Vikiaris, MichaelMoustakidis, CharalambosVlasios PetousisVeselsky MartinTill today, the nature of dark matter remains elusive despite all our efforts. This missing matter of the universe has not been observed by the already operating dark matter direct-detection exper- iments, but we can infer its gravitational effects. Galaxies and clusters of galaxies are most likely to contain dark matter trapped to their gravitational field. This leads us to the natural assumption that compact objects might contain dark matter too. Among the compact objects exist in galaxies, neutron stars considered as natural laboratories, where theories can be tested, and observational data can be received. Thus, many models of dark matter they have proposed it’s presence in those stars. By employing the two fluid model, we discovered a stable area in the M-R diagram of a celestial formation consisting of neutron and dark matter that is substantial in size and vast in di- mensions. This formation spans hundreds of kilometers in diameter and possesses a mass equivalent to 100 or more times that of our sun. To elucidate, this entity resembles an enormous celestial body of dark matter, with a neutron star at its core. This implies that a supramassive stellar compact entity can exist without encountering any issues of stability and without undergoing a collapse into a black hole. In any case, the present theoretical prediction can, if combined with corresponding observations, shed light on the existence of dark matter and even more on its basic properties.application/pdf10.12681/hnpsanp.6270https://eproceedings.epublishing.ekt.gr/index.php/hnps/article/view/6270engHellenic Nuclear Physics Society (HNPS)Πνευματική ιδιοκτησία (c) 2024 Michael Vikiaris, Charalambos Moustakidis, Vlasios Petousis, Veselsky Martinhttp://creativecommons.org/licenses/by-nc-nd/4.0Annual Symposium of the Hellenic Nuclear Physics Society2654-00882654-007XAnnual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 30 (2024); 96-103HNPS Advances in Nuclear Physics; Vol. 30 (2024): HNPS2023; 96-103Neutron StarTwo Fluid ModelCompact ObjectDark MatterSupermassive ObjectSupramassive dark objects with neutron star origininfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersion2024-07-31Πυρηνική φυσικήNuclear Physicsisi - Physics, Nuclear includes resources on the study of nuclear structure, decay, radioactivity, reactions, and scattering. Resources in this category focus on low-energy physics. High-energy physics is covered in the PHYSICS, PARTICLES & FIELDS category.Άρθρο συνεδρίουConference articleΕπιστημονικό άρθροScientific articleHellenic Nuclear Physics SocietyGreek Aggregator OpenArchives.gr | National Documentation Centre (EKT)