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26 April 2024
 
  » arxiv » nucl-ex/9502001

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Radial Flow in Au+Au Collisions at E=0.25-1.15 A GeV
M.A. Lisa ; S. Albergo ; F. Bieser ; F.P. Brady ; Z. Caccia ; D.A. Cebra ; A.D. Chacon ; J.L. Chance ; Y. Choi ; S. Costa ; J.B. Elliott ; M.L. Gilkes ; J.A. Hauger ; A.S. Hirsch ; E.L. Hjort ; A. Insolia ; M. Justice ; D. Keane ; J. Kintner ; H.S. Matis ; M. McMahan ; C. McParland ; D.L. Olson ; M.D. Partlan ; N.T. Porile ; R. Potenza ; G. Rai ; J. Rasmussen ; H.G. Ritter ; J. Romanski ; J.L. Romero ; G.V. Russo ; R. Scharenberg ; A. Scott ; Y. Shao ; B.K. Srivastava ; T.J.M. Symons ; M. Tincknell ; C. Tuve ; S. Wang ; P. Warren ; G.D. Westfall ; H.H. Wieman ; K. Wolf ;
Date 10 Feb 1995
Journal Phys.Rev.Lett. 75 (1995) 2662-2665
Subject nucl-ex
AffiliationEOS Collaboration: LBL-Kent State-Purdue-UC Davis-Texas A&M-Catania
AbstractA systematic study of energy spectra for light particles emitted at midrapidity from Au+Au collisions at E=0.25-1.15 A GeV reveals a significant non-thermal component consistent with a collective radial flow. This component is evaluated as a function of bombarding energy and event centrality. Comparisons to Quantum Molecular Dynamics (QMD) and Boltzmann-Uehling-Uhlenbeck (BUU) models are made for different equations of state.
Source arXiv, nucl-ex/9502001
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