Phys. Rev. C
61,
061601(R)
(2000)
[4 pages]
Isotropic emission components in splintering central collisions: (17-115)A MeV 40Ar + Cu, Ag, Au
Rulin Sun et al.
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Rulin Sun1, E. Colin1,4, N. N. Ajitanand1, John M. Alexander1, M. A. Barton3, P. A. DeYoung3, K. L. Drake3, A. Elmaani1,*, C. J. Gelderloos6,†, E. E. Gualtieri2, D. Guinet4, S. Hannuschke2, J. A. Jaasma3, L. Kowalski5, Roy A. Lacey1, J. Lauret1, E. Norbeck7, R. Pak2, G. F. Peaslee3, M. Stern4, N. T. B. Stone2, S. D. Sundbeck3, A. M. Vander Molen2, G. D. Westfall2, L. B. Yang7, and J. Yee2
1Department of Chemistry, State University of New York at Stony Brook, Stony Brook, New York 11794 2National Superconducting Laboratory, Michigan State University, East Lansing, Michigan 48824 3Departments of Chemistry and Physics, Hope College, Holland, Michigan 49423 4Institut de Physique Nucléaire de Lyon, Institut National de Physique Nucléaire et de Physique des Particules–Centre National de la Recherche Scientifique/UniversitéClaude Bernard, 43, Blvd. du 11 Novembre 1918, F-69622 Villeurbanne, Cedex, France 5Department of Physics and Geoscience, Montclair State College, Upper Montclair, New Jersey 07043 6Nuclear Physics Laboratory, University of Colorado, Boulder, Colorado 80309-0446 7Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242
Received 8 November 1999; published 2 May 2000
The ensemble of charged isotropically emitted ejectiles is studied for central collisions of (17-115)A MeV 40Ar + Cu, Ag, Au. Measurements of average multiplicities, spectral slopes, and masses of the heaviest fragments are compared to statistical models for multifragmentation or sequential evaporation. The multifragmentation models predict much more complete nuclear disassembly than is observed. The evaporation model reproduces the data much more closely except for the spectra of Z=1 ejectiles. The kinetic energies of Z=1 and 2 ejectiles are much less than found for 1A GeV 197Au+12C for similar energy depositions. Entrance channel dynamics seem to affect the isotropic emission ensembles, often taken to define an equilibrated emission source.
© 2000 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevC.61.061601
DOI:
10.1103/PhysRevC.61.061601
PACS:
25.70.Pq, 25.70.Hi, 25.70.Pq
*Present address: Battelle Pacific Northwest National Laboratory, National Security Division, Box 999, K6-48, Richland, WA 99352. †Present address: Hughes Space and Communications, P.O. Box 92919, Los Angeles, CA 90009.
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