Emulsion stars of 200, 300 and 400 GeV protons

Details Emulsion stars of 200, 300 and 400 GeV protons Emulsion stars of 200, 300 and 400 GeV protons

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977nciml..20..257t&link_type=abstract

Nuovo Cimento, Lettere, vol. 20, Oct. 22, 1977, p. 257-262. Research supported by the Marcelino Botin Foundation.

Computer Science

16

Cosmic Rays, High Energy Interactions, Nuclear Emulsions, Particle Production, Proton Beams, Angular Distribution, Cosmic Ray Showers, Energy Spectra, Particle Collisions, Secondary Cosmic Rays

Scientific paper

Stacks of 600-micron emulsion were exposed to 400 GeV proton beams, and the characteristics of about 1000 stars and of the secondaries were compared with previously observed characteristics for stars of 200 and 300 GeV protons. Data reported include angular distributions of grey and black prongs, multiplicities and dispersions for shower prongs, and angular distributions of shower particles. It is shown that emulsion stars undergo slow but steady evolutions from proton energy of 6 GeV to 200-400 GeV.

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