A new class of relativistic model of compact stars of embedding class I
From MaRDI portal
Publication:5363936
DOI10.1142/S0218271817500900zbMath1371.85005arXiv1703.03289OpenAlexW2594788460MaRDI QIDQ5363936
P. Bhar, Tuhina Manna, Ksh. Newton Singh
Publication date: 2 October 2017
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1703.03289
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Galactic and stellar structure (85A15)
Related Items (7)
Relativistic Krori‐Barua Compact Stars in f(R,T)$f(R,T)$ Gravity ⋮ Comprehensive analysis of relativistic embedded class-I exponential compact spheres in f(R, ϕ) gravity via Karmarkar condition ⋮ On evolution of compact stars from string fluid in Rastall gravity ⋮ Anisotropic fluid spheres satisfying the Karmarkar condition ⋮ Explicit isometric embeddings of collapsing dust ball ⋮ Embedded class-i solution of compact stars in \(f(R)\) gravity with Karmarkar condition ⋮ Relativistic fluid spheres with Karmarkar condition
Cites Work
- Unnamed Item
- Sharp bounds on the critical stability radius for relativistic charged spheres
- Insufficiency of Karmarkar's condition
- General Relativistic Fluid Spheres
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- Anisotropic stars in general relativity
- ANISOTROPIC COMPACT STARS WITH VARIABLE COSMOLOGICAL CONSTANT
- Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
- The contraction of gravitating spheres
- Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- General solution for a class of static charged spheres
This page was built for publication: A new class of relativistic model of compact stars of embedding class I