Hadronic interactions at energies around 10/sup 3/ TeV inferred fromthe large-scale emulsion-chamber experiment at Mt. Fuji
Journal Article
·
· Phys. Rev. D; (United States)
Details of experimental results, obtained with large-scale emulsion chambers at Mt. Fuji (3776 m above sea level), are presented. The experimental data, which is sensitive to hadronic interactions at energies around 10/sup 3/ TeV, is compared with Monte Carlo simulations based on various assumed interaction models and primary particles. The results may be briefly summarized as follows. (1) Scaling in the fragmentation region can be valid up to at least 10/sup 3/ TeV only if the primary particles are mixed with significant amounts of heavy nuclei at energies over 10/sup 14/ eV. (2) Cross sections should continue to increase with energy up to 10/sup 3/ TeV, at least, at almost the same rate as that obtained at lower energies. (3) There exists some evidence to indicate remarkable production of particles or jets with high P/sub t/ of several GeV/c at energies around 10/sup 3/ TeV. (4) Hadron-to-..gamma..-ray ratios in the observed family events remain almost within the scope of simulation prediction. Other interesting characteristics of family events are also discussed.
- Research Organization:
- Department of Physics, Hirosaki University, Aomori, Japan
- OSTI ID:
- 6071834
- Journal Information:
- Phys. Rev. D; (United States), Journal Name: Phys. Rev. D; (United States) Vol. 24:9; ISSN PRVDA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Large-scale emulsion chamber experiment at Mt. Fuji
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Hadronic interactions and primary-cosmic-ray composition at energies around 10/sup 15/--10/sup 16/ eV derived from the analysis of high-energy gamma families
Conference
·
Sat Mar 31 23:00:00 EST 1979
· AIP (Am. Inst. Phys.) Conf. Proc.; (United States)
·
OSTI ID:6252545
Properties of hadron families observed with thick-type emulsion chambers at Mts. Kanbala and Fuji and search for Centauro events
Journal Article
·
Thu Sep 01 00:00:00 EDT 1988
· Phys. Rev. D; (United States)
·
OSTI ID:6907896
Hadronic interactions and primary-cosmic-ray composition at energies around 10/sup 15/--10/sup 16/ eV derived from the analysis of high-energy gamma families
Journal Article
·
Thu Sep 01 00:00:00 EDT 1988
· Phys. Rev. D; (United States)
·
OSTI ID:6839408
Related Subjects
645103* -- High Energy Physics-- Particle Interactions & Properties-Experimental-- Strong Interactions & Baryon & Meson Properties
645104 -- High Energy Physics-- Particle Interactions & Properties-Experimental-- Strong Meson-Induced Interactions-- (-1987)
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COSMIC RADIATION
CROSS SECTIONS
ENERGY RANGE
ENERGY SPECTRA
FRAGMENTATION
HADRON-HADRON INTERACTIONS
INTERACTIONS
IONIZING RADIATIONS
JET MODEL
MATHEMATICAL MODELS
MONTE CARLO METHOD
NUCLEAR EMULSIONS
PARTICLE INTERACTIONS
PARTICLE MODELS
RADIATIONS
SPECTRA
TEV RANGE
645104 -- High Energy Physics-- Particle Interactions & Properties-Experimental-- Strong Meson-Induced Interactions-- (-1987)
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COSMIC RADIATION
CROSS SECTIONS
ENERGY RANGE
ENERGY SPECTRA
FRAGMENTATION
HADRON-HADRON INTERACTIONS
INTERACTIONS
IONIZING RADIATIONS
JET MODEL
MATHEMATICAL MODELS
MONTE CARLO METHOD
NUCLEAR EMULSIONS
PARTICLE INTERACTIONS
PARTICLE MODELS
RADIATIONS
SPECTRA
TEV RANGE