EPJ Web of Conferences (Jan 2015)

Study of charm production in the forward cone at energy ELab ∼ 75 TeV with a two-storey X-ray emulsion chamber exposed at, mountain altitudes

  • Borisov A.S.,
  • Chubenko A.P.,
  • Denisova V.G.,
  • Galkin V.I.,
  • Guseva Z.M.,
  • Kanevskaya E.A.,
  • Kogan M.G.,
  • Kulikov V.N.,
  • Morozov A.E.,
  • Mukhamedshin R.A.,
  • Puchkov V.S.,
  • Nazarov S.I.,
  • Pyatovsky S.E.,
  • Shoziyoev G.P.,
  • Smirnova M.D.,
  • Vargasov A.V.

DOI
https://doi.org/10.1051/epjconf/20159910004
Journal volume & issue
Vol. 99
p. 10004

Abstract

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The origin of the cosmic ray hadron excess observed in a deep uniform lead X-ray emulsion chamber (XREC) at depths larger than 70 radiation lengths is analyzed. We present preliminary experimental data on the absorption of cosmic ray hadrons in the two-storey XREC with a large air gap exposed at the Tien Shan mountains. The design of the chamber was especially invented to prove the hypothesis on a substantial increase of the charm particle production cross section with energy at ELab ∼ 75 TeV as the main source of the darkness spot excess observed on X-ray films. Experimental data obtained with both a 2-storey XREC and a deep uniform XREC are compared with simulation results calculated with the FANSY 1.0 model. The comparison reveals a qualitative agreement between experimental and simulated data under the assumption of high values of charm particle production cross section at ELab ∼ 75 TeV in the forward kinematic region at xLab > 0.1.