Transverse collective flow and midrapidity emission of isotopically identified light charged particles

Z. Kohley, L. W. May, S. Wuenschel, M. Colonna, M. Di Toro, M. Zielinska-Pfabe, K. Hagel, R. Tripathi, A. Bonasera, 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 83, 044601 – Published 1 April 2011

Abstract

The transverse flow and relative midrapidity yield of isotopically identified light charged particles (LCPs) has been examined for the 35 MeV/nucleon 70Zn+70Zn, 64Zn+64Zn, and 64Ni+64Ni systems. A large enhancement of the midrapidity yield of the LCPs was observed relative to the yield near the projectile rapidity. In particular, this enhancement was increased for the more neutron-rich LCPs demonstrating a preference for the production of neutron-rich fragments in the midrapidity region. Additionally, the transverse flow of the LCPs was extracted, which provides insight into the average movement of the particles in the midrapidity region. Isotopic and isobaric effects were observed in the transverse flow of the fragments. In both cases, the transverse flow was shown to decrease with an increasing neutron content in the fragments. A clear inverse relationship between the transverse flow and the relative midrapidity yield is shown. The increased relative midrapidity emission produces a decreased transverse flow. The stochastic mean-field model was used for comparison to the experimental data. The results showed that the model was able to reproduce the general isotopic and isobaric trends for the midrapidity emission and transverse flow. The sensitivity of these observables to the density dependence of the symmetry energy was explored. The results indicate that the transverse flow and midrapidity emission of the LCPs are sensitive to the denisty dependence of the symmetry energy.

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  • Received 13 June 2010

DOI:https://doi.org/10.1103/PhysRevC.83.044601

©2011 American Physical Society

Authors & Affiliations

Z. Kohley1,2,*, L. W. May1,2, S. Wuenschel1,2, M. Colonna3, M. Di Toro3,4, M. Zielinska-Pfabe5, K. Hagel2, R. Tripathi2, A. Bonasera2,3, G. A. Souliotis2,6, D. V. Shetty2,†, S. Galanopoulos2, M. Mehlman2,7, 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, INFN, I-95123 Catania, Italy
  • 4Physics and Astronomy Department, University of Catania, Italy
  • 5Smith College, Northampton, Massachusetts, USA
  • 6Laboratory of Physical Chemistry, Department of Chemistry, National and Kapodistrian University of Athens, Athens GR-15771, Greece
  • 7Physics and Astronomy Department, Texas A&M University, College Station, Texas 77843, USA

  • *zkohley@comp.tamu.edu; current address: Physics Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA
  • Current address: Physics Department, Western Michigan University, Kalamazoo, MI 49008, USA

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Vol. 83, Iss. 4 — April 2011

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