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Gravitationally decoupled anisotropic compact stars immersed in Dehnen-(1,4,0) density profiles

The term cosmic dark matter is commonly studied in the context of galactic rotation profiles, particularly along the outer galactic halo. However, its influence may differ significantly in dense-matter astrophysical configurations characterized by strong gravitational fields. In this study, we const...

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מידע ביבליוגרפי
Principais autores: S. Khan, Javlon Rayimbaev, Otaboyev Sirajiddin, Yunus Turaev, Sulton Usanov, Aybek Seytov
פורמט: Artigo
שפה:Inglês
יצא לאור: Elsevier 2026-03-01
סדרה:Nuclear Physics B
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גישה מקוונת:http://www.sciencedirect.com/science/article/pii/S0550321326000647
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