ANGULAR DISTRIBUTION OF SHOWER PARTICLES IN STARS PRODUCED BY HIGH ENERGY PARTICLES (in Russian)
Journal Article
·
· Zhur. Eksptl'. i Teoret. Fiz.
OSTI ID:4215976
An analysis is carried out of the angular distribution of a unique star consisting of 20 + 15 + 59 p and probably produced by a proton of energy > 1000 Bev. The angular distribution of the shower particles is characterized bv two maxima and is explained by the anisotropic angular distribution and power-law energy spectrum of the created particles in the c.m.s. The presence of a large number of strongly ionizing particles indicates that the Heitler--Terreaux theory does not give a correct description of pi -meson production. The angular distribution of 11 other showers with the same characteristic anisotropy is also investigated. (auth)
- Research Organization:
- Inst. of Nuclear Physics, Academy of Sciences, Kazakh S.S.R.
- NSA Number:
- NSA-13-020477
- OSTI ID:
- 4215976
- Journal Information:
- Zhur. Eksptl'. i Teoret. Fiz., Journal Name: Zhur. Eksptl'. i Teoret. Fiz. Vol. Vol: 37
- Country of Publication:
- Country unknown/Code not available
- Language:
- Russian
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