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Effects of dark matter in star formation

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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


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