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Search: WFRF:(Reno Mary Hall)

  • Result 11-14 of 14
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11.
  • Jeong, Yu Seon, et al. (author)
  • Prompt atmospheric neutrino flux
  • 2016
  • Conference paper (other academic/artistic)abstract
    • We evaluate the prompt atmospheric neutrino flux including nuclear correction and B hadron contribution in the different frameworks: NLO perturbative QCD and dipole models. The nuclear effect is larger in the prompt neutrino flux than in the total charm production cross section, and it reduces the fluxes by 10%−30% depending on the model. We also investigate the uncertainty using the QCD scales allowed by the charm cross section data from RHIC and LHC experiments.
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12.
  • Jeong, Yu Seon, et al. (author)
  • Prompt atmospheric neutrino flux from the various QCD models
  • 2017
  • In: XLVI International Symposium On Multiparticle Dynamics (ISMD 2016). - : EDP Sciences.
  • Conference paper (peer-reviewed)abstract
    • 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.
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13.
  • Jeong, Yu Seon, et al. (author)
  • Prompt atmospheric neutrino flux in perturbative QCD and its theoretical uncertainties
  • 2017
  • In: XXVII International Conference on Neutrino Physics and Astrophysics (Neutrino2016). - : Institute of Physics Publishing (IOPP).
  • Conference paper (peer-reviewed)abstract
    • Using the most recent PDFs and the cosmic ray spectrum, we evaluate the charm/bottom induced prompt atmospheric muon neutrino fluxes including nuclear corrections. We investigate their impact in perturbative QCD and estimate the comprehensive uncertainties from other various factors. The prompt atmospheric tau neutrino fluxes are also presented.
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14.
  • Reno, Mary Hall, et al. (author)
  • EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors
  • 2022
  • In: 37th International Cosmic Ray Conference, ICRC 2021. - : Sissa Medialab Srl.
  • Conference paper (peer-reviewed)abstract
    • Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe. Detection of neutrinos, in particular tau neutrinos generated by neutrino oscillations in transit from their sources to Earth, is possible for neutrino energies above 10 PeV using optical Cherenkov detectors imaging upward-moving extensive air showers (EAS). These EAS are produced from Earth-interacting tau neutrinos leading to tau leptons that subsequently decay in the atmosphere. We compare neutrino detection sensitivities for generic short- and long-burst transient neutrino sources and sensitivities to the diffuse neutrino flux for the second generation Extreme Universe Space Observatory on a Super-Pressure Balloon (EUSO-SPB2) balloon-borne mission and the proposed space-based Probe of Extreme Multi-Messenger Astrophysics (POEMMA) mission.
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  • Result 11-14 of 14

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