A family of anisotropic super-dense star models using a space-time describing charged perfect fluid distributions
From MaRDI portal
Publication:2844866
DOI10.1088/0031-8949/86/02/025009zbMath1272.83037OpenAlexW2041704096MaRDI QIDQ2844866
Y. K. Gupta, Sunil Kumar Maurya
Publication date: 20 August 2013
Published in: Physica Scripta (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0031-8949/86/02/025009
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (7)
Charged fluid to anisotropic fluid distribution in general relativity ⋮ Relativistic modelling of stable anisotropic super-dense star ⋮ Anisotropic compact star model on Finch-Skea space-time ⋮ All static charged dust spheres in general relativity ⋮ Charge analogue of Tolman IV solution for anisotropic fluid ⋮ Realistic solutions of fluid spheres in \(f(\mathcal{G},\mathcal{T})\) gravity under Karmarkar condition ⋮ Relativistic strange stars in Tolman-Kuchowicz spacetime
This page was built for publication: A family of anisotropic super-dense star models using a space-time describing charged perfect fluid distributions
