Computer Science
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aipc..276..511m&link_type=abstract
The seventh international symposium on very high energy cosmic-ray interactions. AIP Conference Proceedings, Volume 276, pp. 51
Computer Science
Hadron-Induced High- And Super-High-Energy Interactions
Scientific paper
A simplified model for halo generation is used to obtain intensity of halo as dependent on simple fundamental parameters: the attenuation length and the energy spectrum slope of single γ-quanta. The obtained result is compared with the experimental data. The single γ-quanta slope is interpreted according to appropriate numerical simulations of EMC cascade development in the air and chamber.
Maciaszczyk I.
Tomaszewski A.
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