Effects of dark matter in star formation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6699

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DC Field	Value	Language
dc.contributor.author	Arun, K	-
dc.contributor.author	Gudennavar, S	-
dc.contributor.author	Prasad, A	-
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2020-11-10T01:53:28Z	-
dc.date.available	2020-11-10T01:53:28Z	-
dc.date.issued	2019-02	-
dc.identifier.citation	Astrophysics and Space Science, Vol. 364, No. 2, 24	en_US
dc.identifier.issn	1572-946X	-
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/6699	-
dc.description	Restricted Access	en_US
dc.description	The original publication is available at springerlink.com	-
dc.description.abstract	The standard model for the formation of structure assumes that there existed small fluctuations in the early universe that grew due to gravitational instability. The origins of these fluctuations are as yet unclear. In this work we propose the role of dark matter in providing the seed for star formation in the early universe. Very recent observations also support the role of dark matter in the formation of these first stars. With this we set observable constraints on luminosities, temperatures, and lifetimes of these early stars with an admixture of dark matter.	en_US
dc.language.iso	en	en_US
dc.publisher	Springer	en_US
dc.relation.uri	https://doi.org/10.1007/s10509-019-3511-6	-
dc.rights	© Springer	-
dc.subject	Dark matter	en_US
dc.subject	Structure formation	en_US
dc.subject	Early universe	en_US
dc.subject	Maximal luminosity	en_US
dc.title	Effects of dark matter in star formation	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

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