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HAL Id: jpa-00207101

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Submitted on 1 Jan 1971

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Correction coulombienne du facteur de phase en théorie diffractionnelle de la diffusion subcoulombienne

Ch. Leclercq-Willain

To cite this version:

Ch. Leclercq-Willain. Correction coulombienne du facteur de phase en théorie diffrac- tionnelle de la diffusion subcoulombienne. Journal de Physique, 1971, 32 (7), pp.475-482.

�10.1051/jphys:01971003207047500�. �jpa-00207101�

(2)

CORRECTION COULOMBIENNE DU FACTEUR

DE PHASE EN THÉORIE DIFFRACTIONNELLE

DE LA DIFFUSION SUBCOULOMBIENNE

Ch.

LECLERCQ-WILLAIN

Institut Interuniversitaire des Sciences

Nucléaires,

Université Libre de

Bruxelles, Bruxelles, Belgique (Reçu

le 28 janvier 1971)

Résumé. 2014 La méthode

semi-classique

développée en théorie d’excitation coulombienne est utilisée pour définir les sections efficaces différentielles

élastique

et inélastique d’excitation d’un niveau nucléaire vibrationnel à un phonon 03BB, en diffusion subcoulombienne de particules 03B1. L’inter- férence des interactions coulombienne et nucléaire modifie la structure diffractionnelle aux petits angles de diffusion. Les résultats théoriques présentés sont appliqués à l’étude des diffusions élas- tique Ni58 (03B1, 03B1) Ni58 et inélastique Ni58 (03B1, 03B1’) Ni58 avec excitation des niveaux 2+ et 3- du Ni58.

Abstract. 2014 A phase Coulomb correction is introduced in the usual diffractional model to define the differential cross sections for elastic and inelastic subcoulomb 03B1 scattering with excitation of a

vibrational one phonon 03BB nuclear level. The interference of Coulomb and nuclear interactions modifies the diffractional structure at small scattering angles.

Those theoretical results are used to study the elastic scattering Ni58 (03B1, 03B1) Ni58 and the inelastic

one with excitation of 2+ and 3- levels in Ni58.

Classification Physics Abstracts :

12.17, 12.37

1. Introduction. - One of the most

striking

features

of the

scattering

of a

particles,

with an energy E which

exceeds the Coulomb

barrier,

is the

persistence

of

sharp, regularly spaced

oscillations in the

angular

distributions. Such oscillations are a characteristic feature of so-called surface reactions. We assume that the conditions

of

high

incident energy and

for excitation of collective levels in an

absorbing

target nucleus, are fulfilled. In the

expressions (1)

and

(2) ;

t1 = zz’

e21!iv

is the Coulomb

parameter, k

the wave

number of the incident

particle, R

the radius of the nucleus and àE the energy of the excited level.

Then,

in the process of

scattering,

the nucleus can be consi-

dered immovable and the

change

in energy of the

particles

in inelastic

scattering

can be

ignored.

The

adiabatic

approximation

is thus

applicable.

The solu-

tion of the

scattering problem

reduces to

finding

the

scattering amplitude fez2, ç) (3)

of

particles

from a

fixed nucleus

where ç

define the internal

variables,

characteristic of the target

nucleus,

and Ç2 =

(0, rp)

determine the direction of

scattering.

In this case the differential elastic

scattering

cross-

section and the inelastic one for the excitation of a final

level IM

> in the target nucleus are defined

by

different

projections

of the same

scattering amplitude f(Q, ç) (3) :

If condition

(1)

is

fulfilled,

it is

possible

to calculate

the

scattering amplitude (3) using

the diffraction

theory

method

[1 ]-[4]

where k is the wave number of the

outgoing particle.

Integration

is defined in the shadow

plane (p, cp) perpendicular

to the unit vector

in a direction deflected

by 0/2

from the incident beam.

Here,

Q(p)

is the function which accounts for the characteristics of the nucleus and of the elastic and inelastic

scattering potentials [1 ]-[3].

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01971003207047500

(3)

476

We find the differential cross-sections for elastic and inelastic

scattering

with excitation of a vibrational one

phonon A

nuclear level in the field of a nuclear and a

Coulomb

scattering potential.

2.

Sharp

cutoff-model. -

Assuming

that the

scattering potential

is

composed

of a nuclear and a

Coulomb part

the function

Q(p)

can be

split

up into a nuclear and a

Coulomb factor

2.1 THE

NUCLEAR FUNCTION. - The function

Q’(p) accounts

for the characteristics of a black nucleus :

Q’(p)

= 1 on all

planes

Z = const. aside

from the shadow of the nucleus in which the value is 0.

(9) Assuming

that the

equation

of the nuclear sur-

face is

the shadow line is defined

by

2.2 THE COULOMB FUNCTION. - The function

S2°b(p)

accounts for the

charge

effects of the target nucleus

Assuming

that the

charge density

function for the target nucleus is

where

the Coulomb interaction

potential,

for small deforma-

tion parameter aÂ, in the

expression (10),

is

Then,

the

explicit

form of

Qc’(p)

is

2. 3 SCATTERING AMPLITUDE AND CROSS-SECTIONS. -

With the

expressions (5), (9)

and

(15)

the

scattering amplitude f(Q, ç)

is

To find the cross-sections for elastic and inelastic

scattering

we

expand

the

amplitude (16)

into a series

for small deformation parameters which is limited

by

linear

approximation.

We obtain the

following general

expression

for the

scattering amplitude

of

charged particles

from a fixed nucleus whose surface has  vibrations

So the elastic

scattering amplitude

(4)

where the Coulomb

amplitude

is

and the functions

Foo(kRo 0)

is defined in

Appendice

1.

Thus,

the total

amplitude

of elastic

scattering

consists

of the

amplitude

of elastic

scattering

in the electric field of the nucleus and a nuclear part

which,

for the Cou-

lomb parameter il =

0,

is

exactly

the

expression

of

the Blair

sharp

cutoff model

[1].

So,

the elastic differential cross section

splits

into

three terms :

The Coulomb cross section

a nuclear term in Coulomb field

and an interference term

with

With

regard

to the

expression

of the total elastic

cross-section divided

by

the Rutherford cross-section

where

the condition y = 1 defines a limit

scattering angle

For il

>

kRo > 1, 0.

is

large

and the

scattering

fol-

lows the Rutherford law.

For

kRo > q

>

1,

the second term is dominant in the

expression (22)

and the

scattering

has a diffractional structure. For

kRo -- il » 1,

the

scattering

is « Cou-

lomb » for 0

Oo

and « diffractional » for 0 >

00.

Those three

possibilities

are summarized

by

three

experimental

results in

figures 1,

2 and 3.

FIG. 1. - At incident energies lower than the Coulomb barrier, the angular distribution follows the Rutherford law.

The inelastic

scattering amplitude

for excitation

of a one

phonon

vibrational level

is defined

by

the

following expression :

where

(5)

478

FIG. 2. - At incident energies much higher than the Coulomb barrier,

a diffractional theory is applicable to describe the angular distribution.

FIG. 3. - At energies near the Coulomb barrier, the description of the scattering process must take both the Coulomb and

nuclear interactions into account.

So the differential

scattering

cross section is :

and

splits

into three terms

(Appendice 2).

In the linear

approximation

for small deformation parameters of the target

nucleus,

the

angular

distri-

butions for elastic

scattering

on a

spherical

or a non-

spherical

nucleus are the same and the

angular

distri-

butions of inelastic

scattering

with excitation of the first rotational level of a permanent deformed nucleus

are defined

by

the same

expression (17)

with the

dyna-

mic variable aA,

replaced by

(w

shows the orientation of the axes of symmetry of the nucleus and is the permanent deformation

(6)

parameter)

and the

expression (24)

with

flz replaced by

The

general expressions (21), (25)

and

(A 2)

are

applied

to the excitation of a one

phonon A

=

2, 2+

level

[5] [6]

and a one

phonon A

=

3,

3- level

[6].

2.4 RESULTS OF CALCULATION AND COMPARISON WITH EXPERIMENTAL DATA. -

According

to the expres- sions of the

sharp

cutoff Blair model

[1] ]

both the

elastic and inelastic cross-sections measured for

projectiles

of different wave number k should follow

« universal » curves when divided

by k2

and

plotted

versus x = 2

kRo

sin

0/2.

In

figure 4,

a universal curve has been drawn to summarize the oc elastic

scattering experimental

data

on

Ni58

at incident

energies Eo

= 100 MeV

[7],

FIG. 4. - Universal curve of the a elastic scattering experi-

mental data on Ni 5 8 at incident energies of 100, 41 and 33 MeV.

41 and 43 MeV

[8]

and 33 MeV

[7].

Some elastic

data

corresponding to

the

highest energies (100-85 MeV)

are

displayed

at small

angles.

We believe that this may be attributed to the

varying importance

of the

Coulomb corrections to the scattered

amplitude

at

small

angles.

The theoretical universal curves calcu- ted

according

to formula

(21) [narrow

solid curve for

41,

33

MeV,

dashed curve for 100-85

MeV]

and to formula of the

sharp

cutoff Blair model

[1] [large

solid

curve]

have been drawn in

figure

5. As the energy

FIG. 5. - Theoretical universal curves of ce elastic scattering

on Ni 5 8 calculated according to formula (21) (narrow solid

curve for 41 and 33 MeV - dashed curve for 100 and 85 MeV) and to formula of the sharp cutoff B!air model (large solid curve).

FIG. 6. - Experimental and theoretical angular distributions in elastic a scattering on Ni$g at energy of 33 MeV. The results of the sharp cutoff Blair model and of this calculation are

compared.

(7)

480

is

increased,

the Coulomb

complications occuring

at

small

angles

should be reduced and indeed it is seen

that the

high

energy data lie much closer to the Blair

curve than does the universal curve at lower

energies.

Similar

experimental

and theoretical results are

obtained in inelastic

scattering Ni58(OC, a’)

Ni58* 2+

FIG. 7. - Angular distributions of inelastic ce scattering at

33 MeV with excitation of 2+ and 3- levels in Nis 8.

and 3 - levels. In

figure 6,

the

experimental angular

distribution in elastic a

scattering

on

Nis8

at

Eo

= 33 MeV is

compared

to the theoretical curves

calculated

according

to the

sharp

cutoff Blair model

[1]

(dashed curve)

and to the formula

(21)

with Coulomb and nuclear interference effects

(solid curve).

At this

energy, in the

angular

distributions of inelastic scat-

tering

with excitation of 2+ and 3-

levels, (A

2

with = 2 and

3)

the interference of the Coulomb and nuclear interactions modifies the diffractional

structure at small

scattering angles (0 200) (see Fig. 7).

A

sharp

minimum is defined at a

scattering angle

for which the Blair model result is near a

maximum.

3. Smooth Cutoff Model. - In the above

results,

it is seen that the

magnitudes

of the theoretical diffe- rential cross sections

drop

off much too

slowly

with

scattering angles.

Some authors

[9], [10]

have

already pointed

out the

improvement

of the adiabatic nuclear

theory by using

a smooth cutoff

picture.

This rounded cutoff correction is introduced in

assuming

for the

nuclear function

QN(P)

the form

Some results are

developped

with an

optical

surface

nuclear

potential

By

similar

calculations,

we can define the correspon-

ding scattering amplitude f(Q, aÂ,).

At the zero and

first order

approximation

in az., we have :

where and

(8)

This

formalism has been

investigated by

Drozdov

[12]

and

applied by

this author to calculate differential cross-sections

Nis8, Mg24 (p, p’)

at 40 MeV with 2+

and 3 - excitation. The results seem to

depend largely

on the

imaginary

part of the nuclear

potential.

We must note that the

approximate expressions,

obtained

by

Drozdov

display

a difference from the formulas

(28), (29) ;

the last term of

fi being

absent

from the Drozdov

expression.

4. Conclusion. - Elastic and inelastic

scattering

of fast

charged particles

is

investigated

in the diffrac- tion

approximation

in which a Coulomb

phase

correc-

tion has been

partly

introduced.

Indeed,

the

scattering

wave function

is an

approximate expression,

the z

dependence being

characteristic of a

plane

wave.

Perhaps,

it would be

necessary to

develop

a

theory

based on the Coulomb

wave functions and on the Coulomb Green function.

However,

in this case, it seems easier to use a distorted

wave method.

With the smooth cutoff

correction,

the results are the same as those calculated

by

distorted wave

theory [10], [11]

and the agreement with

experiment

is

quite impressive.

The D. W. B. A. is more

general

and

requires

fewer

approximations. However,

when Coulomb interactions have to be taken into account, many

partial

waves have to be considered in the deve-

lopment

of the Coulomb excitation terms ; then the distorted wave method

requires

more

developed

numerical calculations on

big

computers.

So,

this Coulomb and nuclear smooth cutoff model

can be used

successfully

and presents the

advantage

of

simplicity

on the D. W. B. A. method.

Acknowledgements.

- We are

grateful

to Profes-

sor M. Demeur for many useful discussions and fo his constant and

unfailing help

and encouragement

at all times.

We are indebted to the staff of the

Computer

Center

of Brussels

University

for extensive use of their faci- lities.

APPENDICES 1. Function

We use the

multiplication

theorem of Bessel functions

So we obtain

By solving

the

u-integration :

2.

Scattering

differential cross-sections for excitation of a one Â

phonon

level.

(9)

482

where

is defined in

(A 1).

References

[1] BLAIR (J. S.), « Inelastic Excitation of Collective Levels » Lectures on Nuclear Interactions, Herceg- Novi, 1962, VII, 1.

[2] AKHIEZER (A. I.) et SITENKO (A. G.), Phys. Rev., 1957, 106, 1236.

[3] GLAUBER (R. J.), « High-energy Collision Theory »:

Lectures in theoretical Physics, Boulder 1959, ed.

Interscience Publ. Inc., New York, 1959, p. 315.

[4] FESHBACH (H.), Intern. School of Physics « E. Fermi », Varenna Course 38-Academic Press, New York, p. 183.

[5] DROZDOV (S. I.), Soviet Physics JETP, 1959, 36, 1335.

[6] LECLERCQ-WILLAIN (C.), « Etude théorique de l’inter- férence des excitations coulombienne et nucléaire », Thèse Bruxelles.

[7] MERIWETHER (J. R.), BUSSIERE DE NERCY (A.) et

HARVEY (B. G.), Phys. Lett., 1964, 11, 299.

[8] BROEK (H. W.), YNTEMA (J. L.), BUCH (B.) et SATCH-

LER (G. R.), Nucl. Phys., 1965, 64, 259 ; Mc DANIELS (D. K.), BLAIR (J. S.), CHEW (S. W.) et

FARWELL (G. W.), Nucl. Phys., 1960, 17, 614.

[9] BLAIR (J. S.), SHARP (D.) et WILETS (L.), Phys. Rev., 1962, 125, 1625.

[10] RosT (E.), Phys. Rev., 1962, 128, 2708.

[11] BASSEL (R. H.), SATCHLER (G. R.), DRISKO (R. M.) et

RosT (E.), Phys. Rev., 1962, 128, 2693.

[12] DROZDOV (S. I.), Proc. of Conf. on « Direct Interac- tions and Reaction Mechanisms », Padua 1962, Gordon and Breach Science Publ., New York,

p. 799.

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