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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24034
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dc.contributor.authorNaculich, Stephen G.-
dc.contributor.authorNastase, Horatiu-
dc.contributor.authorSchnitzer, Howard J.-
dc.date.accessioned2014-05-20T14:08:39Z-
dc.date.accessioned2016-10-25T17:14:39Z-
dc.date.available2014-05-20T14:08:39Z-
dc.date.available2016-10-25T17:14:39Z-
dc.date.issued2012-01-01-
dc.identifierhttp://dx.doi.org/10.1007/JHEP01(2012)041-
dc.identifier.citationJournal of High Energy Physics. New York: Springer, n. 1, p. 21, 2012.-
dc.identifier.issn1126-6708-
dc.identifier.urihttp://hdl.handle.net/11449/24034-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24034-
dc.description.abstractThe IR divergences of supergravity amplitudes are less severe than those of planar SYM amplitudes, and are comparable to those subleading-color SYM amplitudes that are most subleading in the 1/N expansion, namely O(1/epsilon(L)) for L-loop amplitudes. We derive linear relations between one-and two-loop four-point amplitudes and one-loop five-point amplitudes of N = 4, 5, and 6 supergravity and the most-subleading-color contributions of the analogous amplitudes of N = 0, 1, and 2 SYM theory, extending earlier results for N = 8 supergravity amplitudes. Our work relies on linear relations between N >= 4 supergravity and planar SYM amplitudes that were recently derived using the double-copy property of gravity, and color-kinematic duality of gauge theories.en
dc.description.sponsorshipNSF-
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
dc.description.sponsorshipSBF-
dc.description.sponsorshipDOE-
dc.format.extent21-
dc.language.isoeng-
dc.publisherSpringer-
dc.sourceWeb of Science-
dc.subjectSupersymmetric gauge theoryen
dc.subjectExtended Supersymmetryen
dc.subject1/N Expansionen
dc.subjectSupergravity Modelsen
dc.titleLinear relations between N >= 4 supergravity and subleading-color SYM 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.affiliationUniv Estadual Paulista, UNESP, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.description.affiliationBrandeis Univ, Martin Fisher Sch Phys, Theoret Phys Grp, Waltham, MA 02454 USA-
dc.description.affiliationUnespUniv Estadual Paulista, UNESP, Inst Fis Teor, BR-01140070 São Paulo, Brazil-
dc.description.sponsorshipIdNSF: PHY10-67961-
dc.description.sponsorshipIdCNPq: 301219/2010-9-
dc.description.sponsorshipIdDOE: DE-FG02-92ER40706-
dc.identifier.doi10.1007/JHEP01(2012)041-
dc.identifier.wosWOS:000300181800041-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofJournal of High Energy Physics-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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