This is the development page for the PromptNuFlux project.
PromptNuFlux computes the prompt atmospheric neutrino flux , including the total associated theory uncertainty, for a range of energies between GeV and GeV. The prompt flux is computed as an interpolation of the results obtained in arXiv:1511.06346.
Results are available for five different parametrizations of the input cosmic ray flux: BPL, H3P, H3A, H14a, H14b.
For usage, please see the README in the tarball.
The source code is available for download here.
If you use PromptNuFlux for scientific publications, please cite this webpage and:
R. Gauld, J. Rojo, L. Rottoli, J. Talbert, Charm production in the forward region: constraints on the small-x gluon and backgrounds for neutrino astronomy, JHEP 1511 (2015) 009, arXiv:1506.08025
R. Gauld, J. Rojo, L. Rottoli, S. Sarkar, J. Talbert, The prompt atmospheric neutrino flux in the light of LHCb , 1511.06346
PromptNuFlux developers: Luca Rottoli (contact)