Isotopic scaling of heavy projectile residues from the collisions of 25MeV/nucleon86Kr with 124Sn, 112Sn and 64Ni, 58Ni

G. A. Souliotis, D. V. Shetty, M. Veselsky, G. Chubarian, L. Trache, A. Keksis, E. Martin, and S. J. Yennello
Phys. Rev. C 68, 024605 – Published 25 August 2003
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Abstract

The scaling of the yields of heavy projectile residues from the reactions of 25MeV/nucleon86Kr projectiles with 124Sn, 112Sn and 64Ni, 58Ni targets is studied. Isotopically resolved yield distributions of projectile fragments in the range Z=1036 from these reaction pairs were measured with the MARS recoil separator in the angular range 2.7°5.4°. For these deep inelastic collisions, the velocities of the residues, monotonically decreasing with Z down to Z2628, are employed to characterize the excitation energy. The ratios R21(N,Z) of the yields of a given fragment (N,Z) from each pair of systems are found to exhibit isotopic scaling (isoscaling), namely, an exponential dependence on the fragment atomic number Z and neutron number N. The isoscaling is found to occur in the residue Z range corresponding to the maximum observed excitation energies. The corresponding isoscaling parameters are α=0.43 and β=0.50 for the Kr+Sn system and α=0.27 and β=0.34 for the Kr+Ni system. For the Kr+Sn system, for which the experimental angular acceptance range lies inside the grazing angle, isoscaling was found to occur for Z<~26 and N<~34. For heavier fragments from Kr+Sn, the parameters vary monotonically, α decreasing with Z and β increasing with N. This variation is found to be related to the evolution towards isospin equilibration and, as such, it can serve as a tracer of the N/Z equilibration process. The present heavy-residue data extend the observation of isotopic scaling from the intermediate mass fragment region to the heavy-residue region. Interestingly, such high-resolution mass spectrometric data can provide important information on the role of isospin and isospin equilibration in peripheral and midperipheral collisions, complementary to that accessible from modern large-acceptance multidetector devices.

  • Received 8 May 2003

DOI:https://doi.org/10.1103/PhysRevC.68.024605

©2003 American Physical Society

Authors & Affiliations

G. A. Souliotis, D. V. Shetty, M. Veselsky*, G. Chubarian, L. Trache, A. Keksis, E. Martin, and S. J. Yennello

  • Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA

  • *On leave from the Institute of Physics of the Slovak Academy of Sciences, Bratislava, Slovakia.

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Vol. 68, Iss. 2 — August 2003

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