Dissipation and forces in time-dependent Hartree-Fock calculations

P.-G. Reinhard, A. S. Umar, K. T. R. Davies, M. R. Strayer, and S.-J. Lee
Phys. Rev. C 37, 1026 – Published 1 March 1988
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Abstract

We have performed time-dependent Hartree-Fock calculations for the 16O+16O system using various parametrizations of the Skyrme force. These calculations also include the spin-orbit part of the Skyrme force. We have refitted the finite-range version of the Skyrme force to the ground state properties of eight nuclei with improved accuracy. Particular emphasis is given to comparisons of calculations with and without the spin-orbit force. We see a strong sensitivity of the results to the different parametrizations of the effective interaction. The spin-orbit force introduces a significant enhancement of the dissipation. A schematic model of heavy-ion scattering is used to investigate the origin of the observed sensitivity. We find that the dissipation is essentially determined by the additional residual interaction.

  • Received 19 October 1987

DOI:https://doi.org/10.1103/PhysRevC.37.1026

©1988 American Physical Society

Authors & Affiliations

P.-G. Reinhard

  • Joint Institute for Heavy-Ion Research, Oak Ridge, Tennessee 37831

A. S. Umar

  • Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennessee 37235

K. T. R. Davies and M. R. Strayer

  • Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831

S.-J. Lee

  • Department of Physics, McGill University, Montreal, Quebec, Canada H3A 2T8

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Vol. 37, Iss. 3 — March 1988

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