Isospin effects on particle emission time sequence in EA=61MeV Ar36+Sn112,124 reactions

R. Ghetti, J. Helgesson, V. Avdeichikov, B. Jakobsson, N. Colonna, and H. W. Wilschut
Phys. Rev. C 70, 034601 – Published 3 September 2004

Abstract

The emission time sequence of neutrons, protons, and deuterons is deduced from velocity-gated two-particle correlation functions in EA=61MeV Ar36+Sn112,124 reactions. A dependence of the emission sequence on the isospin of the emitting source is observed.

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  • Received 29 April 2004

DOI:https://doi.org/10.1103/PhysRevC.70.034601

©2004 American Physical Society

Authors & Affiliations

R. Ghetti1,*, J. Helgesson2, V. Avdeichikov3, B. Jakobsson1, N. Colonna4, and H. W. Wilschut5

  • 1Department of Physics, Lund University, Box 118, S-22100 Lund, Sweden
  • 2School of Technology and Society, Malmö University, S-205 06 Malmö, Sweden
  • 3Joint Institute for Nuclear Research, 141980 Dubna, Russia
  • 4INFN and Dipartimento di Fisica, Via Amendola 173, I-70126 Bari, Italy
  • 5Kernfysisch Versneller Instituut, Zernikelaan 25, NL-9747 AA Groningen, The Netherlands

  • *Corresponding author; Email address: roberta.ghetti@nuclear.lu.se

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Vol. 70, Iss. 3 — September 2004

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