Perturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC
arXiv:1502.01076 · doi:10.1007/JHEP06(2015)110
Abstract
We re-evaluate the prompt atmospheric neutrino flux, using the measured charm cross sections at RHIC and the Large Hadron Collider to constrain perturbative QCD parameters such as the factorization and renormalization scales, as well as modern parton distribution functions and recent estimates of the cosmic-ray spectra. We find that our result for the prompt neutrino flux is lower than previous perturbative QCD estimates and, consequently, alters the signal-to-background statistics of the recent IceCube measurements at high energies.
19 pages, 8 figures, Published version
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Cited by in corpus (10)
- Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption
- Perturbative charm production and the prompt atmospheric neutrino flux in light of RHIC and LHC
- Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects
- Using hadron-in-jet data in a global analysis of fragmentation functions
- On the IceCube spectral anomaly
- Dark Matter interpretation of low energy IceCube MESE excess
- Charm decay in slow-jet supernovae as the origin of the IceCube ultra-high energy neutrino events
- Mapping the dominant regions of the phase space associated with production relevant for the Prompt Atmospheric Neutrino Flux
- Diffuse axion-like particle searches