Prompt atmospheric neutrinos in the quark-gluon string model
arXiv:1812.11341 · doi:10.1140/epjc/s10052-019-7547-0
Abstract
We calculate the atmospheric flux of prompt neutrinos, produced in decays of the charmed particles at energies beyond 1 TeV. Cross sections of the -mesons and baryons production in pA and A collisions are calculated in the phenomenological quark-gluon string model (QGSM) which is updated using of the recent measurements of cross sections of the charmed meson production in the LHC experiments. A new estimate of the prompt atmospheric neutrino flux is obtained and compared with the limit of the IceCube experiment as well as with predictions of other charm production models.
15 pages, 18 figures; corrected text and figures, added references
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Cited by in corpus (4)
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- Greybody Factor for a Rotating Bardeen Black Hole by Perfect Fluid Dark Matter
- High-energy spectra of the atmospheric neutrinos: predictions and measurements