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Extremal charged black holes, dark matter and dark energy

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dc.contributor.author Sivaram, C
dc.contributor.author Arun, K
dc.contributor.author Prasad, A
dc.date.accessioned 2020-11-14T07:30:46Z
dc.date.available 2020-11-14T07:30:46Z
dc.date.issued 2018-10
dc.identifier.citation Astrophysics and Space Science, Vol. 363, 202 en_US
dc.identifier.issn 1572-946X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7017
dc.description Restricted Access © Springer The original publication is available at springerlink.com https://doi.org/10.1007/s10509-018-3428-5 en_US
dc.description.abstract Formation of black holes may be constrained by intrinsic parameters characterizing them such as electric charge. Here we discuss the effects of a relatively minute excess of charge on extremal black hole formation and the horizon. We extend the implications of this argument to the formation of primordial black holes (PBH) in the early universe which gives a possible reason for the lack of detection of Hawking radiation. These charge limits also apply to dark matter (DM) particles that may form PHBs in the early universe. The constraint thus obtained on the electric charge of DM particles could also account for the required magnitude of the repulsive dark energy (DE) currently causing an accelerated universe which provides a possible unified picture of DM and DE. en_US
dc.language.iso en en_US
dc.publisher Springer en_US
dc.subject Extremal black hole en_US
dc.subject Primordial black holes en_US
dc.subject Dark matter en_US
dc.subject Dark energy en_US
dc.title Extremal charged black holes, dark matter and dark energy en_US
dc.type Article en_US


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