An exponential \(F(R)\) dark energy model
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Publication:2435129
DOI10.1007/s10714-013-1597-7zbMath1283.83033arXiv1304.4089OpenAlexW1984788754MaRDI QIDQ2435129
Publication date: 3 February 2014
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1304.4089
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
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Cites Work
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- Notes on wormhole existence in scalar-tensor and \(F(R)\) gravity
- \({f(\mathcal R)}\) quantum cosmology
- Born-Infeld quantum condensate as dark energy in the universe
- Quantum de Sitter cosmology and phantom matter
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- <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?
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
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- STOCHASTIC BACKGROUND OF GRAVITATIONAL WAVES "TUNED" BY f(R) GRAVITY
- CONSISTENCY CONDITION OF SPHERICALLY SYMMETRIC SOLUTIONS IN f(R) GRAVITY
- PHANTOM AND QUANTUM MATTER IN AN ANTI DE SITTER UNIVERSE
- QUANTUM EFFECTS AND STABILITY OF CHAMELEON COSMOLOGY
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