Projectile fragmentation of radioactive beams of Ni68, Cu69, and Zn72

S. Lukyanov, M. Mocko, L. Andronenko, M. Andronenko, D. Bazin, M. A. Famiano, A. Gade, S. P. Lobastov, W. G. Lynch, A. M. Rogers, O. B. Tarasov, M. B. Tsang, G. Verde, M. S. Wallace, and R. G. T. Zegers
Phys. Rev. C 80, 014609 – Published 14 July 2009

Abstract

The fragment production cross sections of secondary neutron-rich beams of Ni68, Cu69, and Zn72 isotopes at energies of about 95A MeV have been measured. We compare the measured cross sections to EPAX, an empirical parametrization of fragmentation cross sections. A reasonable agreement of the experimental data and EPAX predictions suggests that an EPAX parametrization used for stable beams seems to be valid for unstable neutron-rich ion beams. EPAX tends to overestimate the yields of neutron-rich isotopes. This problem is amplified when neutron-rich radioactive beams are employed, leading to overly optimistic estimates of the production of neutron-rich isotopes.

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  • Received 21 April 2009

DOI:https://doi.org/10.1103/PhysRevC.80.014609

©2009 American Physical Society

Authors & Affiliations

S. Lukyanov1,2,*, M. Mocko1,3,4, L. Andronenko1,5, M. Andronenko1,5,†, D. Bazin1, M. A. Famiano1,6, A. Gade1, S. P. Lobastov1,2, W. G. Lynch1,4, A. M. Rogers1,4, O. B. Tarasov1,2, M. B. Tsang1,4, G. Verde1,7, M. S. Wallace1,3, and R. G. T. Zegers1,4

  • 1National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA
  • 2Flerov Laboratory of Nuclear Reactions, Joint Institute for Nuclear Research, RU-141980 Dubna, Moscow region, Russian Federation
  • 3Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 4Department of Physics & Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
  • 5PNPI, Gatchina, Leningrad district RU-188300, Russian Federation
  • 6Department of Physics, Western Michigan University, Kalamazoo, Michigan 49008, USA
  • 7INFN, Sezione di Catania, 64 Via Santa Sofia, I-95123 Catania, Italy

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Vol. 80, Iss. 1 — July 2009

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