You are in the accessibility menu

Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/113044
Full metadata record
DC FieldValueLanguage
dc.contributor.authorNaculich, Stephen G.-
dc.contributor.authorNastase, Horatiu-
dc.contributor.authorSchnitzer, Howard J.-
dc.date.accessioned2014-12-03T13:11:22Z-
dc.date.accessioned2016-10-25T20:13:58Z-
dc.date.available2014-12-03T13:11:22Z-
dc.date.available2016-10-25T20:13:58Z-
dc.date.issued2013-04-01-
dc.identifierhttp://dx.doi.org/10.1007/JHEP04(2013)114-
dc.identifier.citationJournal Of High Energy Physics. New York: Springer, n. 4, 23 p., 2013.-
dc.identifier.issn1029-8479-
dc.identifier.urihttp://hdl.handle.net/11449/113044-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/113044-
dc.description.abstractThe infrared singularities of gravitational amplitudes are one-loop exact, in that higher-loop divergences are characterized by the exponential of the one-loop divergence. We show that the contributions to SU(N) gauge-theory amplitudes that are most-subleading in the 1/N expansion are also one-loop exact, provided that the dipole conjecture holds. Possible corrections to the dipole conjecture, beginning at three loops, could violate one-loop-exactness, though would still maintain the absence of collinear divergences. We also demonstrate a relation between L-loop four-point N = 8 supergravity and most-subleading-color N = 4 SYM amplitudes that holds for the two leading IR divergences, O(1/epsilon(L)) and O(1/epsilon(L-1)), but breaks down at O(1/epsilon(L-2)).en
dc.description.sponsorshipNSF-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.description.sponsorshipDOE-
dc.format.extent23-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.subjectSupersymmetric gauge theoryen
dc.subjectScattering Amplitudesen
dc.subjectModels of Quantum Gravityen
dc.subject1/N Expansionen
dc.titleAll-loop infrared-divergent behavior of most-subleading-color gauge-theory amplitudesen
dc.typeoutro-
dc.contributor.institutionBowdoin Coll-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionBrandeis Univ-
dc.description.affiliationBowdoin Coll, Dept Phys, Brunswick, ME 04011 USA-
dc.description.affiliationUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.description.affiliationBrandeis Univ, Martin Fisher Sch Phys, Theoret Phys Grp, Waltham, MA 02454 USA-
dc.description.affiliationUnespUNESP Univ Estadual Paulista, Inst Fis Teor, BR-01140070 Sao Paulo, Brazil-
dc.description.sponsorshipIdNSFPHY10-67961-
dc.description.sponsorshipIdCNPq: 301219/2010-9-
dc.description.sponsorshipIdDOEDE-FG02-92ER40706-
dc.identifier.doi10.1007/JHEP04(2013)114-
dc.identifier.wosWOS:000321208800029-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofJournal of High Energy Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

There are no files associated with this item.
 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.