Production cross sections of gamma-rays, electrons, and positrons in p-p collisions
arXiv:1304.0879 · doi:10.1016/j.astropartphys.2014.01.001
Abstract
Because the production cross sections of gamma-rays, electrons, and positrons made in p-p collisions, $Ï_{pp\rightarrow γ}$ and $Ï_{pp\rightarrow {e}^\pm}$, respectively, are kinematically equivalent with respect to the parent pion-production cross section $Ï_{pp\rightarrow Ï}$, we obtain $Ï_{pp\rightarrow {e}^\pm}$ directly from the machine data on $Ï_{pp\rightarrow γ}$. In Sato et al. (2012), we give explicitly $Ï_{pp\rightarrow γ}$, reproducing quite well the accelerator data with LHC, namely $Ï_{pp\rightarrow {e}^\pm}$ is applicable enough over the wide energy range from GeV to 20\,PeV for projectile proton energy. We dicuss in detail the relation between the cross sections, and present explicitly $Ï_{pp\rightarrow {e}^\pm}$ that are valid into the PeV electron energy.
27 pages, 2 tables, 4 figures. Version after major revision. Accepted for publication in Astroparticle Physics; paper can be also downloaded from http://www.phys.aoyama.ac.jp/~ryo/papers/pp-collision2_ApP.pdf