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Phys. Rev. C 43, 1804–1820 (1991)

Space-time evolution of the reactions 14N+27Al, 197Au at E/A=75 MeV and 129Xe+27Al, 122Sn at E/A=31 MeV probed by two-proton intensity interferometry

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W. G. Gong, C. K. Gelbke, W. Bauer, N. Carlin, R. T. de Souza, Y. D. Kim, W. G. Lynch, T. Murakami, G. Poggi, D. P. Sanderson, M. B. Tsang, and H. M. Xu
National Superconducting Cyclotron Laboratory and Department of Physics Astronomy, Michigan State University, East Lansing, Michigan 48824

D. E. Fields, K. Kwiatkowski, R. Płaneta, V. E. Viola, Jr., and S. J. Yennello
Indiana University Cyclotron Facility, Indiana University, Bloomington, Indiana 47405

S. Pratt
Department of Physics, University of Wisconsin, Madison, Wisconsin 53706

Received 15 October 1990; published in the issue dated April 1991

Two-proton correlation functions have been measured at θlab≊25° for the ‘‘forward kinematics’’ reactions 14N+27Al, 14N+197Au at E/A=75 MeV, for the ‘‘inverse kinematics’’ reaction 129Xe+27Al at E/A=31 MeV, and for the nearly symmetric reaction 129Xe+122Sn at E/A=31 MeV. For the reactions at 75 MeV per nucleon, the correlation functions exhibit pronounced maxima at relative proton momenta, q≊20 MeV/c, and minima at q≊0 MeV/c. These correlations indicate emission from fast, nonequilibrium processes. They are analyzed in terms of standard Gaussian source parametrizations and compared to microscopic simulations performed with the Boltzmann-Uehling-Uhlenbeck equation. For the reactions at 31 MeV per nucleon, the two-proton correlation functions do not exhibit maxima at q≊20 MeV/c, but only minima at q≊0 MeV/c. These correlations indicate emission on a slower time scale. They can be reproduced by calculations based on the Weisskopf formula for evaporative emission from fully equilibrated compound nuclei. For all reactions, the measured longitudinal and transverse correlation functions are very similar, in agreement with theoretical predictions.

© 1991 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.43.1804
DOI:
10.1103/PhysRevC.43.1804
PACS:
25.70.Np