Forming supermassive black holes like J1342+0928 (invoking dark matter) in early universe

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6902

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.contributor.author	Arun, K	-
dc.contributor.author	Kiren, O. V	-
dc.date.accessioned	2020-11-11T01:45:16Z	-
dc.date.available	2020-11-11T01:45:16Z	-
dc.date.issued	2018-02	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 363, 40	en_US
dc.identifier.issn	0004-640X	-
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6902	-
dc.description	Restricted Access © Springer The original publication is available at springerlink.com https://doi.org/10.1007/s10509-018-3258-5	en_US
dc.description.abstract	Recent discovery of J1342+0928 using data from the WISE telescope and ground based surveys indicate presence of a supermassive black hole (SMBH) having a mass of 800 million solar mass at a redshift of about 7.6. This imply that the black hole grew to this mass only 690 million years after the universe started expanding. Here we suggest that formation of such SMBH's so early in the universe is consistent with our present understanding of the phenomena involved by invoking dark matter (DM).	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.subject	Supermassive black hole	en_US
dc.subject	Early universe	en_US
dc.subject	Structure formation	en_US
dc.subject	Dark matter theory	en_US
dc.title	Forming supermassive black holes like J1342+0928 (invoking dark matter) in early universe	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

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