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Brane-world cosmology and varying G
(World Scientific, 2010-07)
We consider a brane-world cosmological model coupled to a bulk scalar field. Since the brane tension turns out to be proportional to Newton’s coupling G, in such a model a time variation of G naturally occurs. By resorting ...
The low energy problem on astrophysics braneworld
(Facultad Experimental de Ciencias de la Universidad del Zulia, 2010)
Smooth braneworld models possibility in modified gravities
(World Scientific Publ Co Pte Ltd, 2015-10-01)
In this paper, it is shown that the consideration of the braneworld consistency conditions within the framework of bulk modified gravities allows for the existence of thick branes in the five-dimensional case with compact ...
Braneworlds scenarios in a gravity model with higher order spatial three-curvature terms
(Springer, 2013-04-04)
Vacuum thin shells in Einstein-Gauss-Bonnet brane-world cosmology
(IOP Publishing, 2018-03)
In this paper we construct new solutions of the Einstein-Gauss-Bonnet field equations in an isotropic Shiromizu-Maeda-Sasaki brane-world setting which represent a couple of Z 2-symmetric vacuum thin shells splitting from ...
Gauss-Codazzi formalism to brane-world within Brans-Dicke theory
(Springer, 2008-05-01)
We apply the Gauss-Codazzi formalism to brane-worlds within the framework of Brans-Dicke gravity. The compactification is taken from six to five dimensions in order to formalize brane-world models with hybrid compactification ...
Braneworld effective field theories — holography, consistency and conformal effects
(2020-04-01)
Braneworld theories are often described as low-energy effective field theories (EFTs) featuring an infinitely thin 3-brane and 4D fields exactly localized on it. We investigate whether an exactly localized braneworld can ...
Crossing the phantom divide with k-essence in braneworlds
(World Scientific, 2010-06)
We study a flat three-brane in the presence of a linear k field with nonzero cosmological constant Λ4. In this model the crossing of the phantom divide (PD) occurs when the k-essence energy density becomes negative. We ...
Anti-de sitter curvature radius constrained by quasars in brane-world scenarios
(World Scientific Publ Co Pte LtdSingaporeSingapura, 2005)