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Physics Seminar: Updating the Prompt Atmospheric Neutrino Background at IceCube


September 17, 2015
12:00 pm
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Physics Department

Place: Namm 823
Thursday, September 17 at 12:00 PM
Presented by Jim Talbert
Faculty and students are welcome, light refreshments will be served.


I will present an updated prediction of the flux of neutrinos arising from the prompt decay of charmed hadrons formed in collisions of cosmic rays on the upper atmosphere. This ‘prompt’ flux of atmospheric neutrinos serves as a principal background that must be discriminated against at neutrino telescopes such as IceCube, whose primary mission is the detection of astrophysical neutrinos of similar energies. Our calculation is semianalytic, employs NLO pQCD Monte-Carlo event generation and up-todate parton distribution functions, and has been validated in detail with the recent LHCb charm production data, which cover a similar kinematical region. The calculation of the lepton fluxes is performed in the well-established framework of ‘cascade’ equations, which trace the (re)generation and evolution of nucleons, mesons, and leptons in the earth’s atmosphere. Our results are consistent with former calculations, though provide a much more robust uncertainty estimate.

[icon name=”file-pdf-o” class=””] Click to view poster.

Nucleus Volume 9 WInter 2018