Predicting signatures of string theory on cosmological observables is not sufficient. Often the observable effects string theory may impact upon the cosmological arena may equally be predicted by features of inflationary physics. The question: what observable signatures are unique to new physics, is thus of crucial importance for claiming evidence for the theory. Here we discuss recent progress in addressing the above question.The evidence relies on identifying discrepancies between the source terms that give rise to large scale structure (LSS) and CMB, by cross-correlating the weak lensing potential that maps LSS with the CMB spectra
String cosmology is a rapidly changing field, which is still in its early days. One of the most prom...
In string theory, the traditional picture of a Universe that emerges from the inflation of a very sm...
To a good approximation our Universe is flat and homogeneous, and possesses perturbations which, alb...
Predicting signatures of string theory on cosmological observables is not sufficient. Often the obse...
Predicting signatures of string theory on cosmological observables is not sufficient. Often the obse...
We propose a new method for identifying new physics imprints on present observational data in cosmol...
The cosmic string theory for cosmological fluctuations is a good example of healthy scientific progr...
In spite of its great phenomenological success, current models of scalar field-driven inflation suff...
Brane inflation is a specific realization of the inflationary universe scenario in the early univers...
I discuss cosmological models either derived from, or inspired by, string theory or M-theory. In par...
This article briefly summarizes the motivations for -- and recent progress in -- searching for cosmo...
Recent developments in string theory have important implications for cosmology. Topics discussed her...
These lectures present a brief review of inflationary cosmology, provide an overview of the theory o...
This is the second paper in the series that confronts predictions of a model of the landscape with c...
The Wilkinson Microwave Anisotropy Probe microwave background data may be giving us clues about new ...
String cosmology is a rapidly changing field, which is still in its early days. One of the most prom...
In string theory, the traditional picture of a Universe that emerges from the inflation of a very sm...
To a good approximation our Universe is flat and homogeneous, and possesses perturbations which, alb...
Predicting signatures of string theory on cosmological observables is not sufficient. Often the obse...
Predicting signatures of string theory on cosmological observables is not sufficient. Often the obse...
We propose a new method for identifying new physics imprints on present observational data in cosmol...
The cosmic string theory for cosmological fluctuations is a good example of healthy scientific progr...
In spite of its great phenomenological success, current models of scalar field-driven inflation suff...
Brane inflation is a specific realization of the inflationary universe scenario in the early univers...
I discuss cosmological models either derived from, or inspired by, string theory or M-theory. In par...
This article briefly summarizes the motivations for -- and recent progress in -- searching for cosmo...
Recent developments in string theory have important implications for cosmology. Topics discussed her...
These lectures present a brief review of inflationary cosmology, provide an overview of the theory o...
This is the second paper in the series that confronts predictions of a model of the landscape with c...
The Wilkinson Microwave Anisotropy Probe microwave background data may be giving us clues about new ...
String cosmology is a rapidly changing field, which is still in its early days. One of the most prom...
In string theory, the traditional picture of a Universe that emerges from the inflation of a very sm...
To a good approximation our Universe is flat and homogeneous, and possesses perturbations which, alb...