Neutron star with dark matter admixture: A candidate for bridging the mass gap

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00387818" target="_blank" >RIV/68407700:21670/25:00387818 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1142/S0218271825500646" target="_blank" >https://doi.org/10.1142/S0218271825500646</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1142/S0218271825500646" target="_blank" >10.1142/S0218271825500646</a>

Result language
angličtina
Original language name
Neutron star with dark matter admixture: A candidate for bridging the mass gap
Original language description
Neutron stars, white dwarfs and black holes are the after death remnants of massive stars. However, according to the most recent observations, the neutron stars' maximum mass is between 2.0-2.5 M circle dot while black holes of less than 5 M circle dot have not yet been observed. The region between the most massive neutron star and the least massive black hole is called the mass gap. If indeed its existence is confirmed by future observations, that indicates a gap in our understanding which seeks for explanation. In addition, the existence of compact objects within the mass gap should also be supported with the help of possible new theoretical scenarios. In this study, we propose a possible explanation for the existence of compact objects within the mass gap region. Specifically, we propose that the mass gap region could be bridged by the existence of a hybrid compact object, composed of hadronic and self interacting and nonannihilating fermionic dark matter, considering that the interaction between these two fluids its only gravitational. Fundamental questions about how these objects form and how they can be detected are also addressed.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Project
<a href="/en/project/GA21-24281S" target="_blank" >GA21-24281S: Experiment IS581 "(d,p)-transfer induced fission of heavy radioactive beams"</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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