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dc.date.accessioned2021-01-18T20:46:08Z
dc.date.available2021-01-18T20:46:08Z
dc.date.created2021-01-11T13:51:23Z
dc.date.issued2020
dc.identifier.citationPlestid, Ryan Takhistov, Volodomyr Tsai, Yu-Dai Bringmann, Torsten Kusenko, Alexander Pospelov, Maxim . New Constraints on Millicharged Particles from Cosmic-ray Production. Physical Review D. Particles and fields. 2020
dc.identifier.urihttp://hdl.handle.net/10852/82334
dc.description.abstractWe study cosmic-ray-atmosphere collisions as a permanent production source of exotic millicharged particles (MCPs) for all terrestrial experiments. [MCPs are also known as charged massive particles (CHAMPs).] Based on data from Super-K, this allows us to derive new limits on MCPs that are competitive with, or improve, the currently leading bounds from accelerator-based searches for masses up to 1.5 GeV. In models where a subdominant component of dark matter (DM) is fractionally charged, these constraints probe parts of the parameter space that is inaccessible for conventional direct-detection DM experiments, independently of assumptions about the DM abundance.
dc.languageEN
dc.publisherAmerican Physical Society
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleNew Constraints on Millicharged Particles from Cosmic-ray Production
dc.typeJournal article
dc.creator.authorPlestid, Ryan
dc.creator.authorTakhistov, Volodomyr
dc.creator.authorTsai, Yu-Dai
dc.creator.authorBringmann, Torsten
dc.creator.authorKusenko, Alexander
dc.creator.authorPospelov, Maxim
cristin.unitcode185,15,4,80
cristin.unitnameTeoretisk fysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode0
dc.identifier.cristin1869036
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review D. Particles and fields&rft.volume=&rft.spage=&rft.date=2020
dc.identifier.jtitlePhysical Review D. Particles and fields
dc.identifier.volume102
dc.identifier.issue11
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.102.115032
dc.identifier.urnURN:NBN:no-85218
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0556-2821
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/82334/2/scoap3-fulltext.pdf
dc.type.versionPublishedVersion
cristin.articleid115032


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