Abstract
The ground state properties of and at equilibrium and at large amplitude compression are investigated. We use a realistic effective baryon-baryon Hamiltonian that includes and 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 model spaces. At equilibrium, we find no case of mixing between nucleons and in our largest model space of eight major nucleon shells plus 16 orbitals. On the contrary, there is mixing in and in the smaller model space of seven major nucleon shells plus eight 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 states. Most of the excitation energy delivered to the system during compression is employed by two nuclei with a neutron excess (i.e., to create massive resonances. On the other hand, in the nucleus most of the excitation energy goes to a simple reduction in the binding, suggesting a suppressed role for the states. Under extreme compression, at a density 2–3 times the normal nuclear density, the excitation of nucleons to increases sharply up to 10% of the total number of constituents. At fixed excitation energy under compression, the number of excitations is not dependent on the number of states over the range studied. The -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