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Next: Mean-field calculations with tensor Up: Tensor densities in the Previous: Spin-orbit and tensor forces

Spin-orbit and tensor energy densities

Within the energy-density approach, one does not relate the EDF to an average of the two-body force, but one postulates the EDF based on symmetry conditions only. Then, the most general EDF, depending on the spin-current densities, reads[4]

\begin{displaymath}
\begin{array}{rcl}
{\mathcal H}_{SO} &=&
\sum_{t=0,1}
C_{t}...
...
+ C_{t}^{J2} \underline{\mathsf J}_{t}^{2}\Big) ,
\end{array}\end{displaymath} (5)

where the spherical-symmetry condition has been released. The standard pseudoscalar $\underline{{J}}_{t}$, vector $\mbox{\boldmath${J}$\unboldmath }_{t}$, and pseudotensor $\underline{\mathsf J}_{t}$ parts of the spin-current density,[16]
\begin{displaymath}
\begin{array}{rcl}
J_{abt}
&=&{\textstyle{\frac{1}{2i}}}\Big...
...boldmath }=\mbox{\boldmath${r}$\unboldmath }'}, \\
\end{array}\end{displaymath} (6)

are defined as
\begin{displaymath}
\begin{array}{rcl}
\underline{{J}}_{t}&=&
\sum_{a=x,y,z}{J}_...
...style{\frac{1}{3}}} \underline{{J}}_{t}\delta_{ab}.
\end{array}\end{displaymath} (7)

The tensor energy density ${\mathcal H}_T$ now depends on six coupling constants, $C_{t}^{J0}$, $C_{t}^{J1}$, and $C_{t}^{J2}$, for $t$=0,1, and not on two coupling constants, $t_e$ and $t_o$, as in Eq. 3. Similarly, the SO energy density ${\mathcal H}_{SO}$ depends now on two coupling constants $C_{t}^{\nabla {J}}$ for $t$=0,1, and not on one, $W_0$, (the latter generalization has been introduced and studied in Ref.[17]).

From the symmetry conditions imposed by the spherical, axial, and reflection symmetries one obtains[18] that:

1$^\circ$
The pseudoscalar densities $\underline{{J}}_{t}$ vanish unless the axial or reflection symmetries are broken.
2$^\circ$
The pseudotensor densities $\underline{\mathsf J}_{t}$ vanish unless the spherical symmetry is broken.
Finally, the gauge-invariance symmetry conditions[4] require that there are only two gauge-invariant combinations of the pseudoscalar, vector, and pseudotensor terms, namely,
\begin{displaymath}
\begin{array}{rcl}
G^{T}_t&=& {\textstyle{\frac{1}{3}}} \und...
...tstyle{\frac{1}{2}}}\underline{{\mathsf J}}_t^{2} .
\end{array}\end{displaymath} (8)

In such a case, only four out of the six tensor coupling constants are linearly independent, i.e.,
\begin{displaymath}
\begin{array}{rcl}
C_t^{J0 } &=& {\textstyle{\frac{1}{3}}} A...
...2 } &=& ~ A_t + {\textstyle{\frac{1}{2}}} B_t . \\
\end{array}\end{displaymath} (9)

On the other hand, the averaging of the tensor forces (1) implies that only two out of the six tensor coupling constants remain linearly independent, i.e.,
\begin{displaymath}
\begin{array}{rcl}
B_0 &=& -3 A_0 = - {\textstyle{\frac{3}{8...
...textstyle{\frac{3}{8}}} \left(t_e- t_o\right) . \\
\end{array}\end{displaymath} (10)


next up previous
Next: Mean-field calculations with tensor Up: Tensor densities in the Previous: Spin-orbit and tensor forces
Jacek Dobaczewski 2006-04-22