51-Sb-124 JNDC EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.
----JENDL-4.0 MATERIAL 5134
-----INCIDENT NEUTRON DATA
JENDL-3.3 data were automatically transformed to JENDL-4.0.
JENDL-3.2 data were automatically transformed to JENDL-3.3.
Interpolation of spectra: 22 (unit base interpolation)
(3,251) deleted, T-matrix of (4,2) deleted, and others.
84-10 Evaluation for JENDL-2 was made by JNDC FPND W.G./1/
90-03 Modification for JENDL-3 was made/2/.
mf = 1 General information
mt=451 Comments and dictionary
mf = 2 Resonance parameters
mt=151 Resolved and unresolved resonance parameters
No resolved resonance parameters
Unresolved resonance region : 2.54 eV - 100 keV
The neutron strength function, S0, was estimated from those of
other Sb isotopes, and S1 and S2 were calculated with optical
model code CASTHY/3/. The observed level spacing was
determined to reproduce the capture cross section calculated
with CASTHY at 100 keV. The effective scattering radius was
obtained from fitting to the calculated total cross section at
Typical values of the parameters at 70 keV:
S0 = 0.300e-4, S1 = 2.700e-4, S2 = 0.760e-4, Sg = 211.e-4,
Gg = 0.100 eV, R = 5.700 fm.
The unresolved parameters should be used only for
calculated 2200-m/s cross sections and res. integrals (barns)
2200 m/s res. integ.
total 21.22 -
elastic 3.776 -
capture 17.41 156 (*)
(*) Integrated from 0.5 eV to 10 MeV.
mf = 3 Neutron cross sections
Below 2.54 eV, the capture and elastic scattering cross sections
were assumed to be in 1/v form and constant, respectively. The
capture cross section at 0.0253 eV was taken from the
compilation by Mughabghab et al./4/ unresolved resonance
parameters were given in the energy range from 2.54 eV to 100
Above 100 keV, the spherical optical and statistical model
calculation was performed with CASTHY, by taking account of
competing reactions, of which cross sections were calculated
with PEGASUS/5/ standing on a preequilibrium and multi-step
evaporation model. The OMP's for neutron given in Table 1 were
determined to reproduce a systematic trend of the total cross
section by changing rso of Iijima-Kawai potential/6/. The
OMP's for charged particles are as follows:
proton = Perey/7/
alpha = Huizenga and Igo/8/
deuteron = Lohr and Haeberli/9/
helium-3 and triton = Becchetti and Greenlees/10/
Parameters for the composite level density formula of Gilbert
and Cameron/11/ were evaluated by Iijima et al./12/ More
extensive determination and modification were made in the
present work. Table 2 shows the level density parameters used
in the present calculation. Energy dependence of spin cut-off
parameter in the energy range below E-joint is due to Gruppelaar
mt = 1 Total
Spherical optical model calculation was adopted.
mt = 2 Elastic scattering
Calculated as (total - sum of partial cross sections).
mt = 4, 51 - 91 Inelastic scattering
Spherical optical and statistical model calculation was
adopted. The level scheme was taken from Ref./14/.
no. energy(MeV) spin-parity
gr. 0.0 3 -
1 0.0107 5 +
Levels above 0.041 MeV were assumed to be overlapping.
mt = 102 Capture
Spherical optical and statistical model calculation with
CASTHY was adopted. Direct and semi-direct capture cross
sections were estimated according to the procedure of Benzi
and Reffo/15/ and normalized to 1 milli-barn at 14 MeV.
The gamma-ray strength function (1.97e-02) was determined from
the systematics of radiation width (0.1 eV) and the average
s-wave resonance level spacing (5.08 eV) calculated from the
level density parameters.
mt = 16 (n,2n) cross section
mt = 17 (n,3n) cross section
mt = 22 (n,n'a) cross section
mt = 28 (n,n'p) cross section
mt = 32 (n,n'd) cross section
mt = 33 (n,n't) cross section
mt =103 (n,p) cross section
mt =104 (n,d) cross section
mt =105 (n,t) cross section
mt =107 (n,alpha) cross section
These reaction cross sections were calculated with the
preequilibrium and multi-step evaporation model code PEGASUS.
The Kalbach's constant k (= 176.9) was estimated by the
formula derived from Kikuchi-Kawai's formalism/16/ and level
Finally, the (n,p) and (n,alpha) cross sections were
normalized to the following values at 14.5 MeV:
(n,p) 3.53 mb (systematics of Forrest/17/)
(n,alpha) 1.91 mb (systematics of Forrest)
mt = 251 mu-bar
Calculated with CASTHY.
mf = 4 Angular distributions of secondary neutrons
Legendre polynomial coefficients for angular distributions are
given in the center-of-mass system for mt=2 and discrete inelas-
tic levels, and in the laboratory system for mt=91. They were
calculated with CASTHY. For other reactions, isotropic distri-
butions in the laboratory system were assumed.
mf = 5 Energy distributions of secondary neutrons
Energy distributions of secondary neutrons were calculated with
PEGASUS for inelastic scattering from overlapping levels and for
other neutron emitting reactions.
TABLE 1 NEUTRON OPTICAL POTENTIAL PARAMETERS
DEPTH (MEV) RADIUS(FM) DIFFUSENESS(FM)
---------------------- ------------ ---------------
V = 47.64-0.473E R0 = 6.256 A0 = 0.62
WS = 9.744 RS = 6.469 AS = 0.35
VSO= 7.0 RSO= 6.241 ASO= 0.62
THE FORM OF SURFACE ABSORPTION PART IS DER. WOODS-SAXON TYPE.
TABLE 2 LEVEL DENSITY PARAMETERS
NUCLIDE SYST A(1/MEV) T(MEV) C(1/MEV) EX(MEV) PAIRING
49-IN-120 * 1.757E+01 6.016E-01 2.330E+01 4.366E+00 0.0
49-IN-121 1.601E+01 6.060E-01 1.119E+00 5.277E+00 1.430E+00
49-IN-122 * 1.707E+01 5.968E-01 1.737E+01 4.092E+00 0.0
49-IN-123 1.470E+01 6.100E-01 1.134E+00 4.483E+00 1.090E+00
50-SN-121 1.630E+01 6.100E-01 2.010E+00 5.217E+00 1.190E+00
50-SN-122 1.434E+01 7.060E-01 3.423E-01 7.416E+00 2.620E+00
50-SN-123 1.509E+01 6.870E-01 3.062E+00 6.032E+00 1.190E+00
50-SN-124 1.601E+01 6.160E-01 3.224E-01 6.294E+00 2.280E+00
51-SB-122 1.772E+01 5.500E-01 1.346E+01 3.517E+00 0.0
51-SB-123 1.585E+01 6.213E-01 1.285E+00 5.469E+00 1.430E+00
51-SB-124 1.696E+01 5.600E-01 1.090E+01 3.433E+00 0.0
51-SB-125 1.700E+01 5.120E-01 7.883E-01 3.792E+00 1.090E+00
syst: * = ldp's were determined from systematics.
Spin cutoff parameters were calculated as 0.146*sqrt(a)*a**(2/3).
In the CASTHY calculation, spin cutoff factors at 0 MeV were
assumed to be 5.0 for Sb-124 and 7.267 for Sb-125.
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Reactions", North Holland (1968).
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