1995
DOI: 10.1103/physrevlett.74.5001
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Cluster Formation during Expansion of Hot and Compressed Nuclear Matter Produced in Central Collisions of Au on Au at 250AMeV

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Cited by 36 publications
(26 citation statements)
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“…Thus, the size of the emission sources of the d, α, t and 3 He particles would be about 63%, 54%, 53% and 44% of that of the protons, respectively. This finding is in qualitative agreement with the results of an earlier investigation [28] of the cluster formation process in central Au+Au collisions at 250 A·MeV. There, the authors compare the experimental data with predictions of a model which describes the hydrodynamic isotropic expansion of an ideal nucleonic gas and the clustering by statistical disassembly.…”
Section: Discussionsupporting
confidence: 88%
“…Thus, the size of the emission sources of the d, α, t and 3 He particles would be about 63%, 54%, 53% and 44% of that of the protons, respectively. This finding is in qualitative agreement with the results of an earlier investigation [28] of the cluster formation process in central Au+Au collisions at 250 A·MeV. There, the authors compare the experimental data with predictions of a model which describes the hydrodynamic isotropic expansion of an ideal nucleonic gas and the clustering by statistical disassembly.…”
Section: Discussionsupporting
confidence: 88%
“…Older exclusive information on heavy cluster formation from Bevalac times was limited to an experiment at 200 A MeV [15] concentrating on sideflow: a remarkable result of this study was the demonstrated higher sensitivity of the IMF's to flow, a fact that had been anticipated in the framework of hydrodynamical model calculations [16]. Since then, new information from central or semicentral collisions at energies beyond 100 A MeV has emerged from work done both at Berkeley and Darmstadt [17][18][19][20][21][22][23][24][25][26][27][28][29][30][31].…”
Section: Introductionmentioning
confidence: 93%
“…One of the important new observations, favoured by the sensitivity of IMF's to flow, was the overwhelming and unambiguous evidence of a new kind of axially symmetric or 'radial' flow [20][21][22]26,28] as a signature of highly exclusive central collisions. This flow was far more important in magnitude than the sideflow predicted [32] and discovered [33,34] earlier and was characteristic of participant matter, in contrast to the sideflow phenomenon which was primarily interpreted as a spectator phenomenon.…”
Section: Introductionmentioning
confidence: 99%
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“…Despite of extensive efforts of several experimental groups [8] - [13] this question is not finally decided yet. The main reason is that, surprisingly enough, both approaches give very similar results for at least two key observables.…”
Section: Introductionmentioning
confidence: 99%