The Modified Weighted Slab Technique: Description of the Technique and Models

Details The Modified Weighted Slab Technique: Description of the Technique and Models The Modified Weighted Slab Technique: Description of the Technique and Models

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....4..215j&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

In an atempt to understand the source and propagation of galactic cosmic rays (Webber, 1997) we have employed the modified weighted slab technique of Ptuskin, Jones, and Ormes along with recent values of the relevant cross sections to compute primary to secondary ratios including B/C and Sub-Fe/Fe for different galactic propagation models. The models that we have considered are the standard diffusion model (leaky box or thin disk model), the dynamical halo model, the turbulent diffusion model and a model with minimal reacceleration. The modified weighted slab technique will be briefly discussed and a more detailed description of the models will be given. The results of our calculation will be given in an accompanying paper.

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