 2022-01-10T07:24:41Z | |
| dc.date.issued | 2021 | |
| dc.identifier.citation | Kainulainen, 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.other | CONVID_103768061 | |
| dc.identifier.uri | https://jyx.jyu.fi/handle/123456789/79253 | |
| dc.description.abstract | Primordial 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.mimetype | application/pdf | |
| dc.language.iso | eng | |
| dc.publisher | American Physical Society (APS) | |
| dc.relation.ispartofseries | Physical Review D | |
| dc.rights | In Copyright | |
| dc.title | Can primordial black holes as all dark matter explain fast radio bursts? | |
| dc.type | research article | |
| dc.identifier.urn | URN:NBN:fi:jyu-202201101032 | |
| dc.contributor.laitos | Fysiikan laitos | fi |
| dc.contributor.laitos | Department of Physics | en |
| dc.type.uri | http://purl.org/eprint/type/JournalArticle | |
| dc.type.coar | http://purl.org/coar/resource_type/c_2df8fbb1 | |
| dc.description.reviewstatus | peerReviewed | |
| dc.relation.issn | 2470-0010 | |
| dc.relation.numberinseries | 12 | |
| dc.relation.volume | 104 | |
| dc.type.version | publishedVersion | |
| dc.rights.copyright | © 2021 American Physical Society | |
| dc.rights.accesslevel | openAccess | fi |
| dc.type.publication | article | |
| dc.relation.grantnumber | 318319 | |
| dc.subject.yso | kosmologia | |
| dc.subject.yso | pimeä aine | |
| dc.subject.yso | mustat aukot | |
| dc.format.content | fulltext | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p7160 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p14101 | |
| jyx.subject.uri | http://www.yso.fi/onto/yso/p18360 | |
| dc.rights.url | http://rightsstatements.org/page/InC/1.0/?language=en | |
| dc.relation.doi | 10.1103/PhysRevD.104.123033 | |
| dc.relation.funder | Research Council of Finland | en |
| dc.relation.funder | Suomen Akatemia | fi |
| jyx.fundingprogram | Academy Project, AoF | en |
| jyx.fundingprogram | Akatemiahanke, SA | fi |
| jyx.fundinginformation | This 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. | |
| dc.type.okm | A1 |
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