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New calculation of radioactive secondaries in cosmic rays.


DE2001783154

Publication Date 2001
Personal Author Moskalenko, I. V.; Mashnik, S. G.; Strong, A. W.
Page Count 5
Abstract We use a new version of our numerical model for particle propagation in the Galaxy to study radioactive secondaries. For evaluation of the production cross sections we use the Los Alamos compilation of all available experimental cross sections together with calculations using the improved Cascade-Exciton Model code CEM2k. Using the radioactive secondary ratios (sup 26)Al/(sup 27)Al, (sup 36)Cl/Cl, (sup 54)Mn/Mn, we show how the improved cross-section calculations together with the new propagation code allow us to better constrain the size of the CR halo.
Keywords
  • Cosmic rays
  • Radioactive transport
  • Calculations
  • Particles
  • Cross sections
  • Evaluation
  • Production
Source Agency
  • Technical Information Center Oak Ridge Tennessee
NTIS Subject Category
  • 54D - Cosmic Ray Research
  • 77 - Nuclear Science & Technology
Corporate Authors Los Alamos National Lab., NM.; Department of Energy, Washington, DC.
Document Type Conference Proceedings
NTIS Issue Number 200125
Contract Number
  • W-7405-ENG-36
New calculation of radioactive secondaries in cosmic rays.
New calculation of radioactive secondaries in cosmic rays.
DE2001783154

  • Cosmic rays
  • Radioactive transport
  • Calculations
  • Particles
  • Cross sections
  • Evaluation
  • Production
  • Technical Information Center Oak Ridge Tennessee
  • 54D - Cosmic Ray Research
  • 77 - Nuclear Science & Technology
  • W-7405-ENG-36
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