Large scale voids are a very prominent feature in recent redshift surveys: here we attempt an explanation in terms of a first order phase transition occurring during the slow roll epoch of a two field inflation. The ensuing bubble like perturbations -- nucleated at a number of e-folds Napprox 50 before reheating -- are thought to be the precursors of the voids we observe today. They pass the CMB constraints. Furthermore, the claim, in apparent conflict with inflation, that the Universe is open, may also be explained if we live in a superhorizon bubble nucleated around Napprox 60 and if the Universe itself be a collection of such bubbles. Our model predicts sharply peaked bubble spectra, e.g. at Omega0 ≅.2, so that our probability of living ...
The detection of a stochastic Gravitational Wave (GW) background sourced by a cosmological phase tra...
Quasi-conformal models are an appealing scenario that can offer naturally a strongly supercooled pha...
Strongly first-order phase transitions, i.e., those with a large order parameter, are characterized ...
We propose to explain the present large scale structure of the universe in terms of a first order ph...
Scale-invariant (flat) fluctuation spectra are the most generic outcomes of inflation. However, curr...
We propose a new inflationary toy model that produces two episodes of phase transitions. With the fi...
Restricted AccessScale-invariant (flat) fluctuation spectra are the most generic outcomes of inflati...
We show that a particular class of postrecombination phase transitions in the vacuum can lead to loc...
Motivated by recent observations suggesting that structures in the Universe appear to be concentrate...
We consider true vacuum bubbles generated in a first order phase transition occurring during the slo...
We review the observable effects produced by phase transitions occurring along with inflation. First...
It is already understood that the increasing observational evidence for an open universe can be reco...
One important prediction of a cosmological model based on grand unified theories is the production o...
Determining cosmological parameters from current observational data requires knowledge of the primor...
[[abstract]]Motivated by the discovery of a plenitude of metastable vacua in a string landscape and ...
The detection of a stochastic Gravitational Wave (GW) background sourced by a cosmological phase tra...
Quasi-conformal models are an appealing scenario that can offer naturally a strongly supercooled pha...
Strongly first-order phase transitions, i.e., those with a large order parameter, are characterized ...
We propose to explain the present large scale structure of the universe in terms of a first order ph...
Scale-invariant (flat) fluctuation spectra are the most generic outcomes of inflation. However, curr...
We propose a new inflationary toy model that produces two episodes of phase transitions. With the fi...
Restricted AccessScale-invariant (flat) fluctuation spectra are the most generic outcomes of inflati...
We show that a particular class of postrecombination phase transitions in the vacuum can lead to loc...
Motivated by recent observations suggesting that structures in the Universe appear to be concentrate...
We consider true vacuum bubbles generated in a first order phase transition occurring during the slo...
We review the observable effects produced by phase transitions occurring along with inflation. First...
It is already understood that the increasing observational evidence for an open universe can be reco...
One important prediction of a cosmological model based on grand unified theories is the production o...
Determining cosmological parameters from current observational data requires knowledge of the primor...
[[abstract]]Motivated by the discovery of a plenitude of metastable vacua in a string landscape and ...
The detection of a stochastic Gravitational Wave (GW) background sourced by a cosmological phase tra...
Quasi-conformal models are an appealing scenario that can offer naturally a strongly supercooled pha...
Strongly first-order phase transitions, i.e., those with a large order parameter, are characterized ...