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Space-time evolution of the reactionsN14+27Al,Au197atE/A=75 MeV andXe129+27Al,Sn122atE/A=31 MeV probed by two-proton intensity interferometry

Authors :
H.M. Xu
D. E. Fields
R. T. de Souza
T. Murakami
D.P. Sanderson
N. Carlin
M. B. Tsang
Scott Pratt
W. G. Gong
R. Planeta
C. K. Gelbke
Y. D. Kim
Sherry Yennello
V. E. Viola
Giacomo Poggi
Wolfgang Bauer
K. Kwiatkowski
W. G. Lynch
Source :
Physical Review C. 43:1804-1820
Publication Year :
1991
Publisher :
American Physical Society (APS), 1991.

Abstract

Two-proton correlation functions have been measured at {theta}{sub lab}{approx}25{degree} for the forward kinematics'' reactions {sup 14}N+{sup 27}Al, {sup 14}N+{sup 197}Au at {ital E}/{ital A}=75 MeV, for the inverse kinematics'' reaction {sup 129}Xe+{sup 27}Al at {ital E}/{ital A}=31 MeV, and for the nearly symmetric reaction {sup 129}Xe+{sup 122}Sn at {ital E}/{ital A}=31 MeV. For the reactions at 75 MeV per nucleon, the correlation functions exhibit pronounced maxima at relative proton momenta, {ital q}{approx}20 MeV/{ital c}, and minima at {ital q}{approx}0 MeV/{ital 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 {ital q}{approx}20 MeV/{ital c}, but only minima at {ital q}{approx}0 MeV/{ital 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.

Details

ISSN :
1089490X and 05562813
Volume :
43
Database :
OpenAIRE
Journal :
Physical Review C
Accession number :
edsair.doi...........0989a11764e40c5efab80d3cd273bda0
Full Text :
https://doi.org/10.1103/physrevc.43.1804