Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases
Autor(a) principal: | |
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Data de Publicação: | 2008 |
Outros Autores: | , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.78.065046 http://hdl.handle.net/11449/225301 |
Resumo: | The thermodynamics of a scalar field with a quartic interaction is studied within the linear δ expansion (LDE) method. Using the imaginary-time formalism the free energy is evaluated up to second order in the LDE. The method generates nonperturbative results that are then used to obtain thermodynamic quantities like the pressure. The phase transition pattern of the model is fully studied, from the broken to the symmetry restored phase. The results are compared with those obtained with other nonperturbative methods and also with ordinary perturbation theory. The results coming from the two main optimization procedures used in conjunction with the LDE method, the principle of minimal sensitivity (PMS) and the fastest apparent convergence (FAC) are also compared with each other and studied in which cases they are applicable or not. The optimization procedures are applied directly to the free energy. © 2008 The American Physical Society. |
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Repositório Institucional da UNESP |
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Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phasesThe thermodynamics of a scalar field with a quartic interaction is studied within the linear δ expansion (LDE) method. Using the imaginary-time formalism the free energy is evaluated up to second order in the LDE. The method generates nonperturbative results that are then used to obtain thermodynamic quantities like the pressure. The phase transition pattern of the model is fully studied, from the broken to the symmetry restored phase. The results are compared with those obtained with other nonperturbative methods and also with ordinary perturbation theory. The results coming from the two main optimization procedures used in conjunction with the LDE method, the principle of minimal sensitivity (PMS) and the fastest apparent convergence (FAC) are also compared with each other and studied in which cases they are applicable or not. The optimization procedures are applied directly to the free energy. © 2008 The American Physical Society.Departamento de Física Teórica Universidade Do Estado Do Rio de Janeiro, 20550-013 Rio de Janeiro, RJInstituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo, SPInstituto de Física Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900 São Paulo, SPUniversidade do Estado do Rio de Janeiro (UERJ)Universidade Estadual Paulista (UNESP)Farias, R. L.S.Krein, G. [UNESP]Ramos, Rudnei O.2022-04-28T20:44:14Z2022-04-28T20:44:14Z2008-09-29info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1103/PhysRevD.78.065046Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 78, n. 6, 2008.1550-79981550-2368http://hdl.handle.net/11449/22530110.1103/PhysRevD.78.0650462-s2.0-53549110504Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-28T20:44:14Zoai:repositorio.unesp.br:11449/225301Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T22:40:10.899215Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
title |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
spellingShingle |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases Farias, R. L.S. |
title_short |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
title_full |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
title_fullStr |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
title_full_unstemmed |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
title_sort |
Applicability of the linear δ expansion for the λ 4 field theory at finite temperature in the symmetric and broken phases |
author |
Farias, R. L.S. |
author_facet |
Farias, R. L.S. Krein, G. [UNESP] Ramos, Rudnei O. |
author_role |
author |
author2 |
Krein, G. [UNESP] Ramos, Rudnei O. |
author2_role |
author author |
dc.contributor.none.fl_str_mv |
Universidade do Estado do Rio de Janeiro (UERJ) Universidade Estadual Paulista (UNESP) |
dc.contributor.author.fl_str_mv |
Farias, R. L.S. Krein, G. [UNESP] Ramos, Rudnei O. |
description |
The thermodynamics of a scalar field with a quartic interaction is studied within the linear δ expansion (LDE) method. Using the imaginary-time formalism the free energy is evaluated up to second order in the LDE. The method generates nonperturbative results that are then used to obtain thermodynamic quantities like the pressure. The phase transition pattern of the model is fully studied, from the broken to the symmetry restored phase. The results are compared with those obtained with other nonperturbative methods and also with ordinary perturbation theory. The results coming from the two main optimization procedures used in conjunction with the LDE method, the principle of minimal sensitivity (PMS) and the fastest apparent convergence (FAC) are also compared with each other and studied in which cases they are applicable or not. The optimization procedures are applied directly to the free energy. © 2008 The American Physical Society. |
publishDate |
2008 |
dc.date.none.fl_str_mv |
2008-09-29 2022-04-28T20:44:14Z 2022-04-28T20:44:14Z |
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.78.065046 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 78, n. 6, 2008. 1550-7998 1550-2368 http://hdl.handle.net/11449/225301 10.1103/PhysRevD.78.065046 2-s2.0-53549110504 |
url |
http://dx.doi.org/10.1103/PhysRevD.78.065046 http://hdl.handle.net/11449/225301 |
identifier_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 78, n. 6, 2008. 1550-7998 1550-2368 10.1103/PhysRevD.78.065046 2-s2.0-53549110504 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology |
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_ |
1808129448744058880 |