Five-dimensional Brans-Dicke \(M^{1}\times R^{3}\times S^{1}\) cosmology with chameleon scalar field

DOI10.1007/s10509-010-0281-6zbMath1187.83078OpenAlexW1981052316MaRDI QIDQ973716

Ahmad Rami El-Nabulsi

Publication date: 26 May 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0281-6

zbMATH Keywords

chameleonvacuum energyBrans-Dicke cosmologyaccelerated expansiondark energyphantom energygrowing matter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (6)

Statefinder parameters for different dark energy models with variable \(G\) correction in Kaluza-Klein cosmology ⋮ Accelerated expansion from a modified-quadratic gravity ⋮ FRW models with particle creation in Brans-Dicke theory ⋮ Behavior of holographic Ricci dark energy in scalar Gauss-Bonnet gravity for different choices of the scale factor ⋮ D-dimensional non-singular universe dominated by dark energy ⋮ Microscopic wormholes, extra-dimensions and cold dark matter from N = 2 maximal supergravity with Gauss–Bonnet corrections

Cites Work

• Generalized second law of thermodynamics in quintom dominated universe
• Interacting holographic dark energy model in non-flat universe
• The holographic dark energy in non-flat Brans-Dicke cosmology
• Accelerated cosmic expansion from Gauss-Bonnet curvature corrections, nonminimal coupling, and infrared second-order gauge gravity
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• EFFECTIVE 3-BRANE BRANS–DICKE COSMOLOGY
• HOLOGRAPHIC CHAPLYGIN DGP COSMOLOGIES
• MAXWELL BRANE COSMOLOGY WITH HIGHER-ORDER STRING CURVATURE CORRECTIONS, A NONMINIMALLY COUPLED SCALAR FIELD, DARK MATTER–DARK ENERGY INTERACTION AND A VARYING SPEED OF LIGHT
• MODIFIED BRANEWORLD COSMOLOGIES IN THE PRESENCE OF STRINGY CORRECTIONS COUPLED TO A CANONICAL SCALAR FIELD
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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