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Prompt atmospheric neutrino flux from the various QCD models
KISTI, Natl Inst Supercomp & Networking, Daejeon 34141, South Korea..
Univ Liege, Space Sci Technol & Astrophys Res STAR Inst, Bat B5a, B-4000 Liege, Belgium..
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, High Energy Physics.ORCID iD: 0000-0003-0452-0671
Yonsei Univ, Dept Phys, Seoul 03722, South Korea.;Yonsei Univ, IPAP, Seoul 03722, South Korea..
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2017 (English)In: XLVI International Symposium On Multiparticle Dynamics (ISMD 2016) / [ed] Yoo, I K, 2017, article id UNSP 07002Conference paper, Published paper (Refereed)
Abstract [en]

We 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.

Place, publisher, year, edition, pages
2017. article id UNSP 07002
Series
EPJ Web of Conferences, ISSN 2100-014X ; 141
National Category
Atom and Molecular Physics and Optics
Identifiers
URN: urn:nbn:se:uu:diva-335839DOI: 10.1051/epjconf/201714107002ISI: 000404462600046OAI: oai:DiVA.org:uu-335839DiVA, id: diva2:1166508
Conference
46th International Symposium on Multiparticle Dynamics (ISMD), AUG 29-SEP 02, 2016, SOUTH KOREA
Available from: 2017-12-15 Created: 2017-12-15 Last updated: 2017-12-15Bibliographically approved

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