Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models
- Autores
- Bengochea, Gabriel R.; León, Gabriel; Pearle, Philip; Sudarsky, Daniel
- Año de publicación
- 2020
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- 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.
Instituto de Astrofísica de La Plata - Materia
-
Ciencias Astronómicas
Continuous spontaneous localization
Quantum gravity
Cosmic inflation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by/4.0/
- Repositorio
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/124025
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Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization modelsBengochea, Gabriel R.León, GabrielPearle, PhilipSudarsky, DanielCiencias AstronómicasContinuous spontaneous localizationQuantum gravityCosmic inflationIn 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.Instituto de Astrofísica de La Plata2020-11-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/124025enginfo:eu-repo/semantics/altIdentifier/issn/1434-6044info:eu-repo/semantics/altIdentifier/issn/1434-6052info:eu-repo/semantics/altIdentifier/arxiv/2008.05285info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-020-08599-zinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-15T11:21:18Zoai:sedici.unlp.edu.ar:10915/124025Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-15 11:21:18.43SEDICI (UNLP) - Universidad Nacional de La Platafalse |
dc.title.none.fl_str_mv |
Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models |
title |
Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models |
spellingShingle |
Discussions about the landscape of possibilities for treatments of cosmic inflation involving continuous spontaneous localization models Bengochea, Gabriel R. Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation |
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 |
dc.creator.none.fl_str_mv |
Bengochea, Gabriel R. León, Gabriel Pearle, Philip Sudarsky, Daniel |
author |
Bengochea, Gabriel R. |
author_facet |
Bengochea, Gabriel R. León, Gabriel Pearle, Philip Sudarsky, Daniel |
author_role |
author |
author2 |
León, Gabriel Pearle, Philip Sudarsky, Daniel |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation |
topic |
Ciencias Astronómicas Continuous spontaneous localization Quantum gravity Cosmic inflation |
dc.description.none.fl_txt_mv |
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. Instituto de Astrofísica de La Plata |
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. |
publishDate |
2020 |
dc.date.none.fl_str_mv |
2020-11-04 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/124025 |
url |
http://sedici.unlp.edu.ar/handle/10915/124025 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
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info:eu-repo/semantics/altIdentifier/issn/1434-6044 info:eu-repo/semantics/altIdentifier/issn/1434-6052 info:eu-repo/semantics/altIdentifier/arxiv/2008.05285 info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-020-08599-z |
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info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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openAccess |
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http://creativecommons.org/licenses/by/4.0/ Creative Commons Attribution 4.0 International (CC BY 4.0) |
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