The generalized second law of thermodynamics for interacting f(R) gravity
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Publication:2878897
DOI10.1142/S0218271814500710zbMath1295.83049arXiv1406.6305OpenAlexW3105670372MaRDI QIDQ2878897
Publication date: 5 September 2014
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1406.6305
Relativistic cosmology (83F05) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05)
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Cites Work
- Modified Gauss-Bonnet theory as gravitational alternative for dark energy
- Friedmann equations of FRW universe in scalar-tensor gravity, \(f(R)\) gravity and first law of thermodynamics
- Particle creation by black holes
- \(f(R)\) theories
- Thermodynamic behavior of field equations for \(f(R)\) gravity
- Thermodynamical description of the interaction between holographic dark energy and dark matter
- Le Châtelier-Braun principle in cosmological physics
- Cosmological constant -- the weight of the vacuum
- Late time acceleration in \(f(G)\) model
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- New general relativity
- Dark Energy
- <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
- The cosmological constant and 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?
- Exact cosmological solutions of scale-invariant gravity theories
- Cosmological horizons and entropy
- Generalized Second Law in Cosmology from Causal Boundary Entropy
- Black hole entropy is the Noether charge
- CURVATURE QUINTESSENCE
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Black Holes and Entropy
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmology in three dimensions: steps towards the general solution
- The graceful exit in pre-big bang string cosmology
- Interacting quintessence
- Density perturbations in the ekpyrotic Universe and string-inspired generalizations
