Tidal Deformability as a Probe of Dark Matter in Neutron Stars

The concept of boson stars (BSs) was first introduced by Kaup and Ruffini-Bonazzola in the 1960s. Following this idea, we investigate an effect of self-interacting asymmetric bosonic dark matter (DM) according to Colpi et al. model for BSs (1986) on different observable properties of neutron stars (...

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Veröffentlicht in:arXiv.org 2021-12
Hauptverfasser: Davood Rafiei Karkevandi, Shakeri, Soroush, Sagun, Violetta, Ivanytskyi, Oleksii
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Sprache:eng
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