Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED
Autor(a) principal: | |
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Data de Publicação: | 2005 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.72.045009 http://hdl.handle.net/11449/231022 |
Resumo: | We perform a very detailed investigation into the possibility of Lorentz and CPT violations in the photon sector, of the Chern-Simons form, being induced by radiative corrections arising from the Lorentz and CPT noninvariant fermionic sector of an extended version of QED. In the discussions it is considered the role played by the scale ambiguities in the perturbative calculations. The origin of the possible contributions are clearly identified, due to the very general character of the calculational method applied, concerning the manipulations and calculations of divergent amplitudes. We show that constraints dictated by the consistency in the perturbative calculations, imposed by physical reasons, eliminate all the sources of violating contributions, leaving no room for the existence of a radiatively induced Lorentz and CPT violations in the extended QED, putting the perturbative evaluations in accordance with the predictions made, by using very general arguments, stated by other authors. © 2005 The American Physical Society. |
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Repositório Institucional da UNESP |
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Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QEDWe perform a very detailed investigation into the possibility of Lorentz and CPT violations in the photon sector, of the Chern-Simons form, being induced by radiative corrections arising from the Lorentz and CPT noninvariant fermionic sector of an extended version of QED. In the discussions it is considered the role played by the scale ambiguities in the perturbative calculations. The origin of the possible contributions are clearly identified, due to the very general character of the calculational method applied, concerning the manipulations and calculations of divergent amplitudes. We show that constraints dictated by the consistency in the perturbative calculations, imposed by physical reasons, eliminate all the sources of violating contributions, leaving no room for the existence of a radiatively induced Lorentz and CPT violations in the extended QED, putting the perturbative evaluations in accordance with the predictions made, by using very general arguments, stated by other authors. © 2005 The American Physical Society.Departamento de Física Universidade Federal de Santa Maria, C.x. Postal 5043, 97119-900, Santa Maria, RSInstituto de Física Teórica, Rua Pamplona, 145, 01405-900 - São Paulo, SPUniversidade Federal de Santa MariaInstituto de Física TeóricaBattistel, O. A.Dallabona, G.2022-04-29T08:43:16Z2022-04-29T08:43:16Z2005-08-15info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1-16http://dx.doi.org/10.1103/PhysRevD.72.045009Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 72, n. 4, p. 1-16, 2005.1550-79981550-2368http://hdl.handle.net/11449/23102210.1103/PhysRevD.72.0450092-s2.0-33749158415Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D - Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2022-04-29T08:43:16Zoai:repositorio.unesp.br:11449/231022Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:34:32.432808Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
title |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
spellingShingle |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED Battistel, O. A. |
title_short |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
title_full |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
title_fullStr |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
title_full_unstemmed |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
title_sort |
Scale ambiguities in perturbative calculations and the value for the radiatively induced Chern-Simons term in extended QED |
author |
Battistel, O. A. |
author_facet |
Battistel, O. A. Dallabona, G. |
author_role |
author |
author2 |
Dallabona, G. |
author2_role |
author |
dc.contributor.none.fl_str_mv |
Universidade Federal de Santa Maria Instituto de Física Teórica |
dc.contributor.author.fl_str_mv |
Battistel, O. A. Dallabona, G. |
description |
We perform a very detailed investigation into the possibility of Lorentz and CPT violations in the photon sector, of the Chern-Simons form, being induced by radiative corrections arising from the Lorentz and CPT noninvariant fermionic sector of an extended version of QED. In the discussions it is considered the role played by the scale ambiguities in the perturbative calculations. The origin of the possible contributions are clearly identified, due to the very general character of the calculational method applied, concerning the manipulations and calculations of divergent amplitudes. We show that constraints dictated by the consistency in the perturbative calculations, imposed by physical reasons, eliminate all the sources of violating contributions, leaving no room for the existence of a radiatively induced Lorentz and CPT violations in the extended QED, putting the perturbative evaluations in accordance with the predictions made, by using very general arguments, stated by other authors. © 2005 The American Physical Society. |
publishDate |
2005 |
dc.date.none.fl_str_mv |
2005-08-15 2022-04-29T08:43:16Z 2022-04-29T08:43:16Z |
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.72.045009 Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 72, n. 4, p. 1-16, 2005. 1550-7998 1550-2368 http://hdl.handle.net/11449/231022 10.1103/PhysRevD.72.045009 2-s2.0-33749158415 |
url |
http://dx.doi.org/10.1103/PhysRevD.72.045009 http://hdl.handle.net/11449/231022 |
identifier_str_mv |
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 72, n. 4, p. 1-16, 2005. 1550-7998 1550-2368 10.1103/PhysRevD.72.045009 2-s2.0-33749158415 |
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.format.none.fl_str_mv |
1-16 |
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_ |
1808129221926584320 |