Physics – Nuclear Physics
Scientific paper
Aug 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6...72k&link_type=abstract
In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 72-75 (SEE N85-35848 24-93)
Physics
Nuclear Physics
Angular Distribution, Cosmic Ray Showers, Nuclear Emulsions, Nuclei (Nuclear Physics), Particle Collisions, Pions, Energy Spectra, Kinematics, Particle Acceleration, Particle Mass, Protons, Regression Coefficients, Scaling Laws
Scientific paper
For 435 accelerator produced antipions jets of 20 GeV/c and 300 GeV, in nuclear emulsion, eta(theta)'s have been individually calculated for each jet, where eta(theta) is a kinematic parameter introduced in order to approximate the LS (laboratory system) rapidity, eta = arctan h (beta cos theta). By taking further averages by dividing the samples into groupings of the LS energy Epi = m cos h etapi Nh, the number of heavy prongs with LS velocity beta 0.7, and n , the number of charged shower particles with LS velocity beta 0.7, much less than eta (theta) much greater than are obtained. By use of the KNO (Koba-Nielsen-Olesen) scaling variable, xi = ns/,n sub s. good fit is found of data to regression function.
Kim C.-O.
Kim Sang Nyon
Park I. G.
Yoon S.-Ch.
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