Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Karkevandi, Davood Rafiei"'
Publikováno v:
Particles 2024, 7(1), 201-213
The presence of dark matter (DM) within neutron stars (NSs) can be introduced by different accumulation scenarios in which DM and baryonic matter (BM) may interact only through the gravitational force. In this work, we consider asymmetric self-intera
Externí odkaz:
http://arxiv.org/abs/2402.18696
Dark matter remains a topic of ongoing controversy. It has gained attention in the theoretical description of compact objects such as neutron stars with cores of very dense matter. Various candidates have been proposed for dark matter in the scientif
Externí odkaz:
http://arxiv.org/abs/2402.18686
Publikováno v:
Phys.Rev.D 109 (2024) 4, 043029
We explore the presence of self-interacting bosonic dark matter (DM) within neutron stars (NSs) in light of the latest multi-messenger observations of the Neutron Star Interior Composition Explorer (NICER) and LIGO/Virgo detectors. The bosonic DM is
Externí odkaz:
http://arxiv.org/abs/2210.17308
Publikováno v:
Published by the World Scientific, Proceedings of the MG16 Meeting, pp. 3713-3731 (2023)
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
Externí odkaz:
http://arxiv.org/abs/2112.14231
Publikováno v:
Phys. Rev. D 105, 023001 (2022)
We study an impact of self-interacting bosonic dark matter (DM) on various observable properties of neutron stars (NSs). The analysis is performed for asymmetric DM with masses from few MeV to GeV, the self-coupling constant of order $\mathcal{O}(1)$
Externí odkaz:
http://arxiv.org/abs/2109.03801
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
The Sixteenth Marcel Grossmann Meeting.
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
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.