HAL Id: jpa-00207101
https://hal.archives-ouvertes.fr/jpa-00207101
Submitted on 1 Jan 1971
HAL
is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire
HAL, estdestinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d’enseignement et de recherche français ou étrangers, des laboratoires publics ou privés.
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�
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 différentiellesélastique
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
featuresof the
scattering
of aparticles,
with an energy E whichexceeds the Coulomb
barrier,
is thepersistence
ofsharp, regularly spaced
oscillations in theangular
distributions. Such oscillations are a characteristic feature of so-called surface reactions. We assume that the conditions
of
high
incident energy andfor excitation of collective levels in an
absorbing
target nucleus, are fulfilled. In theexpressions (1)
and(2) ;
t1 = zz’
e21!iv
is the Coulombparameter, k
the wavenumber 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 theparticles
in inelasticscattering
can beignored.
Theadiabatic
approximation
is thusapplicable.
The solu-tion of the
scattering problem
reduces tofinding
thescattering amplitude fez2, ç) (3)
ofparticles
from afixed nucleus
where ç
define the internalvariables,
characteristic of the targetnucleus,
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 definedby
different
projections
of the samescattering amplitude f(Q, ç) (3) :
If condition
(1)
isfulfilled,
it ispossible
to calculatethe
scattering amplitude (3) using
the diffractiontheory
method[1 ]-[4]
where k is the wave number of the
outgoing particle.
Integration
is defined in the shadowplane (p, cp) perpendicular
to the unit vectorin 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 inelasticscattering potentials [1 ]-[3].
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01971003207047500
476
We find the differential cross-sections for elastic and inelastic
scattering
with excitation of a vibrational onephonon A
nuclear level in the field of a nuclear and aCoulomb
scattering potential.
2.
Sharp
cutoff-model. -Assuming
that thescattering potential
iscomposed
of a nuclear and aCoulomb part
the function
Q(p)
can besplit
up into a nuclear and aCoulomb factor
2.1 THE
NUCLEAR FUNCTION. - The functionQ’(p) accounts
for the characteristics of a black nucleus :Q’(p)
= 1 on allplanes
Z = const. asidefrom the shadow of the nucleus in which the value is 0.
(9) Assuming
that theequation
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 nucleusAssuming
that thecharge density
function for the target nucleus iswhere
the Coulomb interaction
potential,
for small deforma-tion parameter aÂ, in the
expression (10),
isThen,
theexplicit
form ofQc’(p)
is2. 3 SCATTERING AMPLITUDE AND CROSS-SECTIONS. -
With the
expressions (5), (9)
and(15)
thescattering amplitude f(Q, ç)
isTo find the cross-sections for elastic and inelastic
scattering
weexpand
theamplitude (16)
into a seriesfor small deformation parameters which is limited
by
linear
approximation.
We obtain thefollowing general
expression
for thescattering amplitude
ofcharged particles
from a fixed nucleus whose surface has  vibrationsSo the elastic
scattering amplitude
where the Coulomb
amplitude
isand the functions
Foo(kRo 0)
is defined inAppendice
1.Thus,
the totalamplitude
of elasticscattering
consistsof the
amplitude
of elasticscattering
in the electric field of the nucleus and a nuclear partwhich,
for the Cou-lomb parameter il =
0,
isexactly
theexpression
ofthe Blair
sharp
cutoff model[1].
So,
the elastic differential cross sectionsplits
intothree terms :
The Coulomb cross section
a nuclear term in Coulomb field
and an interference term
with
With
regard
to theexpression
of the total elasticcross-section divided
by
the Rutherford cross-sectionwhere
the condition y = 1 defines a limit
scattering angle
For il
>kRo > 1, 0.
islarge
and thescattering
fol-lows the Rutherford law.
For
kRo > q
>1,
the second term is dominant in theexpression (22)
and thescattering
has a diffractional structure. ForkRo -- il » 1,
thescattering
is « Cou-lomb » for 0
Oo
and « diffractional » for 0 >00.
Those three
possibilities
are summarizedby
threeexperimental
results infigures 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 excitationof a one
phonon
vibrational levelis defined
by
thefollowing expression :
where
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 targetnucleus,
theangular
distri-butions for elastic
scattering
on aspherical
or a non-spherical
nucleus are the same and theangular
distri-butions of inelastic
scattering
with excitation of the first rotational level of a permanent deformed nucleusare defined
by
the sameexpression (17)
with thedyna-
mic variable aA,
replaced by
(w
shows the orientation of the axes of symmetry of the nucleus and a is the permanent deformationparameter)
and theexpression (24)
withflz replaced by
The
general expressions (21), (25)
and(A 2)
areapplied
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 thesharp
cutoff Blair model[1] ]
both theelastic and inelastic cross-sections measured for
projectiles
of different wave number k should follow« universal » curves when divided
by k2
andplotted
versus x = 2
kRo
sin0/2.
In
figure 4,
a universal curve has been drawn to summarize the oc elasticscattering experimental
dataon
Ni58
at incidentenergies 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 elasticdata
corresponding to
thehighest energies (100-85 MeV)
are
displayed
at smallangles.
We believe that this may be attributed to thevarying importance
of theCoulomb corrections to the scattered
amplitude
atsmall
angles.
The theoretical universal curves calcu- tedaccording
to formula(21) [narrow
solid curve for41,
33MeV,
dashed curve for 100-85MeV]
and to formula of thesharp
cutoff Blair model[1] [large
solid
curve]
have been drawn infigure
5. As the energyFIG. 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.
480
is
increased,
the Coulombcomplications occuring
atsmall
angles
should be reduced and indeed it is seenthat the
high
energy data lie much closer to the Blaircurve than does the universal curve at lower
energies.
Similar
experimental
and theoretical results areobtained 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,
theexperimental angular
distribution in elastic a
scattering
onNis8
atEo
= 33 MeV iscompared
to the theoretical curvescalculated
according
to thesharp
cutoff Blair model[1]
(dashed curve)
and to the formula(21)
with Coulomb and nuclear interference effects(solid curve).
At thisenergy, in the
angular
distributions of inelastic scat-tering
with excitation of 2+ and 3-levels, (A
2with = 2 and
3)
the interference of the Coulomb and nuclear interactions modifies the diffractionalstructure at small
scattering angles (0 200) (see Fig. 7).
Asharp
minimum is defined at ascattering angle
for which the Blair model result is near amaximum.
3. Smooth Cutoff Model. - In the above
results,
it is seen that themagnitudes
of the theoretical diffe- rential cross sectionsdrop
off much tooslowly
withscattering angles.
Some authors[9], [10]
havealready pointed
out theimprovement
of the adiabatic nucleartheory by using
a smooth cutoffpicture.
This rounded cutoff correction is introduced inassuming
for thenuclear function
QN(P)
the formSome results are
developped
with anoptical
surfacenuclear
potential
By
similarcalculations,
we can define the correspon-ding scattering amplitude f(Q, aÂ,).
At the zero andfirst order
approximation
in az., we have :where and
This
formalism has beeninvestigated by
Drozdov[12]
and
applied by
this author to calculate differential cross-sectionsNis8, Mg24 (p, p’)
at 40 MeV with 2+and 3 - excitation. The results seem to
depend largely
on the
imaginary
part of the nuclearpotential.
We must note that the
approximate expressions,
obtained
by
Drozdovdisplay
a difference from the formulas(28), (29) ;
the last term offi being
absentfrom the Drozdov
expression.
4. Conclusion. - Elastic and inelastic
scattering
of fast
charged particles
isinvestigated
in the diffrac- tionapproximation
in which a Coulombphase
correc-tion has been
partly
introduced.Indeed,
thescattering
wave function
is an
approximate expression,
the zdependence being
characteristic of a
plane
wave.Perhaps,
it would benecessary to
develop
atheory
based on the Coulombwave functions and on the Coulomb Green function.
However,
in this case, it seems easier to use a distortedwave method.
With the smooth cutoff
correction,
the results are the same as those calculatedby
distorted wavetheory [10], [11]
and the agreement withexperiment
is
quite impressive.
The D. W. B. A. is moregeneral
and
requires
fewerapproximations. However,
when Coulomb interactions have to be taken into account, manypartial
waves have to be considered in the deve-lopment
of the Coulomb excitation terms ; then the distorted wave methodrequires
moredeveloped
numerical calculations on
big
computers.So,
this Coulomb and nuclear smooth cutoff modelcan be used
successfully
and presents theadvantage
of
simplicity
on the D. W. B. A. method.Acknowledgements.
- We aregrateful
to Profes-sor M. Demeur for many useful discussions and fo his constant and
unfailing help
and encouragementat all times.
We are indebted to the staff of the
Computer
Centerof Brussels
University
for extensive use of their faci- lities.APPENDICES 1. Function
We use the
multiplication
theorem of Bessel functionsSo we obtain
By solving
theu-integration :
2.
Scattering
differential cross-sections for excitation of a one Âphonon
level.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.