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Local temperature distribution in the vicinity of gravitationally bound objects in the expanding universe

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dc.contributor.authorPetriakova, P. M.
dc.contributor.authorRubin, S. G.
dc.contributor.authorРубин, Сергей Георгиевич
dc.date.accessioned2024-11-21T18:32:12Z
dc.date.available2024-11-21T18:32:12Z
dc.date.issued2019
dc.description.abstract© 2019 DMFA zaloznistvo. All rights reserved.We consider a cluster of Primordial Black Holes which is decoupled from the cosmological expansion (Hubble flow) and this region is heated as compared to the surrounding matter. The increased temperature inside the region can be explained by several mechanisms of Primordial Black Holes formation. We study the temperature dynamics of the heated region of Primordial Black Holes cluster.
dc.format.extentС. 237-246
dc.identifier.citationPetriakova, P. M. Local temperature distribution in the vicinity of gravitationally bound objects in the expanding universe / Petriakova, P.M., Rubin, S.G. // Bled Workshops in Physics. - 2019. - 20. - № 2. - P. 237-246
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85084172412&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19525
dc.relation.ispartofBled Workshops in Physics
dc.titleLocal temperature distribution in the vicinity of gravitationally bound objects in the expanding universe
dc.typeConference Paper
dspace.entity.typePublication
oaire.citation.issue2
oaire.citation.volume20
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