Medium-mass nuclei with Δ excitations under compression

Mahmoud A. Hasan, James P. Vary, and T.-S. H. Lee
Phys. Rev. C 64, 024306 – Published 2 July 2001
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Abstract

The ground state properties of 90Zr, 100Sn, and 132Sn at equilibrium and at large amplitude compression are investigated. We use a realistic effective baryon-baryon Hamiltonian that includes NN, NΔ, and ΔΔ interactions. We perform the calculations in no-core model spaces within the framework of the constrained spherical Hartree-Fock approximation. We specifically investigate the sensitivity to the sizes of the nucleon and Δ model spaces. At equilibrium, we find no case of mixing between nucleons and Δs in our largest model space of eight major nucleon shells plus 16 Δ orbitals. On the contrary, there is mixing in 90Zr, and 132Sn in the smaller model space of seven major nucleon shells plus eight Δ orbitals. Expanding the nucleon model space has a larger effect on reducing the static compression modulus and softening the nuclear equation of state than increasing the number of Δ states. Most of the excitation energy delivered to the system during compression is employed by two nuclei with a neutron excess (i.e., 90Zr, 132Sn) to create massive Δ resonances. On the other hand, in the 100Sn nucleus most of the excitation energy goes to a simple reduction in the binding, suggesting a suppressed role for the Δ states. Under extreme compression, at a density 2–3 times the normal nuclear density, the excitation of nucleons to Δs increases sharply up to 10% of the total number of constituents. At fixed excitation energy under compression, the number of Δ excitations is not dependent on the number of Δ states over the range studied. The Δ-excitation results are consistent with heavy-ion collision data, and suggest an important mean field mechanism for subthreshold pion production in particle-nucleus and nucleus-nucleus collisions.

  • Received 16 January 2001

DOI:https://doi.org/10.1103/PhysRevC.64.024306

©2001 American Physical Society

Authors & Affiliations

Mahmoud A. Hasan1,2, James P. Vary2,3, and T.-S. H. Lee4

  • 1Applied Science University, Amman, Jordan
  • 2International Institute of Theoretical and Applied Physics, Ames, Iowa 50011
  • 3Department of Physics and Astronomy, Iowa State University, Ames, Iowa 50011
  • 4Physics Division, Argonne National Laboratory, Argonne, Illinois 60439

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Vol. 64, Iss. 2 — August 2001

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