International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject to uncertainties related to the choice of the collapse operator. In this paper, we constrain its form based on generic arguments. We show that, if the collapse operator is even in the field variables, it is unable to induce the collapse of the wavefunction. Instead, if it is odd, we find that only linear operators are such that the outcomes are distributed according to Gaussian statistics, as required by measurements of the cosmic microwave background. We discuss implications of these results for previously proposed collapse operators. We conclude that the cosmological CSL collapse operator should be linear in the field variable...
In this work we consider a wide variety of alternatives opened when applying the continuous spontane...
International audienceThe Continuous Spontaneous Localisation (CSL) model solves the measurement pro...
International audienceAttempts to apply quantum collapse theories to Cosmology and cosmic inflation ...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
Abstract The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject to uncer...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
Collapse models describe phenomenologically the quantum-to-classical transition by adding suitable n...
Models of dynamical wave function collapse consistently describe the breakdown of the quantum superp...
Models of spontaneous wave function collapse modify the linear Schroedinger equation of standard qua...
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...
In this work we consider a wide variety of alternatives opened when applying the continuous spontane...
International audienceThe Continuous Spontaneous Localisation (CSL) model solves the measurement pro...
International audienceAttempts to apply quantum collapse theories to Cosmology and cosmic inflation ...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
Abstract The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
The Continuous Spontaneous Localisation (CSL) theory in the cosmological context is subject to uncer...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
International audienceThe Continuous Spontaneous Localisation (CSL) theory in the cosmological conte...
Collapse models describe phenomenologically the quantum-to-classical transition by adding suitable n...
Models of dynamical wave function collapse consistently describe the breakdown of the quantum superp...
Models of spontaneous wave function collapse modify the linear Schroedinger equation of standard qua...
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...
In this work we consider a wide variety of alternatives opened when applying the continuous spontane...
International audienceThe Continuous Spontaneous Localisation (CSL) model solves the measurement pro...
International audienceAttempts to apply quantum collapse theories to Cosmology and cosmic inflation ...