Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7651
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dc.contributor.authorSandeep, S. K-
dc.contributor.authorArun, K-
dc.contributor.authorSivaram, C-
dc.date.accessioned2020-05-21T11:14:40Z-
dc.date.available2020-05-21T11:14:40Z-
dc.date.issued2020-05-
dc.identifier.citationPhysics of the Dark Universe, Vol. 28, 100507en_US
dc.identifier.issn2212-6864-
dc.identifier.urihttp://hdl.handle.net/2248/7651-
dc.descriptionRestricted Accessen_US
dc.description.abstractObservations have indicated that we do not see neutron stars (NS) of mass near the theoretical upper limit as predicted. Here we invoke the role of dark matter (DM) particles in star formation, and their role in lowering the mass of remnants eventually formed from these stars. Massive stars can capture DM particles more effectively than the lower mass stars, thus further softening the equation of state of the remnant neutron stars. We also look at the capture of DM particles by the NS, which could further soften the upper mass limit of NS. The admixture of DM particles would be higher at earlier epochs (high z).en_US
dc.language.isoenen_US
dc.publisherElsevier B.V.en_US
dc.relation.urihttps://doi.org/10.1016/j.dark.2020.100507-
dc.rights© Elsevier B.V-
dc.subjectDark matteren_US
dc.subjectEarly epochen_US
dc.subjectNeutron starsen_US
dc.subjectStar formationen_US
dc.titleEffects of dark matter on the upper bound mass of neutron starsen_US
dc.typeArticleen_US
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