Investigation of transverse collective flow of intermediate mass fragments

Z. Kohley, L. W. May, S. Wuenschel, A. Bonasera, K. Hagel, R. Tripathi, R. Wada, G. A. Souliotis, D. V. Shetty, S. Galanopoulos, M. Mehlman, W. B. Smith, S. N. Soisson, B. C. Stein, and S. J. Yennello
Phys. Rev. C 82, 064601 – Published 3 December 2010

Abstract

The transverse flow of intermediate mass fragments (IMFs) has been investigated for the 35 MeV/u 70Zn+70Zn, 64Zn+64Zn, and 64Ni+64Ni systems. A transition from the IMF transverse flow strongly depending on the mass of the system, in the most violent collisions, to a dependence on the charge of the system, for the peripheral reactions, is shown. This transition was shown to be sensitive to the density dependence of the symmetry energy using the antisymmetrized molecular-dynamics model. The results present an observable, the IMF transverse flow, that can be used to probe the nuclear equation of state. Comparison with the simulation demonstrated a preference for a stiff density dependence of the symmetry energy.

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  • Received 6 April 2010

DOI:https://doi.org/10.1103/PhysRevC.82.064601

© 2010 The American Physical Society

Authors & Affiliations

Z. Kohley1,2,*, L. W. May1,2, S. Wuenschel1,2, A. Bonasera2,3, K. Hagel2, R. Tripathi2, R. Wada2, G. A. Souliotis2,4, D. V. Shetty2,†, S. Galanopoulos2, M. Mehlman2,5, W. B. Smith2, S. N. Soisson1,2, B. C. Stein1,2, and S. J. Yennello1,2

  • 1Chemistry Department, Texas A&M University, College Station, Texas 77843, USA
  • 2Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA
  • 3Laboratori Nazionali del Sud, Istituto Nazionale di Fisica Nucleare, I-95123 Catania, Italy
  • 4Laboratory of Physical Chemistry, Department of Chemistry, National and Kapodistrian University of Athens, Athens GR-15771, Greece
  • 5Physics and Astronomy Department, Texas A&M University, College Station, Texas 77843, USA

  • *zkohley@comp.tamu.edu
  • Also at Physics Department, Western Michigan University, Kalamazoo, MI 49008.

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Vol. 82, Iss. 6 — December 2010

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