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Constraints for the scalar-isovector channel

Validity of the CE for the scalar-isovector density, Eq. (30) for $v=0$ and $t=1$, imposes through Eq. (48) certain specific constraints on the coupling constants of the functional. At second order we obtain,

$\displaystyle C_{00,2000}^{0000,t}$ $\textstyle =$ $\displaystyle -\frac{3^t}{\sqrt{3}}C_{00,1101}^{1101,1-t},$ (53)
$\displaystyle C_{00,1110}^{1110,t}$ $\textstyle =$ $\displaystyle -\frac{3^t}{3\sqrt{3}}C_{00,2011}^{0011,1-t}-\frac{3^t}{3}\sqrt{\frac{5}{3}}C_{00,2211}^{0011,1-t},$ (54)
$\displaystyle C_{00,1111}^{1111,t}$ $\textstyle =$ $\displaystyle -\frac{3^t}{3}C_{00,2011}^{0011,1-t}+\frac{3^t}{6}\sqrt{5}C_{00,2211}^{0011,1-t},$ (55)
$\displaystyle C_{00,1112}^{1112,t}$ $\textstyle =$ $\displaystyle -\frac{3^t}{3}\sqrt{\frac{5}{3}}C_{00,2011}^{0011,1-t}-\frac{3^t}{6\sqrt{3}}C_{00,2211}^{0011,1-t},$ (56)
$\displaystyle C_{11,1111}^{0000,t}$ $\textstyle =$ $\displaystyle C_{11,0011}^{1101,t} = 0 ,$ (57)
$\displaystyle C_{20,0000}^{0000,1}$ $\textstyle =$ $\displaystyle C_{20,0011}^{0011,1} =
C_{22,0011}^{0011,1} = 0 .$ (58)

Constraints in Eqs. (53)-(56) connect the isoscalar and isovector coupling constants. The numerical coefficients of the corresponding linear combinations are the same as those for the scalar-isoscalar CE, see Eqs. (C1)-(C4) of Ref. [Carlsson et al.(2008)Carlsson, Dobaczewski, and Kortelainen], apart from factors of $\sqrt{3}$ explained before Eq. (36). However, conditions for the scalar-isoscalar CE keep the coupling constants in the two isospin channels disconnected. Moreover, in the scalar-isovector channel the spin-orbit coupling constants must vanish, Eq. (57), along with the isovector surface coupling constants, Eq. (58). On the other hand, the corresponding isoscalar surface coupling constants, $C_{20,0000}^{0000,0}$, $C_{20,0011}^{0011,0}$, and $C_{22,0011}^{0011,0}$, are left unrestricted.

For the fourth and sixth orders, analogous constraints are presented in Appendix A.


next up previous
Next: Constraints for the vector-isoscalar Up: Continuity equations in the Previous: Constraints for the scalar-isoscalar
Jacek Dobaczewski 2011-11-11