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dc.contributor.authorOvanesyan, Grigory
dc.contributor.authorRodd, Nicholas Llewellyn
dc.contributor.authorSlatyer, Tracy Robyn
dc.contributor.authorStewart, Iain W
dc.date.accessioned2017-03-07T17:15:10Z
dc.date.available2017-03-07T17:15:10Z
dc.date.issued2017-03
dc.date.submitted2016-12
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttp://hdl.handle.net/1721.1/107216
dc.description.abstractWe calculate the one-loop corrections to TeV-scale dark matter annihilation in a model where the dark matter is described by an SU(2)[subscript L] triplet of Majorana fermions, such as the wino. We use this framework to determine the high- and low-scale [bar over MS] matching coefficients at both the dark matter and weak boson mass scales at one loop. Part of this calculation has previously been performed in the literature numerically; we find our analytic result differs from the earlier work and discuss potential origins of this disagreement. Our result is used to extend the dark matter annihilation rate to next-to-leading logarithmic+O(α[subscript 2]) corrections (NLL[subscript ′]), which enables a precise determination of indirect detection signatures in present and upcoming experiments.en_US
dc.description.sponsorshipUnited States. Dept. of Energy (Grants DE-SC00012567, DE-SC0013999, and DE-SC0011090)en_US
dc.description.sponsorshipSimons Foundation (Investigator Grant 327942)en_US
dc.description.sponsorshipAmerican Australian Association (U.S.) (ConocoPhillips Fellowship)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.95.055001en_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.titleOne-loop correction to heavy dark matter annihilationen_US
dc.typeArticleen_US
dc.identifier.citationOvanesyan, Grigory et al. “One-Loop Correction to Heavy Dark Matter Annihilation.” Physical Review D 95.5 (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.mitauthorRodd, Nicholas Llewellyn
dc.contributor.mitauthorSlatyer, Tracy Robyn
dc.contributor.mitauthorStewart, Iain W
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.updated2017-03-03T23:00:06Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsOvanesyan, Grigory; Rodd, Nicholas L.; Slatyer, Tracy R.; Stewart, Iain W.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-3472-7606
dc.identifier.orcidhttps://orcid.org/0000-0001-9699-9047
dc.identifier.orcidhttps://orcid.org/0000-0003-0248-0979
mit.licensePUBLISHER_POLICYen_US


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