The theory describing physics at the highest energy scales likely contains extra dimensions, whose internal degrees of freedom result in many massive field and particles. At accelerator experiments these fields and particles generally decouple from the low energy physics. However, in cosmology gravity couples everything, thereby invalidating the decoupling assumption. In this thesis we have shown that massive particles and field that do not decouple during cosmological inflation will generate corrections, which lead to possibly observable features in the Cosmic Microwave Background. Furthermore, in specific setups where the massive particles and fields do decouple their stability can still be affected by the low energy physics energy scaleN...
A calculation of the one-mode occupation numbers for vacuum fluctuations of massive fields in De Sit...
© 2020 authors. Published by the American Physical Society. We demonstrate two properties of the tra...
In this thesis, I will present a method I developped to treat cosmological perturbations at linear o...
Cosmological inflation is the most successful theory that explains the homogeneity and flatness of t...
In the last twenty years, cosmology has become a precision science. Since the COBE era, a wealth of ...
Currently there is no definitive description for the accelerated expansion of the Universe at both e...
Phenomenologically, cosmic inflation is a satisfying and well-tested description of the physics of t...
The focus of the dissertation "Aspects of cosmic acceleration" is the study of possible mechanisms r...
In this thesis, we modify the standard single-field inflation scenario by adding additional massive ...
There is a reasonable amount of observational evidence that suggests space was expanding exponential...
In this thesis, we study the decoherence of cosmological scalar perturbations during inflation. We f...
ΛCDM cosmology is described in terms of general relativity and the Robertson-Walker metric. The evol...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2005.Includes bibliographica...
We study the decoherence of massive fields during inflation based on the Zurek’s density matrix appr...
The cosmological constant is not the only possibility in order to describe the accelerated expansion...
A calculation of the one-mode occupation numbers for vacuum fluctuations of massive fields in De Sit...
© 2020 authors. Published by the American Physical Society. We demonstrate two properties of the tra...
In this thesis, I will present a method I developped to treat cosmological perturbations at linear o...
Cosmological inflation is the most successful theory that explains the homogeneity and flatness of t...
In the last twenty years, cosmology has become a precision science. Since the COBE era, a wealth of ...
Currently there is no definitive description for the accelerated expansion of the Universe at both e...
Phenomenologically, cosmic inflation is a satisfying and well-tested description of the physics of t...
The focus of the dissertation "Aspects of cosmic acceleration" is the study of possible mechanisms r...
In this thesis, we modify the standard single-field inflation scenario by adding additional massive ...
There is a reasonable amount of observational evidence that suggests space was expanding exponential...
In this thesis, we study the decoherence of cosmological scalar perturbations during inflation. We f...
ΛCDM cosmology is described in terms of general relativity and the Robertson-Walker metric. The evol...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2005.Includes bibliographica...
We study the decoherence of massive fields during inflation based on the Zurek’s density matrix appr...
The cosmological constant is not the only possibility in order to describe the accelerated expansion...
A calculation of the one-mode occupation numbers for vacuum fluctuations of massive fields in De Sit...
© 2020 authors. Published by the American Physical Society. We demonstrate two properties of the tra...
In this thesis, I will present a method I developped to treat cosmological perturbations at linear o...