This effect is well known both in the MF and
particle-vibration-coupling approaches. Within a deformed MF theory
(with the time-odd mean fields neglected), it corresponds to a
simple fact that the s.p. energies (eigen-energies in a deformed
potential) depend on the deformation in specific way, which is
visualized by the standard Nilsson diagram [1]. Indeed, in an axially
deformed potential, a spherical multiplet of angular momentum
splits into
orbitals according to moduli of the
angular-momentum projections
. Unless
, for prolate
and oblate deformations, orbitals with
decrease and increase
in energy, respectively, while those with maximum
behave in an
opposite way. Therefore, both for prolate and oblate deformations,
and for
, the lowest orbitals have the energies that are
lower than those at the spherical point. Hence, a
particle
added to a doubly-magic core always polarizes the core in such a
way that the total energy decreases. On the other hand, the energy of
a
orbital does not depend on deformation (in the first
order), and thus such an orbital does not exert any shape
polarization (in this order).
Exactly the same result is obtained in a particle-vibration-coupling
model, in which a particle can be coupled with either
0
or 2
state of the core,
or
, and the repulsion of these two configurations
decreases the energy of the ground state with respect to the unperturbed
spherical configuration
. As before, for
, the
configuration
does not exist, and the ground state
is not lowered.
The above reasoning can be repeated for hole states, with the result
that the holes added to the doubly-magic core always
polarize the core in such a way that the total energy also
decreases. As a consequence, the shape polarization effect decreases
the s.p. energies of particle states (21) and increases
those of hole states (22), and thus decreases the shell gap
(24). This effect is clearly illustrated in Fig. 1.