We solve the Einstein equation in five-dimensional space-time for Randall–Sundrum Brane world model with time dependent radion field to study the variation of brane scale factor with time. We have shown that as the radion field decreases with time compactifying the extra dimension, the scale factor increases exponentially with time leading to an inflationary scenario. We have also proposed a time dependent generalization of the Goldberger–Wise moduli stabilization mechanism to explain the time evolution of the radion field to reach a stable value, after which the scale factor on the brane exits from inflationary expansion
We calculate the linearized metric perturbation corresponding to a massless four-dimensional scalar ...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
We study through holography the compact Randall-Sundrum (RS) model at finite temperature. In the pre...
We solve the Einstein equation in five-dimensional space-time for Randall–Sundrum Brane world model ...
We examine the cosmology of Randall-Sundrum model in a dynamic setting where scalar fields are prese...
We derive a general formalism for constructing a four-dimensional effective action for the radion fi...
We find a static solution to Einstein's field equations on a five-dimensional orbifold with a compac...
[[abstract]]The success of the Randall-Sundrum scenario relies on stabilization of the modulus held ...
We discuss cosmology of models with universal extra dimensions, where the Standard Model degrees of ...
We investigate cosmological evolutions of the bulk scalar field $\phi(t)$ and the radion $d(t)$ in f...
Abstract We propose a new radion stabilization mechanism in the Randall-Sundrum spacetime, introd...
Abstract 5D warped extra dimension models with multiple 3-branes can naturally realize multiple hier...
We study the averaged action of the Randall-Sundrum model with a time-dependent metric ansatz. It ca...
We explore the phenomenology of a stabilized modulus field in the Randall-Sundrum scenario. It is fo...
We construct brane effective action induced by the bulk gravitational dynamics in two brane Randall-...
We calculate the linearized metric perturbation corresponding to a massless four-dimensional scalar ...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
We study through holography the compact Randall-Sundrum (RS) model at finite temperature. In the pre...
We solve the Einstein equation in five-dimensional space-time for Randall–Sundrum Brane world model ...
We examine the cosmology of Randall-Sundrum model in a dynamic setting where scalar fields are prese...
We derive a general formalism for constructing a four-dimensional effective action for the radion fi...
We find a static solution to Einstein's field equations on a five-dimensional orbifold with a compac...
[[abstract]]The success of the Randall-Sundrum scenario relies on stabilization of the modulus held ...
We discuss cosmology of models with universal extra dimensions, where the Standard Model degrees of ...
We investigate cosmological evolutions of the bulk scalar field $\phi(t)$ and the radion $d(t)$ in f...
Abstract We propose a new radion stabilization mechanism in the Randall-Sundrum spacetime, introd...
Abstract 5D warped extra dimension models with multiple 3-branes can naturally realize multiple hier...
We study the averaged action of the Randall-Sundrum model with a time-dependent metric ansatz. It ca...
We explore the phenomenology of a stabilized modulus field in the Randall-Sundrum scenario. It is fo...
We construct brane effective action induced by the bulk gravitational dynamics in two brane Randall-...
We calculate the linearized metric perturbation corresponding to a massless four-dimensional scalar ...
This paper presents some cosmological consequences of the five dimensional, two brane Randall-Sundru...
We study through holography the compact Randall-Sundrum (RS) model at finite temperature. In the pre...