AN ANALYSIS OF COSMIC RAY SHOWERS PRODUCED BY HIGH ENERGY PRIMARY PARTICLES BASED ON THE EXCITED NUCLEON MODEL

Journal Article · Sat Jul 01 04:00:00 EDT 1961 · Zhur. Eksptl'. i Teoret. Fiz.

OSTI ID:4841517

Sanko, L A; Takibaev, Zh S; Usik, P A

High energy (E> 10/sup 11/ ev) interactions of cosmic ray nucleons in photographic emulsions are analyzed on the basis of the excited nucleon model. The angular distribution of excited nucleons in the cms is presented. Anisotropy of the angular distribution of the shower particles and the multiplicity of the shower particles are examined in relation to the velocity and emission angle of the excited nucleon. The experimental results are compared with the predictions of the single-meson pole approximation. (auth)

• Research Organization: Inst. of Nuclear Physics, Academy of Sciences, Kazakh SSr
• NSA Number: NSA-15-028334
• OSTI ID: 4841517
• Journal Information: Zhur. Eksptl'. i Teoret. Fiz., Journal Name: Zhur. Eksptl'. i Teoret. Fiz. Vol. Vol: 41
• Country of Publication: Country unknown/Code not available
• Language: Russian

Related Subjects

ANGULAR DISTRIBUTION
ANISOTROPY
COSMIC RADIATION
ENERGY RANGE
EXCITATION
INTERACTIONS
MEASURED VALUES
MESONS
MULTIPLICITY
NUCLEAR EMULSIONS
NUCLEAR STRUCTURE
NUCLEONS
OPE MODEL
PARTICLE TRACKS
PHYSICS
PRODUCTION
SCATTERING
VELOCITY