Critical densities for the Skyrme type effective interactions

Details Critical densities for the Skyrme type effective interactions Critical densities for the Skyrme type effective interactions

2004-09-23

arxiv.org/abs/nucl-th/0409053v1

Phys.Rev. C70 (2004) 057302

Physics

Nuclear Physics

Nuclear Theory

10 pages, 3 figures. Physicsl Review C (in press)

Scientific paper

10.1103/PhysRevC.70.057302

We use the stability conditions of the Landau parameters for the symmetric nuclear matter and pure neutron matter to calculate the critical densities for the Skyrme type effective nucleon-nucleon interactions. We find that the critical density can be maximized by adjusting appropriately the values of the enhancement factor $\kappa$ associated with isovector giant dipole resonance, the quantity $L$ which is directly related to the slope of the symmetry energy and the Landau parameter $G_0^\prime$. However, restricting $\kappa$, $L$ and $G_0^\prime$ to vary within acceptable limits reduces the maximum value for the critical density $\tilde\rho_{cr}$ by $\sim 25%$. We also show that among the various quantities characterizing the symmetric nuclear matter, $\tilde\rho_{cr}$ depends strongly on the isoscalar effective mass $m^*/m$ and surface energy coefficient $E_s$. For realistic values of $m^*/m$ and $E_s$ we get $\tilde\rho_{cr} = 2\rho_0$ to $ 3\rho_0$ ($\rho_0 = 0.16$fm$^{-3}$).

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