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Implications of primordial black holes on the first stars and the origin of the super-massive black holes

dc.contributor.authorBambi, Cosimoen_US
dc.contributor.authorSpolyar, Douglasen_US
dc.contributor.authorDolgov, Alexander D.en_US
dc.contributor.authorFreese, Katherineen_US
dc.contributor.authorVolonteri, Martaen_US
dc.date.accessioned2010-06-01T20:38:18Z
dc.date.available2010-06-01T20:38:18Z
dc.date.issued2009-11-01en_US
dc.identifier.citationBambi, Cosimo; Spolyar, Douglas; Dolgov, Alexander D.; Freese, Katherine; Volonteri, Marta (2009). "Implications of primordial black holes on the first stars and the origin of the super-massive black holes." Monthly Notices of the Royal Astronomical Society 399(3): 1347-1356. <http://hdl.handle.net/2027.42/73744>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/73744
dc.description.abstractIf the cosmological dark matter has a component made of small primordial black holes (BHs), they may have a significant impact on the physics of the first stars and on the subsequent formation of massive BHs. Primordial BHs would be adiabatically contracted into these stars and then would sink to the stellar centre by dynamical friction, creating a larger BH which may quickly swallow the whole star. If these primordial BHs are heavier than ∼10 22  g , the first stars would likely live only for a very short time and would not contribute much to the reionization of the Universe. They would instead become 10–10 3  M ⊙ BHs which (depending on subsequent accretion) could serve as seeds for the super-massive BHs seen at high redshifts as well as those inside galaxies today.en_US
dc.format.extent639465 bytes
dc.format.extent3109 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.publisherBlackwell Publishing Ltden_US
dc.rightsJournal compilation © 2009 RASen_US
dc.subject.otherBlack Hole Physicsen_US
dc.subject.otherDark Matteren_US
dc.subject.otherEarly Universeen_US
dc.titleImplications of primordial black holes on the first stars and the origin of the super-massive black holesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumMCTP, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherIPMU, The University of Tokyo, Kashiwa, Chiba 277-8568, Japanen_US
dc.contributor.affiliationotherDepartment of Physics, University of California, Santa Cruz, CA 95060, USAen_US
dc.contributor.affiliationotherIstituto Nazionale di Fisica Nucleare, Sezione di Ferrara, I-44100 Ferrara, Italyen_US
dc.contributor.affiliationotherDipartimento di Fisica, UniversitÀ degli Studi di Ferrara, I-44100 Ferrara, Italyen_US
dc.contributor.affiliationotherInstitute of Theoretical and Experimental Physics, 113259 Moscow, Russiaen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/73744/1/j.1365-2966.2009.15367.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2009.15367.xen_US
dc.identifier.sourceMonthly Notices of the Royal Astronomical Societyen_US
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dc.owningcollnameInterdisciplinary and Peer-Reviewed


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