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dc.contributor.authorJeong, Yu Seon
dc.contributor.authorBhattacharya, Atri
dc.contributor.authorEnberg, Rikard
dc.contributor.authorKim, C. S.
dc.contributor.authorReno, Mary Hall
dc.contributor.authorSarcevic, Ina
dc.contributor.authorStasto, Anna
dc.date.accessioned2017-08-01T23:07:37Z
dc.date.available2017-08-01T23:07:37Z
dc.date.issued2017-04-12
dc.identifier.citationPrompt atmospheric neutrino flux from the various QCD models 2017, 141:07002 EPJ Web of Conferencesen
dc.identifier.issn2100-014X
dc.identifier.doi10.1051/epjconf/201714107002
dc.identifier.urihttp://hdl.handle.net/10150/625070
dc.description.abstractWe evaluate the prompt atmospheric neutrino flux using the different QCD models for heavy quark production including the b quark contribution. We include the nuclear correction and find it reduces the fluxes by 10% - 50% according to the models. Our heavy quark results are compared with experimental data from RHIC, LHC and LHCb.
dc.description.sponsorshipUS DOE; NRF of Korea; NSC of Poland; SRC of Sweden; FNRS of Belgiumen
dc.language.isoenen
dc.publisherE D P SCIENCESen
dc.relation.urlhttp://www.epj-conferences.org/10.1051/epjconf/201714107002en
dc.rights© The Authors, published by EDP Sciences, 2017. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0.en
dc.titlePrompt atmospheric neutrino flux from the various QCD modelsen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Dept Astronen
dc.identifier.journalEPJ Web of Conferences: XLVI INTERNATIONAL SYMPOSIUM ON MULTIPARTICLE DYNAMICS (ISMD 2016)en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
refterms.dateFOA2018-06-24T17:03:24Z
html.description.abstractWe evaluate the prompt atmospheric neutrino flux using the different QCD models for heavy quark production including the b quark contribution. We include the nuclear correction and find it reduces the fluxes by 10% - 50% according to the models. Our heavy quark results are compared with experimental data from RHIC, LHC and LHCb.


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