Supramassive dark objects with neutron star origin
M. Vikiaris, V. Petousis, M. Veselsky, and Ch.C. Moustakidis

TL;DR
This paper proposes a theoretical model of large, stable dark matter-embedded objects with neutron star cores, potentially revealing properties of dark matter through astrophysical observations.
Contribution
It introduces a two-fluid model predicting stable, massive dark matter-neutron star objects spanning hundreds of kilometers, expanding understanding of dark matter's role in compact objects.
Findings
Existence of stable, massive DM-neutron star objects in the M-R diagram.
Objects can reach hundreds of kilometers in size and over 100 solar masses.
These entities could help identify dark matter properties through observations.
Abstract
Till today, the nature of Dark Matter (DM) remains elusive despite all our efforts. This missing matter of the universe has not been observed by the already operating DM direct-detection experiments, but we can infer its gravitational effects. Galaxies and clusters of galaxies are most likely to contain DM trapped to their gravitational field. This leads us to the natural assumption that compact objects might contain DM too. Among the compact objects exist in galaxies, neutron stars are considered as natural laboratories, where theories can be tested, and observational data can be received. Thus, many models of DM have proposed it's presence in those stars. In particular, in the present study we focus on two types of dark matter particles, namely fermions and bosons with a mass range of [0.01-1.5] GeV and self-interaction strength in the range [10-10] MeV. By…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Solar and Space Plasma Dynamics · Astrophysics and Cosmic Phenomena
