62-Sm-150
62-SM-150 JNDC EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.
DIST-MAR02 REV3-FEB02 20020222
----JENDL-3.3 MATERIAL 6243
-----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
84-10 EVALUATION FOR JENDL-2 WAS MADE BY JNDC FPND W.G./1/
90-03 MODIFICATION FOR JENDL-3 WAS MADE/2/.
94-06 JENDL-3.2 WAS MADE BY JNDC FPND W.G.
***** MODIFIED PARTS FOR JENDL-3.2 ********************
(3,2) TO KEEP CONSISTENCY OF CROSS SECTIONS
(3,4), (3,51), (3,53), (3,55), (3,59)
DIRECT INELASTIC SCATTERING CONTRIBUTION
WAS INCLUDED.
(3,102) RENORMALIZATION TO NEW EXPERIMENTAL DATA. THE
EFFECTS TO INELASTIC SCATTERING CROSS SECTIONS
ABOUT 1 % OR LESS.
(4,51), (4,53), (4,55), (4,59)
DIRECT INELASTIC SCATTERING CONTRIBUTION
***********************************************************
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 1.538 KEV
RESONANCE PARAMETERS WERE TAKEN FROM JENDL-2 WHICH WAS
EVALUATED BY KIKUCHI ET AL./3/ ON THE BASIS OF THE
EXPERIMENTAL DATA BY EILAND ET AL./4/ AND BY ANUFRIEV ET
AL./5/ THE AVERAGE RADIATION WIDTH OF 0.060 EV WAS ASSUMED.
A NEGATIVE RESONANCE WAS ADDED AT -3.5 EV SO AS TO REPRODUCE
THE CAPTURE CROSS SECTION OF 107+-9 BARNS AND THE TOTAL CROSS
SECTION OF 122+-12 BARNS/4/.
UNRESOLVED RESONANCE REGION : 1.538 KEV - 100 KEV
THE NEUTRON STRENGTH FUNCTION S0 WAS BASED ON THE COMPILATION
OF MUGHABGHAB/6/, AND S1 AND S2 WERE CALCULATED WITH OPTICAL
MODEL CODE CASTHY/7/. THE OBSERVED LEVEL SPACING WAS
DETERMINED TO REPRODUCE THE CAPTURE CROSS SECTION 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.
TYPICAL VALUES OF THE PARAMETERS AT 70 KEV:
S0 = 3.600E-4, S1 = 1.400E-4, S2 = 2.300E-4, SG = 10.98E-4,
GG = 0.060 EV, R = 5.916 FM.
CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS)
2200 M/S RES. INTEG.
TOTAL 116.9 -
ELASTIC 8.341 -
CAPTURE 108.6 325
MF = 3 NEUTRON CROSS SECTIONS
BELOW 100 KEV, RESONANCE PARAMETERS WERE GIVEN.
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/8/ STANDING ON A PREEQUILIBRIUM AND MULTI-STEP
EVAPORATION MODEL. THE OMP'S FOR NEUTRON GIVEN IN TABLE 1 WERE
DETERMINED TO REPRODUCE THE TOTAL CROSS SECTION OF NATURAL SM
MEASURED BY FOSTER AND GLASGOW/9/, KELLIE ET AL./10/ AND SO ON.
THE OMP'S FOR CHARGED PARTICLES ARE AS FOLLOWS:
PROTON = PEREY/11/
ALPHA = HUIZENGA AND IGO/12/
DEUTERON = LOHR AND HAEBERLI/13/
HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/14/
PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT
AND CAMERON/15/ WERE EVALUATED BY IIJIMA ET AL./16/ 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
/17/.
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./18/. THE
LEVELS MARKED WITH * INCLUDE THE CONTRIBUTION OF DIRECT
INELASTIC SCATTERING, WHICH WAS CALCUALTED BY THE COUPLED-
CHANNELS THEORY WITH ECIS88 CODE/19/. THE GROUND STATE
ROTATIONAL BAND (0+ 2+ 4+ 6+(1.27891MEV)) AND OCTUPOLE
VIBRATIONAL BAND (3- 1-(1.16573MEV) 5-) WERE COUPLED
SIMULTANEOUSLY. THE WS PARAMETER WAS ADJUSTED TO 3.5 MEV,
OTHERWISE THE SPHERICAL PARAMETERS WERE USED. THE BETA-2 (=
0.1931) AND BETA-3 (= 0.14526) WERE TAKEN FROM ORNL
COMPILATIONS/20,21/.
NO. ENERGY(MEV) SPIN-PARITY C.C. CALCULATION
GR. 0.0 0 +
1 0.3343 2 + *
2 0.7403 0 +
3 0.7733 4 + *
4 1.0463 2 +
5 1.0720 3 - *
6 1.1650 2 +
7 1.1940 2 +
8 1.2550 0 +
9 1.3570 5 - *
10 1.4170 2 +
11 1.4490 4 +
12 1.5050 3 +
13 1.6430 4 +
14 1.7610 0 +
15 1.7940 2 +
16 1.8200 4 +
17 1.8340 2 +
18 1.9270 2 +
19 1.9510 3 -
20 1.9710 4 +
LEVELS ABOVE 2.006 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/22/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV.
THE GAMMA-RAY STRENGTH FUNCTION (1.098E-03) WAS ADJUSTED TO
REPRODUCE THE CAPTURE CROSS SECTION OF 320 MILLI-BARNS AT 50
KEV MEASURED BY WISSHAK ET AL./23/
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 (= 25.0) WAS ASSUMED TO BE THE SAME
AS THAT OF SM-148.
FINALLY, THE (N,P) AND (N,ALPHA) CROSS SECTIONS WERE
NORMALIZED TO THE FOLLOWING VALUES AT 14.5 MEV:
(N,P) 6.90 MB (RECOMMENDED BY FORREST/24/)
(N,ALPHA) 3.40 MB (RECOMMENDED BY FORREST)
THE (N,2N) CROSS SECTION WAS DETERMINED BY EYE-GUIDING OF
THE DATA MEASURED BY FREHAUT ET AL./25/
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 = 46.96-0.0172E R0 = 6.323 A0 = 0.655
WS = 8.455 RS = 7.651 AS = 0.448
VSO= 7.0 RSO= 6.801 ASO= 0.6
THE FORM OF SURFACE ABSORPTION PART IS DER. WOODS-SAXON TYPE.
TABLE 2 LEVEL DENSITY PARAMETERS
NUCLIDE A(1/MEV) T(MEV) C(1/MEV) EX(MEV) PAIRING
---------------------------------------------------------------
60-ND-146 2.019E+01 5.660E-01 1.121E+00 6.714E+00 2.100E+00
60-ND-147 2.398E+01 4.850E-01 5.510E+00 5.235E+00 1.180E+00
60-ND-148 2.359E+01 5.150E-01 1.328E+00 6.751E+00 2.170E+00
60-ND-149 2.657E+01 4.750E-01 1.192E+01 5.636E+00 1.180E+00
61-PM-147 2.192E+01 4.913E-01 4.801E+00 4.589E+00 9.200E-01
61-PM-148 2.227E+01 4.300E-01 1.420E+01 2.672E+00 0.0
61-PM-149 2.377E+01 4.890E-01 8.141E+00 5.075E+00 9.900E-01
61-PM-150 2.270E+01 3.800E-01 7.943E+00 1.973E+00 0.0
62-SM-148 2.097E+01 5.505E-01 1.055E+00 6.694E+00 2.140E+00
62-SM-149 2.325E+01 5.052E-01 5.886E+00 5.504E+00 1.220E+00
62-SM-150 2.362E+01 5.230E-01 1.520E+00 6.973E+00 2.210E+00
62-SM-151 2.687E+01 5.000E-01 2.313E+01 6.327E+00 1.220E+00
---------------------------------------------------------------
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 5.475 FOR SM-150 AND 6.675 FOR SM-151.
REFERENCES
1) AOKI, T. ET AL.: PROC. INT. CONF. ON NUCLEAR DATA FOR BASIC
AND APPLIED SCIENCE, SANTA FE., VOL. 2, P.1627 (1985).
2) KAWAI, M. ET AL.: J. NUCL. SCI. TECHNOL., 29, 195 (1992).
3) KIKUCHI, Y. ET AL.: JAERI-M 86-030 (1986).
4) EILAND, H.M., ET AL.: NUCL. SCI. ENG., 54, 286 (1974).
5) ANUFRIEV, V.A., ET AL.: PROC. 4TH ALL UNION CONF. ON NEUTRON
PHYSICS, KIEV 1977, VOL.2, 263.
6) MUGHABGHAB, S.F.: "NEUTRON CROSS SECTIONS, VOL. I, PART B",
ACADEMIC PRESS (1984).
7) IGARASI, S. AND FUKAHORI, T.: JAERI 1321 (1991).
8) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987).
9) FOSTER, D.G. JR. AND GLASGOW, D.W.: PHYS. REV., C3, 576
(1971).
10) KELLIE, J.D., HALL, S.J. AND CRAWFORD, G.I. ET AL.:
J. PHYS., A7, 1758 (1974).
11) PEREY, F.G: PHYS. REV. 131, 745 (1963).
12) HUIZENGA, J.R. AND IGO, G.: NUCL. PHYS. 29, 462 (1962).
13) LOHR, J.M. AND HAEBERLI, W.: NUCL. PHYS. A232, 381 (1974).
14) 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).
15) GILBERT, A. AND CAMERON, A.G.W.: CAN. J. PHYS., 43, 1446
(1965).
16) IIJIMA, S., ET AL.: J. NUCL. SCI. TECHNOL. 21, 10 (1984).
17) GRUPPELAAR, H.: ECN-13 (1977).
18) MATSUMOTO, J.: PRIVATE COMMUNICATION (1981).
19) RAYNAL, J. CODE ECIS88
20) RAMAN, S. ET AL.:AT. DATA AND NUCL. DATA TABLES 36, 1 (1987).
21) SPEAR, R.H.: AT. DATA AND NUCL. DATA TABLES 42, 55 (1989).
22) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969).
23) WISSHAK, K. ET AL.: KFK 5067 (1992).
24) FORREST, R.A.: AERE-R 12419 (1986).
25) FREHAUT, J., ET AL.: SYMP. ON NEUTRON CROSS SECTIONS FROM
10-50MEV, BNL, P.399 (1980).