Anatomy of symmetry energy of dilute nuclear matter
arXiv:1009.4523 · doi:10.1103/PhysRevC.82.045201
Abstract
The symmetry energy coefficients of dilute clusterized nuclear matter are evaluated in the -matrix framework. Employing a few different definitions commonly used in the literature for uniform nuclear matter, it is seen that the different definitions lead to perceptibly different results for the symmetry coefficients for dilute nuclear matter. They are found to be higher compared to those obtained for uniform matter in the low density domain. The calculated results are in reasonable consonance with those extracted recently from experimental data.
11 pages, 9 figures, Accepted in Phys. Rev. C
References in corpus (10)
- Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
- Symmetry energy of dilute warm nuclear matter
- Experimental determination of the symmetry energy of a low density nuclear gas
- Non-rotating and rotating neutron stars in the extended field theoretical model
- Asymmetric nuclear matter and neutron-skin in extended relativistic mean field model
- Temperature effects on the nuclear symmetry energy and symmetry free energy with an isospin and momentum dependent interaction
- S-matrix approach to equation of state of nuclear matter
- Symmetry coefficients and incompressibility of clusterized supernova matter
- Nuclear condensation and symmetry energy of dilute nuclear matter: an S-matrix approach
- The efficacy of isotope thermometry: examining in the S-matrix approach