22-Ti- 47 KUR EVAL-SEP88 K.KOBAYASHI(KUR),H.HASHIKURA(TOK)
DIST-MAY10 20090804
----JENDL-4.0 MATERIAL 2228
-----INCIDENT NEUTRON DATA
------ENDF-6 FORMAT
HISTORY
88-09 Compiled by T.Asami(nedac)
93-12 JENDL-3.2
Data were adopted from JENDL fusion file.
Compiled by T.Nakagawa
00-03 Reevaluation was made by T.Asami.
01-11 Compiled by K.Shibata (ndc/jaeri)
***** modified parts for JENDL-3.3 ********************
(3,2) re-calculated
(3,28,102,103) revised
(3,104,105,106,111, 203,207) evaluated newly
(3,251) deleted
(4,2) revised
(4,16,22,28,91) deleted
(5,16,22,28,91) deleted
(6,16,22,28,91) taken from JENDL fusion file
(6,203, 207) taken from JENDL fusion file
(12,16-107) evaluated newly
(14,16-107) isotropic distributions
(15,16-107) evaluated newly
***********************************************************
09-08 Compiled by K. Shibata.
The resolved resonance parameters were revised.
mf=1 General information
mt=451 Descriptive data and dictionary
mf=2 Resonance parameters
mt=151 Resolved resonance parameters
Resolved parameters for MLBW formula were given in the energy
region from 1.0e-5 eV to 100 keV. Parameters were taken from
ref./5/, for positive resonances. Parameters for negative
resonance were obtained so that the reproduced cross sections
for both scattering and capture gave the 2200 m/s values of
3.1+-0.2 and 1.7+-0.2 barns, respectively/5/. The scattering
radius was assumed to be 4.5 fermi instead of 3.6 fermi in
ref./5/.
For JENDL-4, the resolved resonance parameters were modified
by Kawano /18/.
Thermal cross sections and resonance integrals at 300 K
----------------------------------------------------------
0.0253 eV res. integ. (*)
(barns) (barns)
----------------------------------------------------------
Total 4.8919E+00
Elastic 3.2656E+00
n,gamma 1.6264E+00 1.3393E+00
----------------------------------------------------------
(*) Integrated from 0.5 eV to 10 MeV.
mf=3 Neutron cross sections
Below 100 kev, no background cross section was given.
The calculation with sincros-ii system/2/ was made by adopting
Walter-Guss omp modified by Yamamuro/2/ for neutron, Perey omp
/6/ for proton, Lemos omp modified by Arthur and Young/7/
for alpha, Lohr-Haeberli omp/8/ for deuteron, Becchettii-
Greenlees omp/9/ for triton and he-3, and standard level
density parameters of sincros-ii system.
mt=1 Total
Below 100 keV, created from the resonance paranmeters.
Above 100 keV, optical and statistical model calculation was
made with the casthy code/10/.
The optical potential parameters used are:
V = 50.75 - 0.120*En, Vso = 4.72 (MeV)
Ws = 10.9 - 0.234*En, Wv = 0.0 (MeV)
r = 1.26, rs = 1.02, rso = 1.16 (fm)
a = 0.52, aso = 0.52, b = 0.40 (fm)
mt=2 Elastic scattering
Obtained by subtracting the sum of the partial cross sections
from the total cross section.
mt=4, 51-66, 91 Inelastic scattering
The cross sections were taken from JENDL fusion file. the
level scheme was based on ref./4/ Contributions of the
direct process were calculated for the levels marked with '*'.
no. energy(MeV) spin-parity (direct process)
g.s. 0.0 5/2 -
1 0.1594 7/2 - *
2 1.2521 9/2 - *
3 1.254 1/2 -
4 1.4442 11/2 - *
5 1.5499 3/2 - *
6 1.67 1/2 -
7 1.7941 1/2 - *
8 1.825 3/2 +
9 2.163 3/2 - *
10 2.1667 5/2 +
11 2.2595 5/2 +
12 2.2971 3/2 -
13 2.344 5/2 +
14 2.3649 1/2 +
15 2.4062 5/2 -
16 2.4163 1/2 -
Levels above 2.416 MeV were assumed to be overlapping.
mt=16, 22 (n,2n), (n,na)
Adopted from JENDL fusion file. Theoretical calculation was
made with sincros-ii. The (n,2n) results were normalized to
0.200 b at 14.9 MeV systematics by Kasugai/11/
mt=28 (n,np)
Obtained from from the sincros-ii calculation made with the
the egnash code/2/.
mt=102 Capture
Calculated with the casthy code/10/ and normalized to 65.5 mb
at 30 keV. Added the semidirect component calculated with
the quick gnash code/16,17/.
mt=103 (n,p)
Taken from JENDL dosimetry file/14/.
mt=107 (n,a)
Calculated with the gnash code/12/.
mf=4 Angular distributions of secondary neutrons
mt=2
Calculated with the casthy code/10/,newly for JENDL-3.3.
mt=51-66
Taken from JENDL fusion file/1/.
mf=6 Energy-angle distributions of secondary particles
Taken from JENDL fusion file/1/.
- Energy distributions of secondary neutrons were replaced
by those calculated by egnash2. The ddx's of the
continuum neutrons were calculated by Kumabe's systema-
tics /3/ using f15tob /1/. The precompound/compound
ratio was calculated by the sincros-ii code system/2/.
mt=16, 22, 28, 91
Based on modified Kumabe's systematics/1/.
mt=203, 207
Based on kalbach's 1988 systematics/13/.
mf=12 Photon production multiplicities and transition probability
arrays
mt=16, 22, 28, 51-66, 91,103, 104, 107
mt=51-66 were given as the transition probability arrays.
mt=16, 22, 28, 91, 102, 103, 104, 107 were calculated with
the egnash code/2/ and processed by the gamfil2 code/15/.
mt=102 was calculated with the casthy code/10/.
mf=14 Photon angular distributions
mt=16, 22, 28, 51-66, 91, 102, 103, 104, 107
Assumed to be isotropic distributions
mf=15 Continuous photon energy spectra
mt=16, 22, 28, 91, 103, 104, 107
Calculated with the egnash code/2/.
mt=102
Calculated with the casthy code/10/.
References
1) Chiba, S. et al.: JAERI-M 92-027, p.35 (1992).
2) Yamamuro, N.: JAERI-M 90-006 (1990).
3) Kumabe, I. et al.: Nucl. Sci. Eng., 104, 280 (1990).
4) ENSDF: Evaluated Nuclear Structure Data File, BNL/NNDC.
5) Mughabghab S.F. et al. : " Neutron Cross Sections ", Vol.1,
Part A (1981).
6) Perey, F.G.: Phys. Rev., 131, 745 (1963).
7) Arthur, E.D. and Young, P.G.: LA-8626-MS (1980).
8) Lohr, J.M. and Haeberli W.: Nucl. Phys., A232, 381 (1974).
9) Becchetti, F.D. Jr. and Greenlees G.W.: "Polarization
Phenomena in Nucl. Reactions," Univ. Wisconsin Press, p.682
(1971).
10) Igarasi S. and Fukahori T.: JAERI 1321 (1991).
11) Kasugai Y.: private communication (1993).
12) Young P.G. and Arthur E.D. : LA-6947 (1977).
13) Kalbach C. : Phys. Rev. C37, 2350(1988).
14) Nakazawa M. et al. : JAERI 1325 (1992).
15) Hida K.: JAERI-M 86-150 (1986) (in Japanese).
16) Young P.G. et al. : LA-12343-MS (1992).
17) Koning A.J. and Delaroche J.P. : ECN-RX-98-015 (1998).
18) Kawano T.: Private communication (2008).