Neutron stars inf(R) gravity and scalar-tensor theories
From MaRDI portal
Publication:5861856
DOI10.1088/1475-7516/2019/09/054OpenAlexW3102676254MaRDI QIDQ5861856
Ryotaro Kase, Shinji Tsujikawa
Publication date: 2 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1906.08954
Related Items (7)
Stellar structure models in modified theories of gravity: lessons and challenges ⋮ BPS Skyrme neutron stars in generalized gravity ⋮ Linear stability of Bardeen anti-de Sitter thin-shell wormhole in f(R) gravity ⋮ Gravastars in modified Gauss-Bonnet gravity ⋮ Emergent gravity as the eraser of anomalous gauge boson masses, and QFT-GR concord ⋮ Instability of compact stars with a nonminimal scalar-derivative coupling ⋮ Anti-de Sitter neutron stars in the theory of gravity with nonminimal derivative coupling
Cites Work
- Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
- \(f(R)\) theories
- \(1/R\) gravity and scalar-tensor gravity
- A no-hair theorem for spherically symmetric black holes in \(R^2\) gravity
- Structure of neutron stars in \(R\)-squared gravity
- A new type of isotropic cosmological models without singularity
- Black hole solutions in \(R^{2}\) gravity
- Spherically symmetric black holes in f ( R ) gravity: is geometric scalar hair supported?
- 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
- Are<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>Dark Energy Models Cosmologically Viable?
- Mach's Principle and a Relativistic Theory of Gravitation
- Junction Conditions in f(R) Theories of Gravity
- The Scalar-Tensor Theory of Gravitation
- A no-hair theorem for black holes in f ( R ) gravity
- Analytical representations of unified equations of state of neutron-star matter
- CURVATURE QUINTESSENCE
- Equation-of-state of neutron stars with junction conditions in the Starobinsky model
- The confrontation between general relativity and experiment
This page was built for publication: Neutron stars inf(R) gravity and scalar-tensor theories