Recent developments in string compactifications demonstrate obstructions to the simplest constructions of low energy cosmologies with positive vacuum energy. The existence of obstacles to creating scale-separated de Sitter solutions indicates a UV/IR puzzle for embedding cosmological vacua in a unitary theory of quantum gravity. Motivated by this puzzle, we propose an embedding of positive energy Friedmann-Lemaitre-Robertson-Walker cosmology within string theory. Our proposal involves confining 4D gravity on a brane which mediates the decay from a nonsupersymmetric five-dimensional anti-de Sitter false vacuum to a true vacuum. In this way, it is natural for a 4D observer to experience an effective positive cosmological constant coupled to m...
In this paper we construct a stringy embedding of the dark bubble model of an expanding 4D cosmology...
Stages of accelerated expansion during the history of the universe - both a very late and very early...
Stages of accelerated expansion during the history of the universe - both a very late and very early...
Recent developments in string compactifications demonstrate obstructions to the simplest constructio...
Constructing an explicit compactification yielding a metastable de Sitter (dS) vacuum in a UV consis...
Constructing an explicit compactification yielding a metastable de Sitter (dS) vacuum in a UV consis...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Finding four-dimensional de Sitter spacetime solutions in string theory has been a vexing quest ever...
In this paper we construct a stringy embedding of the dark bubble model of an expanding 4D cosmology...
In this paper we construct a stringy embedding of the dark bubble model of an expanding 4D cosmology...
Stages of accelerated expansion during the history of the universe - both a very late and very early...
Stages of accelerated expansion during the history of the universe - both a very late and very early...
Recent developments in string compactifications demonstrate obstructions to the simplest constructio...
Constructing an explicit compactification yielding a metastable de Sitter (dS) vacuum in a UV consis...
Constructing an explicit compactification yielding a metastable de Sitter (dS) vacuum in a UV consis...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Our understanding of cosmology has evolved radically in the last decades. Current models demand the ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Motivated by the lack of consensus on whether or not de Sitter (dS) lies in the Swampland, we use a ...
Finding four-dimensional de Sitter spacetime solutions in string theory has been a vexing quest ever...
In this paper we construct a stringy embedding of the dark bubble model of an expanding 4D cosmology...
In this paper we construct a stringy embedding of the dark bubble model of an expanding 4D cosmology...
Stages of accelerated expansion during the history of the universe - both a very late and very early...
Stages of accelerated expansion during the history of the universe - both a very late and very early...