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Prompt neutrino fluxes from atmospheric charm
Department of Physics, University of Arizona.
Department of Physics and Astronomy, University of Iowa.
Department of Physics, University of Arizona.
2008 (English)In: Physical Review D, ISSN 1550-7998, E-ISSN 1550-2368, Vol. 78, no 4, 043005- p.Article in journal (Refereed) Published
Abstract [en]

We calculate the prompt neutrino flux from atmospheric charm production by cosmic rays, using the dipole picture in a perturbative QCD framework, which incorporates the parton saturation effects present at high energies. We compare our results with the next-to-leading order perturbative QCD result and find that saturation effects are large for neutrino energies above 10^6 GeV, leading to a substantial suppression of the prompt neutrino flux. We comment on the range of prompt neutrino fluxes due to theoretical uncertainties.

Place, publisher, year, edition, pages
2008. Vol. 78, no 4, 043005- p.
National Category
Subatomic Physics
Research subject
Physics with specialization in Elementary Particle Physics
Identifiers
URN: urn:nbn:se:uu:diva-162512DOI: 10.1103/PhysRevD.78.043005OAI: oai:DiVA.org:uu-162512DiVA: diva2:460606
Available from: 2011-12-01 Created: 2011-11-30 Last updated: 2017-12-08Bibliographically approved

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