AbstractWe report on explicit cosmological solutions within the framework of an inflating de Sitter brane embedded in five- and ten-dimensional bulk spacetimes. In the specific example we study the brane tension is induced by the curvature related to the expansion of a physical 3+1 spacetime rather than by a bulk cosmological term. In a generic situation with nonzero brane tension, the expansion of the universe accelerates eventually. We also show that inflationary cosmology is possible for a wide class of metrics without violating four- and higher-dimensional null energy condition
We derive the effective cosmological equations for a non-$\mathbb{Z}_2$ symmetric codimension one br...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We propose a cosmological model which exhibits the phenomenon of self-acceleration: the Universe is ...
AbstractWe report on explicit cosmological solutions within the framework of an inflating de Sitter ...
We find cosmological solution corresponding to compactification of 10d supergravity on a warped coni...
AbstractThe standard Friedmann universe embedded in a five-dimensional bulk with constant curvature ...
AbstractWe study cosmological aspects of braneworld models with a warped dimension and an arbitrary ...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
We generalize solutions of Einstein's equations for intersecting branes in higher dimensional spacet...
AbstractWe present a cosmological model in 1+m+p dimensions, where in m-dimensional space there are ...
We propose a supergravity derivation of the Randall-Sundrum action as an effective description of th...
AbstractWe study a 5-dimensional f(R) brane gravity within the framework of scalar-tensor type theor...
A brane universe moving in a curved higher-dimensional bulk space is considered. The motion induces ...
We solve the Einstein equations in higher dimensions with warped geometry where an extra dimension i...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We derive the effective cosmological equations for a non-$\mathbb{Z}_2$ symmetric codimension one br...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We propose a cosmological model which exhibits the phenomenon of self-acceleration: the Universe is ...
AbstractWe report on explicit cosmological solutions within the framework of an inflating de Sitter ...
We find cosmological solution corresponding to compactification of 10d supergravity on a warped coni...
AbstractThe standard Friedmann universe embedded in a five-dimensional bulk with constant curvature ...
AbstractWe study cosmological aspects of braneworld models with a warped dimension and an arbitrary ...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
We generalize solutions of Einstein's equations for intersecting branes in higher dimensional spacet...
AbstractWe present a cosmological model in 1+m+p dimensions, where in m-dimensional space there are ...
We propose a supergravity derivation of the Randall-Sundrum action as an effective description of th...
AbstractWe study a 5-dimensional f(R) brane gravity within the framework of scalar-tensor type theor...
A brane universe moving in a curved higher-dimensional bulk space is considered. The motion induces ...
We solve the Einstein equations in higher dimensions with warped geometry where an extra dimension i...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We derive the effective cosmological equations for a non-$\mathbb{Z}_2$ symmetric codimension one br...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We propose a cosmological model which exhibits the phenomenon of self-acceleration: the Universe is ...