AbstractWe present a cosmological model in 1+m+p dimensions, where in m-dimensional space there are uniformly distributed p-branes wrapping over the extra p dimensions. We find that during cosmological evolution m-dimensional space expands with the exact power-law corresponding to pressureless matter while the extra p dimensions contract. Adding matter, we also obtain solutions having the same property. We show that this might explain in a natural way why the extra dimensions are small compared to the observed three spatial directions
I present the main features of the brane cosmology scenario, according to which our universe is a se...
We study the late-time behavior of a universe in the framework of brane gas cosmology. We investigat...
In braneworld models a variable vacuum energy may appear if the size of the extra dimension changes ...
AbstractWe present a cosmological model in 1+m+p dimensions, where in m-dimensional space there are ...
introduced the study of the evolution of such models in a simple context we then go on to study a mo...
Many theories of particle physics rely on the existence of more than three spatial dimensions. In th...
We consider evolution of compact extra dimensions in cosmology and try to see whether wrapped branes...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
Latex file, 10 pagesThe evolution of the extra dimension is investigated in the context of brane wor...
AbstractWe report on explicit cosmological solutions within the framework of an inflating de Sitter ...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We reconsider theories with low gravitational (or string) scale M(*) where Newton's constant is gene...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
Recent developments in the physics of extra dimensions have opened up new avenues to test such theor...
I present the main features of the brane cosmology scenario, according to which our universe is a se...
We study the late-time behavior of a universe in the framework of brane gas cosmology. We investigat...
In braneworld models a variable vacuum energy may appear if the size of the extra dimension changes ...
AbstractWe present a cosmological model in 1+m+p dimensions, where in m-dimensional space there are ...
introduced the study of the evolution of such models in a simple context we then go on to study a mo...
Many theories of particle physics rely on the existence of more than three spatial dimensions. In th...
We consider evolution of compact extra dimensions in cosmology and try to see whether wrapped branes...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
Latex file, 10 pagesThe evolution of the extra dimension is investigated in the context of brane wor...
AbstractWe report on explicit cosmological solutions within the framework of an inflating de Sitter ...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
We reconsider theories with low gravitational (or string) scale M(*) where Newton's constant is gene...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
D-branes are fundamental in all scenarios where there are large extra dimensions and the string scal...
Recent developments in the physics of extra dimensions have opened up new avenues to test such theor...
I present the main features of the brane cosmology scenario, according to which our universe is a se...
We study the late-time behavior of a universe in the framework of brane gas cosmology. We investigat...
In braneworld models a variable vacuum energy may appear if the size of the extra dimension changes ...