Delineating effects of tensor force on the density dependence of nuclear symmetry energy
arXiv:1207.1639 · doi:10.1088/1742-6596/420/1/012090
Abstract
In this talk, we report results of our recent studies to delineate effects of the tensor force on the density dependence of nuclear symmetry energy within phenomenological models. The tensor force active in the isosinglet neutron-proton interaction channel leads to appreciable depletion/population of nucleons below/above the Fermi surface in the single-nucleon momentum distribution in cold symmetric nuclear matter (SNM). We found that as a consequence of the high momentum tail in SNM the kinetic part of the symmetry energy is significantly below the well-known Fermi gas model prediction of approximately . With about 15% nucleons in the high momentum tail as indicated by the recent experiments at J-Lab by the CLAS Collaboration, the is negligibly small. It even becomes negative when more nucleons are in the high momentum tail in SNM. These features have recently been confirmed by three independent studies based on the state-of-the-art microscopic nuclear many-body theories. In addition, we also estimate the second-order tensor force contribution to the potential part of the symmetry energy. Implications of these findings in extracting information about nuclear symmetry energy from nuclear reactions are discussed briefly.
Talk given by Chang Xu at the 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012. To appear in the NN2012 Proceedings in Journal of Physics: Conference Series (JPCS)
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- Probing the high-density behavior of symmetry energy with gravitational waves
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- Finite particle-number description of symmetric nuclear matter with spin excitations of high-momentum pairs induced by tensor force
- Experimental Study of Bremsstrahlung Gamma Ray Emission and Short-Range Correlations in Sn+Sn Collisions at 25 MeV/u