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MANTS-GNN Meeting 2014

Sep 19 – 21, 2014
Geneva, Switzerland
CET timezone

Session

Atmospheric Neutrinos / Charm

Sep 20, 2014, 2:00 PM
Geneva, Switzerland

Geneva, Switzerland

CERN 385 Route de Meyrin 1217 Meyrin Switzerland

Presentation materials

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  1. 18. hadron and charm production in the atmosphere - Introductory remarks from ISVHECRI 2014
    Paolo Desiati (o=uwmad,ou=Institutions,dc=icecube,dc=wisc,dc=edu)
    9/20/14, 2:00 PM
    Atmospheric Neutrinos & Charm
    This is an introduction to the Charm Production Session of the MANTS 2014 Meeting. It includes a brief summary of hadronic production in extensive air shower, including heavy quark production.
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  2. 29. Self-veto and charm production with HE neutrinos in IceCube
    Gary Binder (UC Berkeley)
    9/20/14, 2:25 PM
    Atmospheric Neutrinos & Charm
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  3. 5. Atmospheric neutrinos and charm production
    Chang Hyon Ha (o=lbl,ou=Institutions,dc=icecube,dc=wisc,dc=edu)
    9/20/14, 2:50 PM
    Atmospheric Neutrinos & Charm
    .
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  4. 17. Charm with High Energy Muons in IceCube - Summary of P.Berghaus' results
    Mr Hans-Peter Bretz (o=desy-zeuthen,ou=Institutions,dc=icecube,dc=wisc,dc=edu)
    9/20/14, 3:15 PM
    Atmospheric Neutrinos & Charm
    This talk gives a summary of an analysis to measure the high energy muon spectrum performed on one year of data of the IceCube detector. The main background for single high energy muons are high-multiplicity bundles comprised of lower energy muons. This analysis attempts to seperate single muons from muon bundles through their different energy loss profiles. A preliminary best fit on the muon...
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  5. 35. Atmospheric neutrinos and diffuse fluxes of cosmic neutrinos with the ANTARES detector.
    Annarita Margiotta (Universita' di Bologna and Sezione INFN di Bologna)
    9/20/14, 4:10 PM
    Atmospheric Neutrinos & Charm
    The undersea neutrino telescope ANTARES measured the atmospheric muon neutrino energy spectrum using data collected in 4 years of data taking. A short review of the methodology and of the results will be given. The search for diffuse fluxes of cosmic neutrinos using track-like events will be presented as well.
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  6. 21. Contribution of Kshort to the flux of atmospheric electron neutrinos
    Dr Thomas Gaisser (University of Delaware)
    9/20/14, 4:45 PM
    Atmospheric Neutrinos & Charm
    We report on a calculation of the contribution of the rare Ke3 decay of the Kshort, which becomes comparable to the contribution from Klong and charged kaons above 100 TeV.
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  7. 30. Review of charm production in colliders (RHIC, ALICE, LHCb, ….)
    Alessandro Grelli (University of Utrecht)
    9/20/14, 5:05 PM
    Atmospheric Neutrinos & Charm
    .
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  8. 31. High energy hadronic interaction models bridging accelerator with cosmic ray physics
    Anatoli Fedynitch (o=uwmad,ou=Institutions,dc=icecube,dc=wisc,dc=edu)
    9/20/14, 5:40 PM
    Atmospheric Neutrinos & Charm
    In this talk I will present the relevance of accelerator data and for cosmic ray physics. The production of charm in hadronic interaction models will be introduced and comparisons of model predictions and available data shown.
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