Chapter Two
MICROSCOPIC
OPTICAL MODEL
All microscopic optical models of NA
scattering that have been developed so far, depend on a (model) prescription of
basic interactions between nucleons. Consequently, to date there is no theory
of such scattering as exact or reliable as exists for electromagnetic scattering.
Nevertheless the full-folding microscopic optical model has reached a very successful stage. In this
review chapter some of the essential details of the developing process of the
full folding coordinate space optical potentials, and of the input to the
codes that have been used in the calculations, are reported briefly. All the
relevant details have been given in much fuller form in a review [7].
Formal theory of the
nucleon--nucleus optical potential
In the optical model approach, the many-nucleon-problem is reduced
to one for a single particle with the kinetic energy being that of the projectile.
The optical potential accounts effectively for all of the complexity
of scattering in the many body system. Note that as the term generalized optical model includes more than solely entrance channel
phenomena, my use of the term optical potential is to be taken to mean
the single elastic channel reduction.
The Feshbach formalism [39, 40] is a convenient
device to use. One divides the Hilbert space of the A+1 scattering system using two
projection operators P and Q. P projects onto the elastic
channel and Q on to all others.
Thus P + Q = 1, PQ = QP = 0 and
With these projection operators, and
with HPQ = HQP etc., the Schrodinger equation segments as
Using the second equation to eliminate
from
the first gives
where outgoing wave boundary conditions
are assumed. The Feshbach formalism reduces the many nucleon problem to an effective
one body one by invoking explicitly the ground state and the influence of
transitions to other channels from the ground state, with
The single nucleon distorted wave
for elastic scattering is thus defined. This optical potential is complex as the intermediate state propagator
is complex (due to pole contributions).
It contains the whole complex spectrum of many body excitations of the
projectile and target nucleons in bound as well as in continuum states, with
Thus
the optical potential is identified by
In general it is nonlocal, and energy dependent as well as
being complex due to the second term.
With a local V, the leading term is real, local, and energy
independent. That is so provided antisymmetrization is ignored. Multiple
scattering effects are contained within the second term.
But this concentration of all multiple
scattering effects in the second term is largely ineffective since realistic NN
potentials are short ranged and multiple scattering may be significant.
Treating such explicitly is the leading
idea behind the Chew [10] and Watson [11] multiple
scattering theory. They replace the
potential in Eq. (2.4) by the complex NN t matrix. As a result,
the leading term is now complex, nonlocal, and energy dependent. In the simplest versions it is assumed that
only pairwise interactions between the projectile and target nucleons are
important. With the projectile tagged 0, and target nucleons tagged i,
Furthermore, the NN t
matrices are associated with the Lippmann-Schwinger (LS) equation
while the NN g matrices which will be used in the current
approach are associated with the Brueckner--Bethe--Goldstone
(BBG) equation
Here
differs
from the free NN propagator
by
including medium effects such as Pauli blocking and a mean field. When such t and g matrices replace V in Eq. (2.4)
the formulations of the
microscopic optical models are in the spirit of KMT [14]. Adhikari and
Kowalski [15] define auxiliary operators that
are useful in this development, such as
and
with which a modified pA T matrix
is defined by
The
Feshbach subtraction technique then yields
and
The optical potential itself then is the expectation value taken
with the wave function attributes of the ith nucleon in the target. It is still a many-nucleon problem as
evaluation requires knowledge of the excitation spectrum of the target.
In a lowest order model, the complexity
of the problem is reduced to a weighted sum of one nucleon expectation
values. The weights, to first order, are
the shell occupancy numbers. The
resultant optical potential is still complex but that is now due to the
complex nature of the g matrix rather than because of higher order terms
in the expansion of Eq. (2.12).
Neglecting medium effects in the g matrix defines the t matrix approximation.
If in addition, the antisymmetrization of the projectile and target
nucleon wave function is ignored one has a very simplified fully off-shell tr approximation.
As will be developed subsequently, the
zero angular momentum transfer I=0 component of the optical potential will be used in specifying radial Schrodinger
equations whose solutions are the distorted waves. There are also
amplitudes
contributing to elastic scattering from non--zero spin targets. They may yield
re--orientation amplitudes even though, generally, they are small in comparison
to the I=0 ones. A practical
means of evaluation of the relevant
scattering amplitudes uses the distorted wave approximation.
scattering amplitudes uses the distorted wave approximation.
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