Strange stars in \(f(R)\) theories of gravity in the Palatini formalism
DOI10.1007/S10714-017-2230-YzbMath1381.83106arXiv1704.04961OpenAlexW2609874326MaRDI QIDQ1700334
Publication date: 5 March 2018
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1704.04961
Palatini formalismmodified theories of gravityrelativistic stars\(f(R)\) theories of gravityequations of state of strange star matter
Strong interaction, including quantum chromodynamics (81V05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (3)
Cites Work
- \(f(R)\) theories
- A new type of isotropic cosmological models without singularity
- Extended theories of gravity and their cosmological and astrophysical applications
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
- Spherically symmetric spacetimes in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity theories
- DYNAMICS OF DARK ENERGY
- Curvature singularities, tidal forces and the viability of Palatini f ( R ) gravity
- Static Solutions of Einstein's Field Equations for Spheres of Fluid
- On Massive Neutron Cores
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