Reionization effect enhancement due to primordial black holes

dc.contributor.author	Belotsky K.
dc.contributor.author	Kirillov A.
dc.contributor.author	Nazarova N.
dc.contributor.author	Rubin S.
dc.date.accessioned	2018-09-19T20:25:44Z
dc.date.available	2018-09-19T20:25:44Z
dc.date.issued	2017
dc.identifier.issn	0218-2718
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/142899
dc.description.abstract	© 2017 World Scientific Publishing CompanyPrimordial black holes (PBHs) could account for variety of phenomena like dark matter, reionization of the universe, early quasars, coalescence of black holes registered through gravitational waves recently. Each phenomenon relates to PBH of a specific mass range. PBH mass spectra varies in a wide range depending on specific model. Earlier, we have shown that PBH with monochromatic mass distribution around (Formula presented.) g value allow to re-ionize the universe moderately. Here, we show that reionization effect and contribution to dark matter can be simultaneously enhanced with more natural extended mass distribution in the range around the same mass value.
dc.relation.ispartofseries	International Journal of Modern Physics D
dc.subject	dark matter
dc.subject	Primordial black holes
dc.subject	reionization
dc.title	Reionization effect enhancement due to primordial black holes
dc.type	Article in Press
dc.collection	Публикации сотрудников КФУ
dc.source.id	SCOPUS02182718-2017-SID85017112289

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.