Inclusive production of neutrons in 300-GeV/c pp interactions

F. T. Dao, R. Hanft, J. Lach, E. Malamud, F. Nezrick, V. Davidson, A. Firestone, D. Lam, F. Nagy, C. Peck, A. Sheng, R. Poster, P. Schlein, W. Slater, and A. Dzierba
Phys. Rev. D 10, 3588 – Published 1 December 1974
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Abstract

An estimate of the average number of neutrons in 300-GeV/c pp collisions can be made from observed neutron secondary interactions (stars). The data are from a 35000-picture exposure of the Fermi National Accelerator Laboratory 30-in. hydrogen bubble chamber. The average number of neutrons and antineutrons per inelastic collision is found to be n+n¯=0.8±0.2, and their average laboratory energy is ∼ 34 GeV.

  • Received 22 July 1974

DOI:https://doi.org/10.1103/PhysRevD.10.3588

©1974 American Physical Society

Authors & Affiliations

F. T. Dao, R. Hanft, J. Lach, E. Malamud, and F. Nezrick*

  • Fermi National Accelerator Laboratory, Batavia, Illinois 60510

V. Davidson, A. Firestone, D. Lam, F. Nagy, C. Peck, and A. Sheng

  • California Institute of Technology, Pasadena, California 91109

R. Poster, P. Schlein, and W. Slater

  • University of California, Los Angeles, California 90024

A. Dzierba

  • Indiana University, Bloomington, Indiana 47401

  • *Operated by Universities Research Association Inc. under contract with the U. S. Atomic Energy Commission.
  • Work supported in part by the National Science Foundation under Grant No. GP-33565.

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Issue

Vol. 10, Iss. 11 — 1 December 1974

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