52-Te-123
52-Te-123 JNDC EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.
DIST-MAY10 20091214
----JENDL-4.0 MATERIAL 5234
-----INCIDENT NEUTRON DATA
------ENDF-6 FORMAT
===========================================================
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.
===========================================================
History
90-03 New evaluation for JENDL-3 was completed by JNDC FPND
W.G./1/
93-09 JENDL-3.2 was made by JNDC FPND W.G.
09-12 Compiled by A.Ichihara.
***** modified parts for JENDL-3.2 ********************
(2,151) Unresolved resonance parameters re-adjusted
so as to reproduce the re-normalized capture
cross section.
(3,102) Re-normalization.
(3,2), (3,4), (3,51-91) and angular distributions
small effects of the re-normalization of
capture cross section.
***********************************************************
***** modified parts for JENDL-4.0 ********************
(2,151) Unresolved resonance parameters were updated.
***********************************************************
mf = 1 General information
mt=451 Comments and dictionary
mf = 2 Resonance parameters
mt=151 Resolved and unresolved resonance parameters
Resolved resonance region (MLBW formula) : below 700 eV
Resonance parameters were based on Mughabghab et al./2/ total
spin J of some resonances was tentatively estimated with a
random number method. Neutron orbital angular momentum L was
estimated with a method of Bollinger and Thomas/3/. Averaged
radiation width was deduced to be 107 meV, and applied to the
levels whose radiation width was unknown. The scattering
radius was also taken from Mughabghab et al.
Unresolved resonance region : 0.7 keV - 200 keV
The neutron strength function S0 was based on the compilation
of Mughabghab et al., and S1 and S2 were calculated with
optical model code CASTHY/4/. The observed level spacing was
determined to reproduce the capture cross sections calculated
with CASTHY. The effective scattering radius was obtained
from fitting to the calculated total cross section at 100 keV.
The radiation width Gg was based on the compilation of
Mughabghab et al.
Typical values of the parameters at 70 keV:
S0 = 0.790e-4, S1 = 1.700e-4, S2 = 1.100e-4, Sg = 80.9e-4,
Gg = 0.124 eV, R = 5.519 fm.
The unresolved resonance parameters were recalculated using
the ASREP code/20/.
The parameters should be used only for self-shielding
calculation.
Thermal cross sections and resonance integrals at 300 K
----------------------------------------------------------
0.0253 eV res. integ. (*)
(barns) (barns)
----------------------------------------------------------
Total 4.190E+02
Elastic 5.923E-01
n,gamma 4.184E+02 5.65E+03
n,alpha 4.6E-05
----------------------------------------------------------
(*) Integrated from 0.5 eV to 10 MeV.
mf = 3 Neutron cross sections
Below 700 eV, resolved resonance parameters were given.
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 r0 and 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
/13/.
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 based on Evaluated Nuclear
Structure Data File (1987 version)/14/ and Nuclear Data
Sheets/15/.
no. energy(MeV) spin-parity
gr. 0.0 1/2 +
1 0.1590 3/2 +
2 0.2475 11/2 -
3 0.4400 3/2 +
4 0.4897 5/2 +
5 0.5053 3/2 +
6 0.5996 1/2 +
7 0.6880 3/2 +
8 0.6975 7/2 +
9 0.7693 5/2 +
10 0.7836 3/2 +
11 0.8947 3/2 +
12 0.9961 5/2 -
13 1.0366 3/2 +
14 1.0682 3/2 +
15 1.0800 7/2 +
Levels above 1.21 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/16/ and normalized to 1 milli-barn at 14 MeV.
The gamma-ray strength function (7.93e-03) was adjusted to
reproduce the capture cross section of 553 milli-barns at 70
keV measured by Macklin et al./17/
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 =103 (n,p) cross section
mt =104 (n,d) cross section
mt =105 (n,t) cross section
mt =106 (n,he3) 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 (= 149.5) was estimated by the
formula derived from Kikuchi-Kawai's formalism/18/ and level
density parameters.
Finally, the (n,p) and (n,alpha) cross sections were
normalized to the following values at 14.5 MeV:
(n,p) 10.60 mb (systematics of Forrest/19/)
(n,alpha) 5.05 mb (systematics of Forrest)
The (n,alpha) cross section below 0.7 keV was calculated from
resonance parameters, by assuming a mean alpha width of
1.15e-8 eV so as to reproduce the thermal cross section/2/.
The cross section was averaged in suitable energy intervals.
Above 0.7 keV, the cross section was connected smoothly to the
PEGASUS calculation.
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 to overlapping levels and for
other neutron emitting reactions.
TABLE 1 NEUTRON OPTICAL POTENTIAL PARAMETERS
DEPTH (MEV) RADIUS(FM) DIFFUSENESS(FM)
---------------------- ------------ ---------------
V = 45.97-0.199E R0 = 6.481 A0 = 0.62
WS = 6.502 RS = 6.926 AS = 0.35
VSO= 7.0 RSO= 6.49 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
---------------------------------------------------------------
50-SN-119 1.635E+01 5.990E-01 1.772E+00 5.050E+00 1.190E+00
50-SN-120 1.595E+01 6.540E-01 4.691E-01 7.083E+00 2.430E+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
51-SB-120 * 1.834E+01 6.016E-01 3.366E+01 4.659E+00 0.0
51-SB-121 1.730E+01 5.740E-01 1.715E+00 5.022E+00 1.240E+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
52-TE-121 1.800E+01 6.200E-01 5.720E+00 6.022E+00 1.140E+00
52-TE-122 1.705E+01 6.350E-01 6.339E-01 7.160E+00 2.380E+00
52-TE-123 1.874E+01 5.850E-01 4.619E+00 5.627E+00 1.140E+00
52-TE-124 1.784E+01 6.740E-01 1.452E+00 8.479E+00 2.570E+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 4.266 for Te-123 and 3.991 for Te-124.
References
1) Kawai, M. et al.: J. Nucl. Sci. Technol., 29, 195 (1992).
2) Mughabghab, S.F. et al.: "Neutron Cross Sections, Vol. I,
Part A", Academic Press (1981).
3) Bollinger, L.M. and Thomas, G.E.: Phys. Rev., 171,1293(1968).
4) Igarasi, S. and Fukahori, T.: JAERI 1321 (1991).
5) Iijima, S. et al.: JAERI-M 87-025, p. 337 (1987).
6) Iijima, S. and Kawai, M.: J. Nucl. Sci. Technol., 20, 77
(1983).
7) Perey, F.G: Phys. Rev. 131, 745 (1963).
8) Huizenga, J.R. and Igo, G.: Nucl. Phys. 29, 462 (1962).
9) Lohr, J.M. and Haeberli, W.: Nucl. Phys. A232, 381 (1974).
10) Becchetti, F.D., Jr. and Greenlees, G.W.: Polarization
Phenomena in Nuclear Reactions ((Eds) H.H. Barshall and
W. Haeberli), p. 682, the University of Wisconsin Press.
(1971).
11) Gilbert, A. and Cameron, A.G.W.: Can. J. Phys., 43, 1446
(1965).
12) Iijima, S., et al.: J. Nucl. Sci. Technol. 21, 10 (1984).
13) Gruppelaar, H.: ECN-13 (1977).
14) ENSDF: Evaluated Nuclear Structure Data File (June 1987).
15) Nuclear Data Sheets, 29, 453 (1980).
16) Benzi, V. and Reffo, G.: CCDN-NW/10 (1969).
17) Macklin, R.L. et al.: ORNL-6561 (1989).
18) Kikuchi, K. and Kawai, M.: "Nuclear Matter and Nuclear
Reactions", North Holland (1968).
19) Forrest, R.A.: AERE-R 12419 (1986).
20) Y.Kikuchi et al., JAERI-Data/Code 99-025 (1999)
[in Japanese].