Effects of dark matter in red giants

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