Title

A Statistical Interpretation of the Correlation Between IMF Multiplicity and Transverse Energy

Authors

L. Phair, Nuclear Science Division, Lawrence Berkeley National Laboratory
L. Beaulieu, Nuclear Science Division, Lawrence Berkeley National Laboratory
L. G. Moretto, Nuclear Science Division, Lawrence Berkeley National Laboratory
G. J. Wozniak, Nuclear Science Division, Lawrence Berkeley National Laboratory
D. R. Bowman, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
N. Carlin, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
L. Celano, Istituto Nazionale di Fisica Nucleare, Via Amendola 173, 70126 Bari, Italy
N. Colonna, Istituto Nazionale di Fisica Nucleare, Via Amendola 173, 70126 Bari, Italy
J. D. Dinius, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
A. Ferrero, Istituto Nazionale di Fisica Nucleare and Dipartimento di Fisica, Via Celoria 16, 20133 Milano, Italy
C. K. Gelbke, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
T. Glasmacher, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
F. Gramegna, Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Legnaro, Via Romea 4, 35020 Legnaro, Italy
D. O. Handzy, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
W. C. Hsi, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
M. J. Huang, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
I. Iori, Istituto Nazionale di Fisica Nucleare and Dipartimento di Fisica, Via Celoria 16, 20133 Milano, Italy
Y. D. Kim, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
M. A. Lisa, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
W. G. Lynch, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
G. V. Margagliotti, Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Via A. Valerio 2, 34127 Trieste, Italy
P. F. Mastinu, Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Bologna, Italy
P. M. Milazzo, Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Bologna, Italy
C. P. Montoya, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
A. Moroni, Istituto Nazionale di Fisica Nucleare and Dipartimento di Fisica, Via Celoria 16, 20133 Milano, Italy
Graham F. Peaslee, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State UniversityFollow
R. Rui, Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Via A. Valerio 2, 34127 Trieste, Italy
C. Schwarz, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
M. B. Tsang, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University
K. Tso, Nuclear Science Division, Lawrence Berkeley National Laboratory
G. Vannini, Dipartimento di Fisica and Istituto Nazionale di Fisica Nucleare, Via A. Valerio 2, 34127 Trieste, Italy
F. Zhu, National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University

Document Type

Article

Publication Date

10-18-1999

Abstract

Multifragment emission following 129Xe+197Au collisions at 30A, 40A, 50A, and 60A MeV has been studied with multidetector systems covering nearly 4π in solid angle. The correlations of both the intermediate mass fragment and light charged particle multiplicities with the transverse energy are explored. A comparison is made with results from a similar system 136Xe+209Bi at 28A MeV. The experimental trends are compared to statistical model predictions.

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