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Submitted on 1 Jan 1978
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Evidence for quasi-static scission configurations obtained
from long range particle accompanied fission
distributions
C. Guet, C. Signarbieux, P. Perrin, H. Nifenecker, B. Leroux, M. Asghar
To cite this version:
L-213
EVIDENCE
FOR
QUASI-STATIC
SCISSION
CONFIGURATIONS
OBTAINED
FROM LONG RANGE PARTICLE ACCOMPANIED FISSION DISTRIBUTIONS
C.GUET,
C. SIGNARBIEUX(*),
P. PERRIN(**),
H. NIFENECKER(**),
B. LEROUX
(***)
and M. ASGHARInstitut
Laue-Langevin,
156X Centre deTri,
38042 GrenobleCedex,
France(Re~u
le 27avril 1978,
accepte
le 18 mai1978)
Résumé. 2014 De nouveaux résultats sur la fission
accompagnée
departicules
légères de 236U sontprésentés. Les largeurs de la distribution angulaire de la
particule
03B1 sont les mêmes dans les fissions de 236U(nth)
etde 252Cf(s.f).
Ilapparait
que cette largeur angulaire est une fonction décroissante del’énergie
cinétique totale desfragments
de fission. Ces résultats suggèrent que lescaractéristiques
dece mode de fission ne sont pas
incompatibles
avec un modèle de la scission supposantl’équilibre
thermodynamique
desdegrés
de liberté collectifs.Abstract.
2014 Newexperimental results on
light-particle-accompanied
neutron-induced fissionof 236U are
presented.
The widths of the03B1-particle
angular distributions are the same for 236U(nth)
and 252Cf(s.f).
This angular width appears to be adecreasing
function of the total fissionfragment
kinetic energy. These results suggest that the characteristics of this mode of fission are not inconsistent with a
semi-equilibrium
model for scission.LE JOURNAL DE PHYSIQUE - LETTRES TOME 39, ler JUILLET 1978,
Classification
Physics Abstracts 25.85
The
knowledge
of thefragment
shapes
and kineticenergies
at scission is essential for anydynamical
theory
of fission. Sincelight charged particles
emitted internary
fission emerge from the neckjoining
the Inascent
fragments
at a time close toscission,
a detailedstudy
of this mode of fission shouldprovide unique
information on the last stage of the fission process andmore
generally
on thedynamical
properties
of nuclear matter at low and moderatetemperatures. However,
the extraction of scission parameters fromternary
fission data isunfortunately
notstraightforward.
Aswe are confronted with a
three-body
problem,
thesimplest
procedure
is to try a set of initial conditions which could be identified with the scission parameters,to compute the
trajectories
[1],
and to compare the calculatedquantities
atinfinity
with theexperimental
data.
By
scission parameters we meanessentially
theprescission
kinetic energyEKo
of the fissionfragments,
the initial momentum of thea-particle
and their relativepositions.
EKo is
the kinetic energyacquired
in the fission modeduring
the descent from saddle to scission.(*) Centre d’Etudes Nuc1éaires, DPhN/MF, BP 2, 91190 Gif
sur Yvette, France.
(**) Centre d’Etudes Nucleaires, DRF/CPN, 85X, 38041
Gre-noble, France.
(***) Universite de Bordeaux, Gradignan, France.
The results which are
presented
below mayprovide
new information on the
sharing
betweenpotential
and kineticenergies during
the descent from saddle to scission. These new features ofa-accompanied
neutron induced fission of236L1
have been obtainedrecently
in anexperiment
carried out at the GrenobleHigh
Flux Reactor where a beam of 5.5 x 109
nth/cm2/s
isavailable. The
angular
distribution of thea-particles
was measured with a
good
accuracy as a function ofthe kinetic energy and mass of the fission
fragments.
A silicon
rectangular
detector( 1
cm x 3cm)
fixed the a direction while 7 circular(yr
cm 2)
fission detectorswere
placed
atangles
from 68° to 98° withrespect
tothe a direction in
steps
of 5°. The Icm 2
circular uraniumtarget
was 150J.1g/cm2
UF4
(235U
enrichmentof 97
%) evaporated
on to a 20J.1g/cm2
VYNSbacking.
The
experimental
set-up allowed for ageometrical
angular
dispersion
(FWHM)
of5°,
and for a massdispersion (FWHM)
of 6 amu. The mass of the fissionfragment
was determinedby
measuring
its kineticenergy and
velocity,
this lastquantity being
derivedfrom the difference of
times-of-flight
of fissionfrag-ment and a
particle
afterappropriate
corrections.A
large
number of correlations have been derived and will bepresented
in a detailedpublication.
Wepresent here two of these results which we believe deserve
special
attention :L-214 JOURNAL DE PHYSIQUE - LETTRES
a)
The widths of theglobal
a-particle angular
distributions arenearly
identical for 236U(nth)
and 252Cf
(st).
The
angular
distribution is defined with respect to thelight
fragment
direction. Its mostprobable
value and widthdepend
slightly
upon the a energy threshold below which the events arerejected.
The mostprobable
angle,
81.3° ± 0.4 forparticles
with kinetic energyhigher
than 10 MeV(820
± 0.4 forEa
> 12.5MeV)
is lower
by
about 20 than theangle
measured for2 5 2Cf
(sf) [2, 3].
This difference iseasily
understandable in terms of the moreasymmetric
ratio of the meanfragments
masses for236U
than for252Cf;
this leads to astronger
deflection away from theperpendicular
direction for
236 U.
After correction of thegeometrical
dispersion,
the width(FWHM)
of the distributionis 18.70 + 0.80 for
Ea
> 10 MeV. This width is lower than those measuredpreviously
[4].
We want to underline thestriking
similarity
between this value and18.50 ± 10
(FWHM)
measured for252Cf
[2, 3].
In so far as the classical
three-point-charge
model isvalid,
these present observations disfavour thedyna-mical
liquid drop
treatment of fissionproposed
by
Nix et al.[5, 6].
In addition tohigh pre-scission
kineticenergies
(around
25 MeV for236U),
theliquid drop
calculationspredict
a marked increase of thisquantity
as a function of thefissibility
parameter.
Forexample,
the
pre-scission
kinetic energy for252Cf
ispredicted
to be about 1.5 times of the value for
236U.
Since the finalangular
distribution of thea-particles
isessen-tially dependent
on their initialpositions
and theinitial
fragment
kinetic energy[1, 7],
one shouldexpect
a wider
angular
spectrum
for252Cf
than for236U
which is
contrary
to theexperimental
results. In order toreproduce
suchglobal angular
widths,
trajectory
calculations have shown
that
with
reasonabledis-persions
of initialparameters,
one cannot rule out thepossibility
of low initialfragment
kinetic energy(E~
10MeV) [7, 8].
b)
Theangular
distribution gets narrower as thekinetic energy of the fission
fragments
increases. Infigure
1 we show thedependence
of the averageangle
0,, - L >
and theangular
width(FWHM)
upon the total kinetic energyEK
of the fissionfragments
forgiven
values offragment
mass and for a-kineticenergies higher
than 10 MeV. The averageangle
does not show anysignificant
variation withEK.
However,
there is a clear decrease of the width asEK
goes up.In order to
preclude
the effect of the well-known anti-correlation betweenE«
andEK [9,
10],
the’angular
distribution was derived after
setting
a narrowwindow
(2 MeV)
on the a-energyspectrum.
The sametrend was observed : the
angular
distribution isnarrower for
higher fragment
energy events. It isgenerally accepted
that the final a-kinetic energy isstrongly
determinedby
its initial value2~
[1].
There-fore,
for agiven
final a-kinetic energy(hence
a smallspread
inE,,,.),
theequation
for variances derived fromFIG. 1. -
Average angle « (}rz-L » and angular width (FWHM) as a function of total fragment energy with the conditions that
Ea > 9.5 MeV and ML = 85-87 amu (0), or ML = 91-93 amu (~),
or ML = 97-99 amu ( x ).
the energy conservation relation :
can be written in a reasonable
approximation
asfollows :
Here C is the Coulomb
potential
energy of thefrag-ments and is sensitive to their deformations. Let us
consider two extreme situations :
i)
First we assume that thespread
inEKo is
muchlarger
than thespread
in the Coulomb energy. In thiscase there is a one-to-one
correspondence
betweenEK
andEKo.
Thefragment
charge
centre distance is then almost constant as is thedispersion
in the initialposition
of thea-particle.
The faster thefragments
separate, the less the
a-particle
will befocused,
thusleading
to abroadening
of theangular
distributionsas
EK
increases. This is contrary to ourexperimental
observations.
ii) Secondly,
we now supposeEKo
to be a constant,then7(~) ~
r(C);
in this case thehigher
values ofEK
configu-L-215
QUASI-STATIC SCISSION CONFIGURATIONS
rations,
andconsequently
a narrower distribution ofthe initial
positions
for the emission ofa-particles.
As the final emissionangle
isstrongly
determinedby
the initialposition along
thefragment
axis,
this extreme modelpredicts
the samequalitative
variationas observed
experimentally.
In
conclusion,
theexperimental
resultspresented
above tend to indicate that the
dispersion
of the total fissionfragment
kinetic energy resultsmainly
from the fluctuations of the scissionshapes (stretching
modes)
rather thanfrom
the distribution of the pre-scission kinetic energy which iscertainly
rather low.This conclusion would mean that the features of the
a-accompanied
fission are notcontradictory
to themodels based on a
quasi-statistical equilibrium
amongthe collective
degrees
of freedom at scission[11, 12]
as discussed and
justified
in terms of fission bandsby
Norenberg
[12].
Acknowledgments.
- Weare
grateful
to S.Bjorn-holm,
M.Brack,
K. Dietrich and P. Schuck for fruitful discussions. We are indebted to M. Brack forreading
themanuscript.
References
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(1967) 1305.
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the physics and chemistry of fission (Rochester, 1973,
Vienna) p. 405.
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