We analyze the possibility of realizing inflation with a subsequent dS vacuum in the K\'ahler uplifting scenario. The inclusion of several quantum corrections to the 4d effective action evades previous no-go theorems and allows for construction of simple and successful models of string inflation. The predictions of several benchmark models are in accord with current observations, i.e., a red spectral index, negligible non-gaussianity, and spectral distortions similar to the simplest models of inflation. A particularly interesting subclass of models are 'left-rolling' ones, where the overall volume of the compactified dimensions shrinks during inflation. We call this phenomenon 'inflation by deflation' (IBD), where deflation refers to the in...
Abstract. Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive v...
It is notoriously difficult to engineer successful models of inflation and late time expansion in st...
We give an overview of flux compactification and a brief introduction to the present ...
We analyze the possibility of realizing inflation with a subsequent dS vacuum in the Käahler uplifti...
Abstract. We analyze the possibility of realizing inflation with a subsequent dS vacuum in the Kähl...
The paradigm of inflation continues to be confirmed by experiments like WMAP, and will be probed mor...
I will discuss aspects of de Sitter space and inflation models of inflation in the context of string...
We introduce slow-roll inflation in string theory on both a conceptual level and a detailed one. In ...
Inflationary scenarios in string theory often involve a large number of light scalar fields, whose p...
We study a model of accidental inflation in type IIB string theory where inflation occurs near the...
In this dissertation, we discuss the possibility of detecting evidence for string theory in the sky....
We analyze a distinctive mechanism for inflation in which particle production slows down a scalar fi...
In this Master Thesis we study the effects of loop corrections to the inflationary potential of the ...
Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive vacuum ener...
We review recent trends in inflationary dynamics in the context of viable modified gravity theories....
Abstract. Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive v...
It is notoriously difficult to engineer successful models of inflation and late time expansion in st...
We give an overview of flux compactification and a brief introduction to the present ...
We analyze the possibility of realizing inflation with a subsequent dS vacuum in the Käahler uplifti...
Abstract. We analyze the possibility of realizing inflation with a subsequent dS vacuum in the Kähl...
The paradigm of inflation continues to be confirmed by experiments like WMAP, and will be probed mor...
I will discuss aspects of de Sitter space and inflation models of inflation in the context of string...
We introduce slow-roll inflation in string theory on both a conceptual level and a detailed one. In ...
Inflationary scenarios in string theory often involve a large number of light scalar fields, whose p...
We study a model of accidental inflation in type IIB string theory where inflation occurs near the...
In this dissertation, we discuss the possibility of detecting evidence for string theory in the sky....
We analyze a distinctive mechanism for inflation in which particle production slows down a scalar fi...
In this Master Thesis we study the effects of loop corrections to the inflationary potential of the ...
Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive vacuum ener...
We review recent trends in inflationary dynamics in the context of viable modified gravity theories....
Abstract. Higher-form flux that extends in all 3+1 dimensions of spacetime is a source of positive v...
It is notoriously difficult to engineer successful models of inflation and late time expansion in st...
We give an overview of flux compactification and a brief introduction to the present ...