Color evaporation induced rapidity gaps

Detalhes bibliográficos
Autor(a) principal: Éboli, O. J P [UNESP]
Data de Publicação: 2000
Outros Autores: Gregores, E. M. [UNESP], Halzen, F.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.61.034003
http://hdl.handle.net/11449/66097
Resumo: We show that soft color rearrangement of final states can account for the appearance of rapidity gaps between jets. In the color evaporation model the probability to form a gap is simply determined by the color multiplicity of the final state. This model has no free parameters and reproduces all data obtained by the ZEUS, H1, DØ, and CDF Collaborations. ©1999 The American Physical Society.
id UNSP_ea6c03bba5c54cd31ea1211935d8abdc
oai_identifier_str oai:repositorio.unesp.br:11449/66097
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling Color evaporation induced rapidity gapsWe show that soft color rearrangement of final states can account for the appearance of rapidity gaps between jets. In the color evaporation model the probability to form a gap is simply determined by the color multiplicity of the final state. This model has no free parameters and reproduces all data obtained by the ZEUS, H1, DØ, and CDF Collaborations. ©1999 The American Physical Society.Inst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900, São Paulo - SPDepartment of Physics University of Wisconsin, Madison, WI 53706Inst. de Fis. Teórica Universidade Estadual Paulista, Rua Pamplona 145, 01405-900, São Paulo - SPUniversidade Estadual Paulista (Unesp)University of WisconsinÉboli, O. J P [UNESP]Gregores, E. M. [UNESP]Halzen, F.2014-05-27T11:19:53Z2014-05-27T11:19:53Z2000-02-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1-9application/pdfhttp://dx.doi.org/10.1103/PhysRevD.61.034003Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 61, n. 3, p. 1-9, 2000.0556-2821http://hdl.handle.net/11449/6609710.1103/PhysRevD.61.034003WOS:0000850796000232-s2.0-181444174752-s2.0-18144417475.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D: Particles, Fields, Gravitation and Cosmologyinfo:eu-repo/semantics/openAccess2024-01-28T06:51:42Zoai:repositorio.unesp.br:11449/66097Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-01-28T06:51:42Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Color evaporation induced rapidity gaps
title Color evaporation induced rapidity gaps
spellingShingle Color evaporation induced rapidity gaps
Éboli, O. J P [UNESP]
title_short Color evaporation induced rapidity gaps
title_full Color evaporation induced rapidity gaps
title_fullStr Color evaporation induced rapidity gaps
title_full_unstemmed Color evaporation induced rapidity gaps
title_sort Color evaporation induced rapidity gaps
author Éboli, O. J P [UNESP]
author_facet Éboli, O. J P [UNESP]
Gregores, E. M. [UNESP]
Halzen, F.
author_role author
author2 Gregores, E. M. [UNESP]
Halzen, F.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
University of Wisconsin
dc.contributor.author.fl_str_mv Éboli, O. J P [UNESP]
Gregores, E. M. [UNESP]
Halzen, F.
description We show that soft color rearrangement of final states can account for the appearance of rapidity gaps between jets. In the color evaporation model the probability to form a gap is simply determined by the color multiplicity of the final state. This model has no free parameters and reproduces all data obtained by the ZEUS, H1, DØ, and CDF Collaborations. ©1999 The American Physical Society.
publishDate 2000
dc.date.none.fl_str_mv 2000-02-01
2014-05-27T11:19:53Z
2014-05-27T11:19:53Z
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.61.034003
Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 61, n. 3, p. 1-9, 2000.
0556-2821
http://hdl.handle.net/11449/66097
10.1103/PhysRevD.61.034003
WOS:000085079600023
2-s2.0-18144417475
2-s2.0-18144417475.pdf
url http://dx.doi.org/10.1103/PhysRevD.61.034003
http://hdl.handle.net/11449/66097
identifier_str_mv Physical Review D - Particles, Fields, Gravitation and Cosmology, v. 61, n. 3, p. 1-9, 2000.
0556-2821
10.1103/PhysRevD.61.034003
WOS:000085079600023
2-s2.0-18144417475
2-s2.0-18144417475.pdf
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 1-9
application/pdf
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_ 1797790423427579904

Registros relacionados