We investigate the quantum fluctuations of an inflaton field in a two-field model of one-bubble open inflation. One of the inflatons is assumed to be responsible for the first false vacuum stage of inflation and the other is assumed to be responsible for the second slow-roll stage of inflation. The mass of the second inflaton is assumed to be negligible throughout the whole era of inflation. We find the super-curvature fluctuations are enhanced by the factor given by the ratio of the Hubble constants at false vacuum and true vacuum. This gives a strong constraint on a class of open inflation models. In particular, this implies the simplest two-field model proposed by Linde and Mezhlumian is in trouble
There are many inflationary models in which inflaton field does not satisfy the slow-roll condition....
textOne of the exciting aspects of cosmology is to understand the period of `cosmic inflation' that ...
We study a model of two-field ultra-slow-roll (USR) inflation bounded by a curve in the field space....
We show that a large class of two-field models of single-bubble open inflation do not lead to infini...
It appears difficult to construct a simple model for an open universe based on the one bubble inflat...
Inflation models are compared with observation on the assumption that the curvature perturbation is ...
Inflation is currently the most promising paradigm of the Early Universe. The simple paradigm involv...
We first develop a method to calculate a complete set of mode functions which describe the quantum f...
We investigate the parameter space of two-field inflation models where inflation terminates via a fi...
We explore the dynamics and observational predictions of the warm little inflaton scenario, presentl...
This is the author accpted manuscript. The final version is available from IOP Publishing via the DO...
We examine the dynamics of a closed cosmology whose matter source is that of a conformally coupled s...
The density fluctuations (both curvature and isocurvature) that arise due to quantum fluctuations in...
We discuss metric perturbations produced during a period of inflation in the early universe where tw...
According to the current experimental data, the Higgs vacuum appears to be metastable due to the dev...
There are many inflationary models in which inflaton field does not satisfy the slow-roll condition....
textOne of the exciting aspects of cosmology is to understand the period of `cosmic inflation' that ...
We study a model of two-field ultra-slow-roll (USR) inflation bounded by a curve in the field space....
We show that a large class of two-field models of single-bubble open inflation do not lead to infini...
It appears difficult to construct a simple model for an open universe based on the one bubble inflat...
Inflation models are compared with observation on the assumption that the curvature perturbation is ...
Inflation is currently the most promising paradigm of the Early Universe. The simple paradigm involv...
We first develop a method to calculate a complete set of mode functions which describe the quantum f...
We investigate the parameter space of two-field inflation models where inflation terminates via a fi...
We explore the dynamics and observational predictions of the warm little inflaton scenario, presentl...
This is the author accpted manuscript. The final version is available from IOP Publishing via the DO...
We examine the dynamics of a closed cosmology whose matter source is that of a conformally coupled s...
The density fluctuations (both curvature and isocurvature) that arise due to quantum fluctuations in...
We discuss metric perturbations produced during a period of inflation in the early universe where tw...
According to the current experimental data, the Higgs vacuum appears to be metastable due to the dev...
There are many inflationary models in which inflaton field does not satisfy the slow-roll condition....
textOne of the exciting aspects of cosmology is to understand the period of `cosmic inflation' that ...
We study a model of two-field ultra-slow-roll (USR) inflation bounded by a curve in the field space....