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  • 标题:Using FRITIOF to Model Nucleus-Nucleus Interactions in a Cosmic Ray Detector
  • 本地全文:下载
  • 作者:Sanchez, Carlos A. ; Murai, Kazuhiko ; Wold, Donald C.
  • 期刊名称:Journal of the Arkansas Academy of Science
  • 印刷版ISSN:2326-0491
  • 出版年度:1995
  • 卷号:49
  • 期号:1
  • 页码:160-165
  • 出版社:University of Arkansas, Fayetteville
  • 摘要:Ascintillating optical fiber calorimeter (SOFCAL) isbeing developed by NASA/Marshall Space Flight Center for use in experiments to study the spectrum of high-energy cosmic rays and gamma rays from 100 GeV to 1,000 TeV. SOFCAL willnot saturate for long exposures and this calorimeter inthese balloon-borne emulsion chambers willbe helpful for the study of the composition of primary cosmic-ray nuclei. For primary nuclei with energies much greater than 1014 eV, nucleus-nucleus interactions are likely to exhibit characteristics of a quark-gluon plasma (QGP). Aparticle event generator was used tomodel the collision of a cosmic-ray nucleus with a target nucleus inan emulsion chamber. FRITIOF withLUCIAE was chosen tomodel collisions of primary cosmic rays inan emulsion chamber with SOFCAL. Pseudo-rapidity distributions were computed for protons on lead at 200 GeV/c and compared with experimental data. Pseudo-rapidity distributions were computed for protons or iron incident on a carbon or silver nucleus. For gamma-rays from nucleus-nucleus interactions, the total energy of the electromagnetic component Z£y was computed. The partial coefficient ofinelasticity kr defined by L£"y = kY E0 ,was computed from the primary energy Eo of the cosmic rays. The f(ky )-distributions were computed and compared with existing calorimeter data. Funding was provided by the NASA/University Joint Venture (JOVE) Program.
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