The Continuous Spontaneous Localization (CSL) model has been proposed as apossible solution to the quantum measurement problem by modifying theSchr"{o}dinger equation. In this work, we apply the CSL model to twocosmological models of the early Universe: the matter bounce scenario and slowroll inflation. In particular, we focus on the generation of the classicalprimordial inhomogeneities and anisotropies that arise from the dynamicalevolution, provided by the CSL mechanism, of the quantum state associated tothe quantum fields. In each case, we obtained a prediction for the shape andthe parameters characterizing the primordial spectra (scalar and tensor), i.e.the amplitude, the spectral index and the tensor-to-scalar ratio. We found thatthere...
Models of spontaneous wave function collapse modify the linear Schroedinger equation of standard qua...
Abstract The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject...
Attempts to apply quantum collapse theories to Cosmology and cosmic inflation are reviewed. These at...
The Continuous Spontaneous Localization (CSL) model has been proposed as apossible solution to the q...
The inflationary paradigm is the most successful model that explains the observed spectrum of primor...
We propose a novel realization for the natural extrapolation of the continuous spontaneous localizat...
In this work we analyze how the spectrum of primordial scalar perturbations is modified, within the ...
In this work we consider a wide variety of alternatives opened when applying the continuous spontane...
4siCollapse models describe phenomenologically the quantum-to-classical transition by adding suitabl...
The Continuous Spontaneous Localisation (CSL) model solves the measurement problem of standard quant...
We consider the eternal inflation scenario of the slow-roll/chaotic type with the additional element...
The hypothesis of the self-induced collapse of the inflaton wave function was introduced as a candid...
The perturbations in the early universe are generated as a result of the interplay between quantum f...
Models of spontaneous wave function collapse modify the linear Schroedinger equation of standard qua...
Abstract The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject...
Attempts to apply quantum collapse theories to Cosmology and cosmic inflation are reviewed. These at...
The Continuous Spontaneous Localization (CSL) model has been proposed as apossible solution to the q...
The inflationary paradigm is the most successful model that explains the observed spectrum of primor...
We propose a novel realization for the natural extrapolation of the continuous spontaneous localizat...
In this work we analyze how the spectrum of primordial scalar perturbations is modified, within the ...
In this work we consider a wide variety of alternatives opened when applying the continuous spontane...
4siCollapse models describe phenomenologically the quantum-to-classical transition by adding suitabl...
The Continuous Spontaneous Localisation (CSL) model solves the measurement problem of standard quant...
We consider the eternal inflation scenario of the slow-roll/chaotic type with the additional element...
The hypothesis of the self-induced collapse of the inflaton wave function was introduced as a candid...
The perturbations in the early universe are generated as a result of the interplay between quantum f...
Models of spontaneous wave function collapse modify the linear Schroedinger equation of standard qua...
Abstract The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject...
Attempts to apply quantum collapse theories to Cosmology and cosmic inflation are reviewed. These at...