EFFECTIVE 3-BRANE BRANS–DICKE COSMOLOGY
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Publication:3529006
DOI10.1142/S0217732308026327zbMath1153.83392OpenAlexW2061290955MaRDI QIDQ3529006
Publication date: 17 October 2008
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0217732308026327
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (12)
Bianchi type-I dust-filled accelerating Brans-Dicke cosmology ⋮ MODIFIED BRANEWORLD COSMOLOGIES IN THE PRESENCE OF STRINGY CORRECTIONS COUPLED TO A CANONICAL SCALAR FIELD ⋮ Accelerated expansion from a modified-quadratic gravity ⋮ Accelerated brans-dicke universe in higher-derivative induced gravity-like conformally coupling and dominated by Gauss-Bonnet dark energy ⋮ D-dimensional non-singular universe dominated by dark energy ⋮ Five-dimensional Brans-Dicke \(M^{1}\times R^{3}\times S^{1}\) cosmology with chameleon scalar field ⋮ Accelerated cosmic expansion from Gauss-Bonnet curvature corrections, nonminimal coupling, and infrared second-order gauge gravity ⋮ Living with phantoms fields in a sheet spacetime ⋮ Dark energy from ``extended modified gravity and Gauss-Bonnet invariant term ⋮ A dark energy and phantom energy dilaton-Brans-Dicke multiverse with positive cosmological constant ⋮ Accelerated expansion of an anisotropic Brans-Dicke cosmology from nonlinear derivative interaction and Gauss-Bonnet invariant ⋮ 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
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