Add to ORKGThe current status of early universe cosmology can be summarized as precision, but inherently limited, data requiring explanation from precision and robust theory. Specifically inflation is presently the single concrete hope for solving the early universe problem, since it is generically realizable in quantum field theory, but treatment of interactions needs considerable attention. This talk reviews the importance and progress in this direction
In this thesis, we study the decoherence of cosmological scalar perturbations during inflation. We f...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
An analysis of the decoherence of quantum fluctuations shows that production of classical adiabatic ...
A brief review of the modern state of quantum cosmology is presented as a theory of quantum initial ...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
Contents: Introduction. The Present State of the Universe. What Can We Expect From a Complete Cosmol...
For simple inflationary models, we provide a consistent and complete scheme by which the macro-physi...
A dissipative mechanism is presented, which emerges in generic interacting quantum field systems and...
The first aim of this lecture is to highlight two areas of recent progress in inflationary cosmology...
A quantum field theory warm inflation model is presented that solves the cosmological horizon/flatne...
The hypothesis that the Universe underwent a period of exponential expansion at very early times has...
We give a brief overview of the role of quantum theory in cosmology, reviewing the standard model of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
In this thesis, we study the decoherence of cosmological scalar perturbations during inflation. We f...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
An analysis of the decoherence of quantum fluctuations shows that production of classical adiabatic ...
A brief review of the modern state of quantum cosmology is presented as a theory of quantum initial ...
Warm inflation presents an exceptional description of the early universe cosmology. It is a scenari...
Contents: Introduction. The Present State of the Universe. What Can We Expect From a Complete Cosmol...
For simple inflationary models, we provide a consistent and complete scheme by which the macro-physi...
A dissipative mechanism is presented, which emerges in generic interacting quantum field systems and...
The first aim of this lecture is to highlight two areas of recent progress in inflationary cosmology...
A quantum field theory warm inflation model is presented that solves the cosmological horizon/flatne...
The hypothesis that the Universe underwent a period of exponential expansion at very early times has...
We give a brief overview of the role of quantum theory in cosmology, reviewing the standard model of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
In this thesis, we study the decoherence of cosmological scalar perturbations during inflation. We f...
This thesis develops the implementation of Open Effective Field Theories in primordial cosmology. Of...
An analysis of the decoherence of quantum fluctuations shows that production of classical adiabatic ...