Equilibrium stellar configurations in Rastall theory and astrophysical implications
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Publication:5113739
DOI10.1142/S0217732320501059zbMath1435.83126arXiv1807.00812OpenAlexW3008108613MaRDI QIDQ5113739
Publication date: 16 June 2020
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.00812
Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Related Items (2)
Stellar structure models in modified theories of gravity: lessons and challenges ⋮ On black holes surrounded by a fluid of strings in Rastall gravity
Cites Work
- Bouncing solutions in Rastall's theory with a barotropic fluid
- Thermodynamics of flat FLRW universe in Rastall theory
- Physical acceptability of isolated, static, spherically symmetric, perfect fluid solutions of Einstein's equations
- Rastall gravity is equivalent to Einstein gravity
- Thermodynamic analysis of the static spherically symmetric field equations in Rastall theory
- Black hole solutions surrounded by perfect fluid in Rastall theory
- Impact of the Rastall parameter on perfect fluid spheres
- The trace-free Einstein equations and inflation
- Generalization of the Einstein Theory
- Unimodular relativity and cosmological constant
- On the trace-free Einstein equations as a viable alternative to general relativity
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- General relativistic stars: Linear equations of state
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