Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem.

Details Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem. Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem.

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989svjnp..50...90b&link_type=abstract

Sov. J. Nucl. Phys., Vol. 50, No. 1, p. 90 - 99

Physics

9

Neutrinos: Earth Atmosphere, Muons: Earth Atmosphere, Cosmic Rays: Energy Spectra

Scientific paper

The energy spectra of hadrons and leptons in the atmosphere are obtained as solutions of transport equations for these particles in the energy range 1 - 105GeV. The spectrum of primary cosmic radiation is used as a boundary condition. The calculated energy spectra of the particles are given by the solution of a direct problem and do not require an additional normalization to the experimental data. The calculated energy spectrum of muons at sea level agrees with the experimental data with an error 8 - 10% in the energy range 10 - 103GeV, and with an error 10 - 15% in the energy range 103 - 104GeV. The error in the calculated neutrino spectra is of the same order of magnitude.

Affiliated with

Also associated with

No associations

Rating

Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem. does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectra of hadrons, muons, and neutrinos in the atmosphere as the solution of a direct problem. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1710368