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Effects of dark matter in red giants

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dc.contributor.author Clea, Sunny
dc.contributor.author Sivaram, C
dc.contributor.author Gudennavar, S. B
dc.date.accessioned 2021-02-07T06:07:40Z
dc.date.available 2021-02-07T06:07:40Z
dc.date.issued 2020-12
dc.identifier.citation Physics of the Dark Universe, Vol. 30, 100727 en_US
dc.identifier.issn 2212-6864
dc.identifier.uri http://hdl.handle.net/2248/7598
dc.description Restricted Access © Elsevier B.V. https://doi.org/10.1016/j.dark.2020.100727 en_US
dc.description.abstract Dark matter (DM) which constitutes five-sixths of all matter is hypothesized to be a weakly interacting non-baryonic particle, created in the early stages of cosmic evolution. It can affect various cosmic structures in the Universe via gravitational interactions. The effect of DM in main sequence stars and stellar remnants like neutron stars and white dwarfs has already been studied. Red giant phase is a late stage of the evolution of stars. In this work, we study, low-mass red giants stars with admixture of DM and how this can effectively change the intrinsic properties of red giants such as their luminosities, temperatures and lifetimes. en_US
dc.language.iso en en_US
dc.publisher Elsevier B. V. en_US
dc.subject Dark matter en_US
dc.subject Low-mass red giants en_US
dc.subject DM admixture en_US
dc.title Effects of dark matter in red giants en_US
dc.type Article en_US

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