Compact static stars in minimal dilatonic gravity
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Publication:5367513
DOI10.1142/S0217732317501413zbMath1372.83058arXiv1402.2813MaRDI QIDQ5367513
Publication date: 13 October 2017
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1402.2813
Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)
Cites Work
- Unnamed Item
- Nonperturbative models of quark stars in \(f(R)\) gravity
- \(f(R)\) theories
- A new type of isotropic cosmological models without singularity
- Relativistic Hydrodynamics
- <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
- Singularity Problem with<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>Models for Dark Energy
- Mach's Principle and a Relativistic Theory of Gravitation
- On Massive Neutron Cores
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