High-energy gamma-ray production in the heavy-ion reaction Xe136 + Sn at E/A=89 and 124 MeV

J. Clayton, J. Stevenson, W. Benenson, Y. Chen, E. Kashy, A. R. Lampis, M. Samuel, C. L. Tam, M. F. Mohar, D. J. Morrissey, T. K. Murakami, B. Sherrill, and J. S. Winfield
Phys. Rev. C 40, 1207 – Published 1 September 1989
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Abstract

Energy spectra and angular distributions have been measured for high-energy gamma rays (Eγ>40 MeV) from the heavy-ion reaction 136Xe+Sn at bombarding energies of E/A=89 and 124 MeV. Gamma rays are observed with energies up to 160 MeV, and the energy spectra are roughly exponential above 40 MeV. The angular distributions of the gamma rays are forward peaked in the laboratory frame and are consistent with emission from a source moving with a velocity equal to the nucleon-nucleon center-of-mass velocity. The angular distributions show no significant anisotropy in the nucleon-nucleon frame. The production cross sections agree with systematics observed for lighter systems.

  • Received 3 April 1989

DOI:https://doi.org/10.1103/PhysRevC.40.1207

©1989 American Physical Society

Authors & Affiliations

J. Clayton, J. Stevenson, W. Benenson, Y. Chen, E. Kashy, A. R. Lampis, M. Samuel, and C. L. Tam

  • National Superconducting Cyclotron Laboratory and Department of Physics Astronomy, Michigan State University, East Lansing, Michigan 48824

M. F. Mohar and D. J. Morrissey

  • National Superconducting Cyclotron Laboratory and Department of Chemistry, Michigan State University, East Lansing, Michigan 48824

T. K. Murakami, B. Sherrill, and J. S. Winfield

  • National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824

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Vol. 40, Iss. 3 — September 1989

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