Behavior of anisotropic fluids with Chaplygin equation of state in Buchdahl spacetime
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Publication:2667409
DOI10.1007/S10714-021-02883-3zbMath1486.86003arXiv2104.13004OpenAlexW3158303899MaRDI QIDQ2667409
Abhijit Sarkar, Amit Kumar Prasad, Jitendra Kumar
Publication date: 4 March 2022
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2104.13004
Black holes (83C57) Seismology (including tsunami modeling), earthquakes (86A15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Statistical thermodynamics (82B30)
Cites Work
- Unnamed Item
- On charged analogues of Buchdahl's type fluid spheres
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- The stability of relativistic stars and the role of the adiabatic index
- On the most general accurate solutions for Buchdahl's fluid spheres
- Effect of pressure anisotropy on Buchdahl-type relativistic compact stars
- A class of new solutions of generalized charged analogues of Buchdahl's type super-dense star
- Some exact anisotropic solutions in general relativity
- Relativistic anisotropic models for compact star with equation of state p = f(ρ)
- Anisotropic spheres in general relativity reexamined
- General Relativistic Fluid Spheres
- Stable dark energy stars
- Bounds on the basic physical parameters for anisotropic compact general relativistic objects
- Anisotropic stars in general relativity
- Relativistic charged spheres: compact stars, compactness and stable configurations
- Influence of the equation of state on a compact star made of hidden-sector nucleons
- Charged anisotropic matter with a linear equation of state
- The contraction of gravitating spheres
- MAXIMUM MASS OF A CLASS OF COLD COMPACT STARS
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
- An alternative to quintessence
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