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dc.contributor.authorRothen, Lorena
dc.contributor.authorTackmann, Frank J.
dc.contributor.authorMoult, Ian James
dc.contributor.authorStewart, Iain W
dc.contributor.authorZhu, HuaXing
dc.date.accessioned2017-05-26T18:45:31Z
dc.date.available2017-05-26T18:45:31Z
dc.date.issued2017-04
dc.date.submitted2017-01
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttp://hdl.handle.net/1721.1/109386
dc.description.abstractThe N-jettiness observable T[subscript N] provides a way of describing the leading singular behavior of the N-jet cross section in the τ=T[subscript N]/Q→0 limit, where Q is a hard interaction scale. We consider subleading-power corrections in the τ≪1 expansion, and employ soft-collinear effective theory to obtain analytic results for the dominant α[subscript s]τlnτ and α[superscript 2][subscript s]τln[superscript 3]τ subleading terms for thrust in e[superscript +]e[superscript -] collisions and 0-jettiness for q[bar over q]-initiated Drell-Yan–like processes at hadron colliders. These results can be used to significantly improve the numerical accuracy and stability of the N-jettiness subtraction technique for performing fixed-order calculations at next-to-leading order and next-to-next-to-leading order. They reduce the size of missing power corrections in the subtractions by an order of magnitude. We also point out that the precise definition of N-jettiness has an important impact on the size of the power corrections and thus the numerical accuracy of the subtractions. The sometimes employed definition of N-jettiness in the hadronic center-of-mass frame suffers from power corrections that grow exponentially with rapidity, causing the power expansion to deteriorate away from central rapidity. This degradation does not occur for the original N-jettiness definition, which explicitly accounts for the boost of the Born process relative to the frame of the hadronic collision, and has a well-behaved power expansion throughout the entire phase space. Integrated over rapidity, using this N-jettiness definition in the subtractions yields another order of magnitude improvement compared to employing the hadronic-frame definition.en_US
dc.description.sponsorshipUnited States. Dept. of Energy. Office of Nuclear Physics (Contract DESC0011090)en_US
dc.description.sponsorshipUnited States. Dept. of Energy. Office of High Energy Physics (Contract DE-AC02-05CH11231)en_US
dc.description.sponsorshipLawrence Berkeley National Laboratoryen_US
dc.description.sponsorshipSimons Foundation (Investigator Grant 327942)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.95.074023en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleSubleading power corrections for N-jettiness subtractionsen_US
dc.typeArticleen_US
dc.identifier.citationMoult, Ian et al. “Subleading Power Corrections for N -Jettiness Subtractions.” Physical Review D 95.7 (2017): n. pag. © 2017 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Center for Theoretical Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.mitauthorMoult, Ian James
dc.contributor.mitauthorStewart, Iain W
dc.contributor.mitauthorZhu, HuaXing
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2017-04-18T22:00:05Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsMoult, Ian; Rothen, Lorena; Stewart, Iain W.; Tackmann, Frank J.; Zhu, Hua Xingen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-4819-4081
dc.identifier.orcidhttps://orcid.org/0000-0003-0248-0979
mit.licensePUBLISHER_POLICYen_US


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