Abstract
The expansion phase of a hot nuclear system as created in an energetic heavy ion collision is calculated and discussed by aselfconsistent field-theoretical model which consideres dynamical growth ofinstabilities arisig from strong fluctuations of the one-body density. Firstmultiplicity distributions andmass spectra resulting from a series of numerical runs in a two dimensional model world are presented and discussed.
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References
G. Bertsch, P.J. Siemens, Phys.Lett. 126B (1983) 9
D.K.Scott, MSUCL peprint-434, September 1983
B.Strack, J.Knoll, GSI Scientific Report 1982, 119
A.Z. Mekjian, Phys.Rev.Lett. 38 (1977) 640, Phys.Rev. C17 (1978) 1051
H. Gutbrod et al., Phys. Rev. Lett. 37 (1976) 667
H. Sato, K. Yazaki, Phys. Lett. 98B (1981) 153
I. Motavey, J. Zimany, Nucl.Phys. A316 (1979) 490
L.P.Csernai et al., UFTP Preprint-70, 1982
M.E. Fisher, Physics 3 (1967), 255
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Strack, B., Knoll, J. Expansion and disasembly phase of energetic nuclear reactions: A problem of dynamical instabilities?. Z Physik A 315, 249–250 (1984). https://doi.org/10.1007/BF01419387
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DOI: https://doi.org/10.1007/BF01419387