Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models

In this work we consider a wide variety of alternatives opened when applying the continuous spontaneous localization (CSL) dynamical collapse theory to the inflationary era. The definitive resolution of many of the issues discussed here will have to await, not only for a general relativistic CSL the...

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Detalles Bibliográficos
Autores principales:	Bengochea, Gabriel R., León, Gabriel, Pearle, Philip, Sudarsky, Daniel
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2020
Materias:	Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/124025
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-124025
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation
spellingShingle	Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation Bengochea, Gabriel R. León, Gabriel Pearle, Philip Sudarsky, Daniel Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
topic_facet	Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation
description	In this work we consider a wide variety of alternatives opened when applying the continuous spontaneous localization (CSL) dynamical collapse theory to the inflationary era. The definitive resolution of many of the issues discussed here will have to await, not only for a general relativistic CSL theory, but for a fully workable theory of quantum gravity. Our concern here is to explore these issues, and to warn against premature conclusions. This exploration includes: two different approaches to deal with quantum field theory and gravitation, the identification of the collapse-generating operator and the general nature and values of the parameters of the CSL theory. All the choices connected with these issues have the potential to dramatically alter the conclusions one can draw. We also argue that the incompatibilities found in a recent paper, between the CSL parameter values and the CMB observational data, are associated with specific choices made for the extrapolation to the cosmological context of the CSL theory (as it is known to work in non-relativistic laboratory situations) which do not represent the most natural ones.
format	Articulo Articulo
author	Bengochea, Gabriel R. León, Gabriel Pearle, Philip Sudarsky, Daniel
author_facet	Bengochea, Gabriel R. León, Gabriel Pearle, Philip Sudarsky, Daniel
author_sort	Bengochea, Gabriel R.
title	Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
title_short	Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
title_full	Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
title_fullStr	Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
title_full_unstemmed	Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
title_sort	discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
publishDate	2020
url	http://sedici.unlp.edu.ar/handle/10915/124025
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Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models

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