Inflationary solutions are constructed in a specific five-dimensional model with boundaries motivated by heterotic M theory. We concentrate on the case where the vacuum energy is provided by potentials on those boundaries. It is pointed out that the presence of such potentials necessarily excites bulk fields. We distinguish a linear and a non-linear regime for those modes. In the linear regime, inflation can be discussed in an effective four-dimensional theory in the conventional way. This effective action is derived by integrating out the bulk modes. Therefore, these modes do not give rise to excited Kaluza-Klein modes from a four-dimensional perspective. We lift a four-dimensional inflating solution up to five dimensions where it represen...
doi:10.1088/1475-7516/2005/07/007 Abstract. In the model of chain inflation, a sequential chain of c...
We present a new mechanism for slow-roll inflation based on higher dimen-sional supersymmetric gauge...
AbstractThe universe may have extra spatial dimensions with large volume that we cannot perceive bec...
We analyze the existence of inflationary solutions in an inhomogeneous Kaluza-Klein cosmological mod...
Change of title : On the problem of inflation in nonlinear multidimensional cosmological models. We ...
The evolution of slow--roll inflation in a five--dimensional brane world model with two boundary bra...
In this thesis, we discuss time-dependent solutions of the low-energy limit of heterotic M-theory. I...
In the context of a five-dimensional brane-world model motivated from heterotic M-theory, we develop...
We introduce a $(5+m)$-dimensional vacuum description of five-dimensional bulk inflaton models with ...
Abstract. Slow-roll inflation requires the inflaton field to have an exceptionally flat potential, w...
We analyze the onset of inflation for a simple single-field model when the system begins with signif...
Randall and Sundrum have proposed that we live on a brane embedded in 5-dimensional anti-deSitter sp...
Recently we introduced an inflationary setup in which the inflaton fields are matrix valued scalar f...
Inflation in a five-dimensional brane world model with two boundary branes is studied. We make use o...
We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cyl...
doi:10.1088/1475-7516/2005/07/007 Abstract. In the model of chain inflation, a sequential chain of c...
We present a new mechanism for slow-roll inflation based on higher dimen-sional supersymmetric gauge...
AbstractThe universe may have extra spatial dimensions with large volume that we cannot perceive bec...
We analyze the existence of inflationary solutions in an inhomogeneous Kaluza-Klein cosmological mod...
Change of title : On the problem of inflation in nonlinear multidimensional cosmological models. We ...
The evolution of slow--roll inflation in a five--dimensional brane world model with two boundary bra...
In this thesis, we discuss time-dependent solutions of the low-energy limit of heterotic M-theory. I...
In the context of a five-dimensional brane-world model motivated from heterotic M-theory, we develop...
We introduce a $(5+m)$-dimensional vacuum description of five-dimensional bulk inflaton models with ...
Abstract. Slow-roll inflation requires the inflaton field to have an exceptionally flat potential, w...
We analyze the onset of inflation for a simple single-field model when the system begins with signif...
Randall and Sundrum have proposed that we live on a brane embedded in 5-dimensional anti-deSitter sp...
Recently we introduced an inflationary setup in which the inflaton fields are matrix valued scalar f...
Inflation in a five-dimensional brane world model with two boundary branes is studied. We make use o...
We discuss a semiclassical treatment to inflationary models from Kaluza-Klein theory without the cyl...
doi:10.1088/1475-7516/2005/07/007 Abstract. In the model of chain inflation, a sequential chain of c...
We present a new mechanism for slow-roll inflation based on higher dimen-sional supersymmetric gauge...
AbstractThe universe may have extra spatial dimensions with large volume that we cannot perceive bec...