Quantum chameleons
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.99.104049 http://hdl.handle.net/11449/189186 |
Resumo: | We initiate a quantum treatment of chameleonlike particles, deriving classical and quantum forces directly from the path integral. It is found that the quantum force can potentially dominate the classical one by many orders of magnitude. We calculate the quantum chameleon pressure between infinite plates, which is found to interpolate between the Casimir and the integrated Casimir-Polder pressures, respectively in the limits of full screening and no screening. To this end we calculate the chameleon propagator in the presence of an arbitrary number of one-dimensional layers of material. For the Eöt-Wash experiment, the five-layer propagator is used to take into account the intermediate shielding sheet, and it is found that the presence of the sheet enhances the quantum pressure by two orders of magnitude. As an example of implication, we show that in both the standard chameleon and symmetron models, large and previously unconstrained regions of the parameter space are excluded once the quantum pressure is taken into account. |
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Quantum chameleonsWe initiate a quantum treatment of chameleonlike particles, deriving classical and quantum forces directly from the path integral. It is found that the quantum force can potentially dominate the classical one by many orders of magnitude. We calculate the quantum chameleon pressure between infinite plates, which is found to interpolate between the Casimir and the integrated Casimir-Polder pressures, respectively in the limits of full screening and no screening. To this end we calculate the chameleon propagator in the presence of an arbitrary number of one-dimensional layers of material. For the Eöt-Wash experiment, the five-layer propagator is used to take into account the intermediate shielding sheet, and it is found that the presence of the sheet enhances the quantum pressure by two orders of magnitude. As an example of implication, we show that in both the standard chameleon and symmetron models, large and previously unconstrained regions of the parameter space are excluded once the quantum pressure is taken into account.Institut de Physique Théorique Université Paris-Saclay CEA CNRSWalter Burke Institute for Theoretical Physics California Institute of TechnologyICTP-SAIFR and IFT-UNESP, Rua Dr. Bento Teobaldo Ferraz 271ICTP-SAIFR and IFT-UNESP, Rua Dr. Bento Teobaldo Ferraz 271CNRSCalifornia Institute of TechnologyUniversidade Estadual Paulista (Unesp)Brax, PhilippeFichet, Sylvain [UNESP]2019-10-06T16:32:40Z2019-10-06T16:32:40Z2019-05-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.99.104049Physical Review D, v. 99, n. 10, 2019.2470-00292470-0010http://hdl.handle.net/11449/18918610.1103/PhysRevD.99.1040492-s2.0-85066445114Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2021-10-23T14:54:40Zoai:repositorio.unesp.br:11449/189186Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T15:01:13.195685Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Quantum chameleons |
title |
Quantum chameleons |
spellingShingle |
Quantum chameleons Brax, Philippe |
title_short |
Quantum chameleons |
title_full |
Quantum chameleons |
title_fullStr |
Quantum chameleons |
title_full_unstemmed |
Quantum chameleons |
title_sort |
Quantum chameleons |
author |
Brax, Philippe |
author_facet |
Brax, Philippe Fichet, Sylvain [UNESP] |
author_role |
author |
author2 |
Fichet, Sylvain [UNESP] |
author2_role |
author |
dc.contributor.none.fl_str_mv |
CNRS California Institute of Technology Universidade Estadual Paulista (Unesp) |
dc.contributor.author.fl_str_mv |
Brax, Philippe Fichet, Sylvain [UNESP] |
description |
We initiate a quantum treatment of chameleonlike particles, deriving classical and quantum forces directly from the path integral. It is found that the quantum force can potentially dominate the classical one by many orders of magnitude. We calculate the quantum chameleon pressure between infinite plates, which is found to interpolate between the Casimir and the integrated Casimir-Polder pressures, respectively in the limits of full screening and no screening. To this end we calculate the chameleon propagator in the presence of an arbitrary number of one-dimensional layers of material. For the Eöt-Wash experiment, the five-layer propagator is used to take into account the intermediate shielding sheet, and it is found that the presence of the sheet enhances the quantum pressure by two orders of magnitude. As an example of implication, we show that in both the standard chameleon and symmetron models, large and previously unconstrained regions of the parameter space are excluded once the quantum pressure is taken into account. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-10-06T16:32:40Z 2019-10-06T16:32:40Z 2019-05-15 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.99.104049 Physical Review D, v. 99, n. 10, 2019. 2470-0029 2470-0010 http://hdl.handle.net/11449/189186 10.1103/PhysRevD.99.104049 2-s2.0-85066445114 |
url |
http://dx.doi.org/10.1103/PhysRevD.99.104049 http://hdl.handle.net/11449/189186 |
identifier_str_mv |
Physical Review D, v. 99, n. 10, 2019. 2470-0029 2470-0010 10.1103/PhysRevD.99.104049 2-s2.0-85066445114 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808128447636045824 |