Abstract

We calculate differential energy spectra (xF-distributions) of charmed particles produced in proton–nucleus collisions, assuming the existence of intrinsic heavy quark components in the proton wavefunction. For the calculation, the recently proposed factorization scheme is used, based on the colour glass condensate theory and specially suited for predictions of a production of particles with large rapidities. It is argued that the intrinsic charm component can, if it exists, dominate in a sum of two components, intrinsic + extrinsic, of the inclusive spectrum of charmed particles produced in proton–nucleus collisions at high energies, in the region of medium xF, 0.15 < xF < 0.7, and can give noticeable contribution to atmospheric fluxes of prompt muons and neutrinos.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.