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Resonant behaviour in the interaction of the 12C + 12C system at energies above the coulomb barrier
Z. Basrak, F. Auger, B. Fernandez, J. Gastebois, N. Cindro
To cite this version:
Z. Basrak, F. Auger, B. Fernandez, J. Gastebois, N. Cindro. Resonant behaviour in the interaction
of the 12C + 12C system at energies above the coulomb barrier. Journal de Physique Lettres, Edp
sciences, 1976, 37 (6), pp.131-134. �10.1051/jphyslet:01976003706013100�. �jpa-00231256�
RESONANT BEHAVIOUR IN THE INTERACTION OF THE 12C
+12C
SYSTEM AT ENERGIES ABOVE THE COULOMB BARRIER
Z. BASRAK
Institut «
Rudjer-Boskovic
»,Zagreb, Yugoslavia
and
Département
dePhysique Nucléaire,
C.E.N.Saclay,
B.P.2,
91190Gif-sur-Yvette,
FranceF.
AUGER,
B.FERNANDEZ,
J. GASTEBOISDépartement
dePhysique Nucléaire,
C.E.N.Saclay,
B.P.2,
91190
Gif-sur-Yvette,
France andN. CINDRO
(*)
Service de
Physique Nucléaire,
C.E.N.Bruyères-le-Châtel,
92120
Montrouge,
France(Reçu
le27 janvier 1976,
revise le 17 mars1976, accepté
le 6 avril1976)
.Résumé. 2014 Des résonances ont été observées dans l’interaction 12C + 12C aux énergies Ecm = 7,45, 8,45, 8,85 et 9,25 MeV qui
correspondent
aux énergies d’excitation de24Mg
de 21,4, 22,4, 22,8 et 23,2 MeVrespectivement.
Ces résonances sont visibles dans les voies de sortie protonet
particules
alpha. Dans cette région d’énergie, des résonances dans le système 12C + 12C n’avaientpas encore été observées alors que des calculs théoriques prévoyaient 1’existence d’un groupe de résonances autour de Ecm = 7,6 MeV.
Abstract. 2014 Resonances in the 12C + 12C interaction at Ecm = 7.45, 8.45, 8.85 and 9.25 MeV
corresponding
to excitation energies in24Mg
of 21.4, 22.4, 22.8 and 23.2 MeVrespectively
arereported.
These resonances are seen in theproton
andalpha
exit channels. No resonances in 12C + 12C were reported previously in this energyregion,
where earlier calculations predicted agroup around Ecm = 7.6 MeV.
Classification Physics Abstracts
4.310 - 4.375
Since the
discovery
fifteen years ago[1]
of the threeresonances in
12C
+12C
nearEern
= 6MeV,
theresonant behaviour of this system was the
object
offrequent experimental
and theoretical studies. Themajor
obstacle inunderstanding
this behaviour wasthe
inability
of thephenomenological
models toreproduce
theincreasing
number of resonances dis- covered around the Coulomb barrierregion. Recently, however; Park,
Scheid and Greiner[2]
andKondo,
Matsuse and Abe[3]
have succeeded inremoving
thisdifficulty by
anappropriate
choice ofscattering potentials.
The latter authorstogether
withqualitati- vely accounting
for theexisting
resonances,have,
moreover,
predicted
a group of resonances(8+, 4+, 6+)
centered around
where none were
previously
observed. A morecareful
scrutiny
ofexisting data, however,
couldhave indicated the presence of resonance behaviour around 7.5 MeV
(cm) :
a minimum inthe 12C + 12C
elastic
scattering
excitation function at 90° "near that energy wasreported
in reference[4]. Also,
several
strong peaks
in the excitation function of the inverse2 ONe (ex, 12C)12C
reaction were observed in reference[5]
for excitationenergies
in24Mg
corres-ponding
to center of massenergies
ofthe 12C + 12C
system in the aboveregion.
Thus a detailedstudy
ofthe resonant behaviour of
12C + 12C
in this energyregion appeared
to bequite interesting.
We have measured the excitation functions of the reactions
12C(12C, p)23Na
at 15° lab. and12C(12C, ex)2°Ne
at 15° and 35° lab.respectively using
the
Saclay
tandem van de Graaff accelerator. The measurements wereperformed
in energysteps
of 200 keV fromE1ab
= 14 to 22 MeV(Eern
= 7-11MeV).
(*) Permanent address : Laboratory for Nuclear Spectroscopy,
Institute « R. Boskovic », Zagreb, Yugoslavia.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyslet:01976003706013100
L-132 JOURNAL DE PHYSIQUE - LETTRES
The
protons
andalpha particles
were detected simul-taneously
in two AE-Etelescopic
detectors. The overall energy resolution of the measurement wasabout 150 keV for protons and 180 keV for
alphas ;
these
figures
include the beam energyspread (-
130-150 keV on a 27Jlg/cm2 12C target).
The excitation functions for three proton groups
(Olab
=15°) leading respectively
to the states of23Na
at
0.0, 2.08
and 3.68 MeV excitation and for fouralpha
groups
(8lab
= 150 and 350respectively), leading respectively
to the states in2°Ne
at0.0, 1.63,
4.25 and 4.97MeV,
are shown from top to bottom infigure
1.In
addition,
excitation functions were measured for twelve otherproton
groupsleading
to levels up to 6.65 MeV excitation in23Na
and also for five otheralpha
groupsleading
to levels up to 7.14 MeV excita- tion in2°Ne,
but none of them are shown in thefigure.
Some of these levels were unresolved. Their
pattern is quite
similar to those shown in thefigure.
FIG. 1. - Excitation functions for (top to bottom) three proton groups (0~b = 15°) leading to, respectively, the states of 0.0, 2.08 and 3.68 MeV excitation in 23Na, for four alpha groups (Blab = 150) leading to, respectively, the states of 0.0, 1.63, 4.25 and 4.97 MeV excitation in 2°Ne and for the same alpha groups at Blab = 35°.
The dashed curves represent excitation functions averaged over
3 000 keV.
Resonant behaviour is
quite
apparent at severalenergies
where eitherstrong
maxima orstrong
minimaare observed in almost all excitation functions. The width of these resonances can be estimated to be about 400 keV
laboratory
energy, A shift in the energy of theresonances
by
about 200 keV was observed in some excitationfunctions;
we shall return to thispoint
later on.
In order to determine which of the observed devia- tions
(maxima
andminima)
from the average trend of the excitation functions arenon-statistical,
we havecalculated for each excitation function
(Jø,r(E) leading
to a final state f measured at a
detecting angle
0 adeviation function :
where
(1o,c(E)
is an average taken over agiven
energyinterval centered around E. Correlated
(non-statis- tical)
deviations shouldpersist
in all or most deviationfunctions,
thus in their sum. Severalaveraging
inter-vals
(ðE1ab
= 600 to 3 000keV)
were used in comput-ing
the deviationfunctions;
this altered thepeak-to- valley
ratios and caused small shifts(~
200keV)
inthe
positions
of thepeaks,
but did not alter thegeneral pattern
of the deviationfunctions,
at least for intervals wider than about1000
keV.FIG. 2. - Summed deviation functions for, respectively, (top to bottom) fifteen proton groups at 150
[Eexc(23Na)
= 0.0, 0.44, 2.08, 2.39, 2.64 + 2.71, 2.98, 3.68, 3.85 + 3.91, 4.43, 4.78, 5.38 + 5.52, 5.78, 5.97 + 6.07, 6.25 + 6.40 and 6.65MeV]
and for ninealpha groups at 150 and 350
[EexceONe)
= 0.0, 1.63, 4.25, 4.97, 5.62 + 5.78, 6.72, 7.01 + 7.16, 7.42 and 7.84MeV]
and for the whole set of results (protons and alphas, all angles). The averaginginterval in this figure was of 3 000 keV. The four vertical dashed lines show the locations of reported resonances.
The summed deviation functions for 15 proton groups at
15~,
for 9alpha
groups at 15° and at 35° and for the whole set of results(protons
andalphas)
areshown, respectively,
from top to bottom infigure
2.The
partial
deviation functions werecomputed
with an
averaging
intervalAElab
= 3 000 keV. Peaks in the total summed deviation function(all particles)
are visible at
Elab
=14.9, 16.9,
17.7 and 18.5 MeVcorresponding
to excitationenergies
in24Mg
of21.4, 22.4,
22.8 and 23.2 MeVrespectively.
It shouldbe noted that
only
thepeaks
at 16.9 and 17.7 MeV show up in all the channel deviation functions(see Fig. 2).
Let us examine the resonances associated with the above
peaks
in more detail. As mentionedbefore,
a strongpeak
was observed in the exci- tation function of theinverse 20Ne(a, 12C)12 C
reactionat
Eern
= 12.1 MeV[5].
The excitation energy in24Mg corresponding
to thispeak (Eexc
= 21.4MeV)
isequal
to that for ourpeak
atElab
= 14.9 MeV(see
Table
I).
From theexperimental angular
distribution it waspossible
to attribute thepeak
at 12.1 MeV totwo
overlapping
levelshaving
J = 4 and 6respecti- vely [5].
In the present data theElab
= 14.9 MeVpeak
is visibleonly
in thealpha particle
exit channels.We have no means of
establishing
whether our obser-vation stands for a
single
or for severalclosely spaced
resonances. The energy shift observed in some excita- tion functions
might
indicate that at least twoclosely spaced
resonances are present.Moreover,
apeak
nearElab
= 15.4 MeV[Eex(24Mg) ~
21.7MeV]
is observ-ed in our
experiment
in the proton deviation functions :resonances of different
spin
will indeed show up with differentstrengths
in proton andalpha particle
channels.
It is worth
pointing
out that other resonancepeaks
observed in the inverse
2°Ne(ex, 12C)12C
reaction showa certain correlation with the
peaks
observed in the summed deviation functionsof, respectively,
thealpha particle
and proton channels in ourexperiment.
Thecomparison
is shown in table I.As to
speculations
about the nature of the observed resonances, it is above alltempting
to associate someor the whole group of the three resonances with the levels J =
8,
4 and 6predicted
around 21.5 MeV in24Mg
in the calculations of Kondo et al.[3]
withthe
peak
observed nearElab
= 14.9 MeV in ourexperiment
and the mentioned 12.1 MeVpeak
in2°Ne(ex, 12c)12C
bothcorresponding
to~=21.4
MeVin
24Mg (see
TableI).
The agreement with the above calculations would indicate a molecular character of the 21.4 MeV resonance. As the observation of thesame resonance in the
2°Ne(ex, 12C)12C
reaction would favour itsalpha
structureconfiguration,
the combinedTABLE I
Comparison
between thepeaks
observed in theexcitation
function
at 900of
the2°Ne(ex, 12c)12C
reaction
(ref. [5])
and the present data(deviation functions) (*)
(*) Energies are uncertain up to 200 keV in the 20Ne + ot experi-
ment and up to 100 keV in the present work (cm).
results of references
[3, 5]
and ourexperiment
may appear as ratherpuzzling.
Several comments are,however, appropriate. First,
the fact that the12C(12C, exo)2°Ne
and the2°Ne(ex, 12C)12C
reactionsshow resonant behaviour at the same energy
(in 24Mg)
may be
simply
due to their inverseness. This fact thenonly
adds to thereality
of a resonance at 21.4 MeV in24Mg,
but need not generatecontradictory
structuralconsiderations.
Furthermore,
the 21.4 MeV resonancewas observed in the
12C
+12C
entrance channelleading
to all or most ofalpha
exit channels and the inverse(i.e. 2°Ne
+ x -7,12C*
+12C*)
nothaving
been
observed,
we have more reason to believe in a resonance inthe 12C + 12 C
entrance channel. A pre-dominantly 12C
+12C
molecular character for theresonance at 21.4 MeV in
24Mg
may therefore be deduced. The agreement with the calculated energy of the J =8, 4
and 6 group(ref. [5]), although strengthen- ing
thispoint,
could nevertheless be fortuitous. Infact,
the weakness of the 21.4 MeV resonance in the proton exit channels(see Fig. 2) although explainable
in terms of a
possible high angular
momentum(J > 6), points
out that the presence ofalpha configu-
rations in the wave function of the 21.4 MeV reso- nance should not be excluded.
As to the nature of other resonances
(22.4,
22.8 and23.2 MeV in
24Mg)
observed in the presentexperiment,
in view of their correlation with
peaks
observed in the2°Ne(ex, 12C)12C reaction, arguments
similar to theabove ones can be advanced about the
interplay
of12C
+12C
vsalpha and/or
otherconfigurations [6].
It
is, however, interesting
topoint
out that resonancesof molecular character were
predicted
in reference[2]
at excitation
energies
in24 Mg
of 22.2( 10 + ),
22.8(8 t )
and 23.2 MeV
(6+) respectively,
in rathergood
agree- ment with ourfindings.
L-134 JOURNAL DE PHYSIQUE - LETTRES
References
[1] ALMQUIST, E., BROMLEY, D. A. and KUEHNER, J. A., Phys.
Rev. Lett. 4 (1960) 515.
[2] PARK, J. Y., SCHEID, W. and GREINER, W., Contrib. Int. Conf.
on Reactions between Complex Nuclei, Nashville, Tenn.
(1974), p. 3 and Phys. Rev. C 10 (1974) 967.
[3] KONDO, Y., MATSUSE, T. and ABE, Y., Contrib. 2nd Int. Conf.
on clustering Phenomena in Nuclei, College Park, Md (1975), paper VII-B-5.
[4] SPINKA, H., Ph. D. Thesis, Calif. Inst. of Technology (1971) unpublished;
SPINKA, H. and WINKLER, H., Nucl. Phys. A 233 (1974) 456.
[5] LASSEN, N. O. and OLSEN, J. S., Mat. Fys. Medd. Dan. Vid.
Selsk. 33, n° 13 (1963).
[6] MICHAUD, G. J. and VOGT, E. N., Phys. Rev. C 5 (1972) 350.
VOIT, H., ISCHENKO, G. and SILLER, F., Phys. Rev. Lett. 30 (1973) 564.