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49-In-115 JNDC EVAL-MAR90 JNDC FP NUCLEAR DATA W.G. DIST-JAN09 20090105 ----JEFF-311 MATERIAL 4931 -----INCIDENT NEUTRON DATA ------ENDF-6 FORMAT *************************** JEFF-3.1.1 ************************* ** ** ** Original data taken from: JEFF-3.1 ** ** ** ****************************************************************** ***************************** JEFF-3.1 ************************* ** ** ** Original data taken from: JENDL-3.3 ** ** ** ****************************************************************** =========================================================== 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/. 93-03 JENDL-3.2 WAS MADE BY JNDC FPND W.G. ***** 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. *********************************************************** 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 2 KEV RESONANCE PARAMETERS OF JENDL-2 WERE MODIFIED AS FOLLOWS: FOR JENDL-2, PARAMETERS WERE TAKEN FROM THE EXPERIMENT BY HACKEN ET AL./3/ ANGULAR MOMENTUM L AND SPIN J WERE BASED ON THE MEASUREMENT OF CORVI AND STEFANON/4/. THE AVERAGE RADIATION WIDTH OF 0.085 EV WAS DEDUCED /3/ AND APPLIED TO THE LEVELS WHOSE RADIATION WIDTH WAS UNKNOWN. FOR JENDL-3, TOTAL SPIN J OF SOME RESONANCES WAS TENTATIVE- LY ESTIMATED WITH A RANDOM NUMBER METHOD. UNRESOLVED RESONANCE REGION : 2 KEV - 100 KEV PARAMETERS WERE TAKEN FROM JENDL-2. THE NEUTRON STRENGTH FUNCTIONS, S0, S1 AND S2 WERE CALCULATED WITH OPTICAL MODEL CODE CASTHY/5/. 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 ET AL./6/ TYPICAL VALUES OF THE PARAMETERS AT 70 KEV: S0 = 0.760E-4, S1 = 2.700E-4, S2 = 0.760E-4, SG = 95.0E-4, GG = 0.077 EV, R = 5.539 FM. CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS) 2200 M/S RES. INTEG. TOTAL 203.5 - ELASTIC 2.526 - CAPTURE 201.0 3210 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/7/ 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/8/. THE OMP'S FOR CHARGED PARTICLES ARE AS FOLLOWS: PROTON = PEREY/9/ ALPHA = HUIZENGA AND IGO/10/ DEUTERON = LOHR AND HAEBERLI/11/ HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/12/ PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT AND CAMERON/13/ WERE EVALUATED BY IIJIMA ET AL./14/ 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 /15/. 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./16/. NO. ENERGY(MEV) SPIN-PARITY GR. 0.0 9/2 + 1 0.3362 1/2 - 2 0.5970 3/2 - 3 0.8284 3/2 + 4 0.8640 1/2 + 5 0.9336 7/2 + 6 0.9412 5/2 + 7 1.0780 5/2 + 8 1.1325 11/2 + 9 1.2905 13/2 + 10 1.4180 9/2 + 11 1.4487 9/2 + 12 1.4625 7/2 + 13 1.4858 9/2 + LEVELS ABOVE 1.5 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/17/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV. THE GAMMA-RAY STRENGTH FUNCTION (9.37E-03) WAS ADJUSTED TO REPRODUCE THE NATURAL IN CAPTURE CROSS SECTION OF 460 MILLI-BARNS AT 80 KEV MEASURED BY KOMPE /18/, SHORIN ET AL./19/ AND KONONOV ET AL./20/ 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 (= 138.9) WAS ESTIMATED BY THE FORMULA DERIVED FROM KIKUCHI-KAWAI'S FORMALISM/21/ 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) 8.00 MB (RECOMMENDED BY FORREST/22/) (N,ALPHA) 2.40 MB (RECOMMENDED BY FORREST) THE (N,2N) CROSS SECTION WAS DETERMINED BY EYE-GUIDING OF THE DATA MEASURED BY SANTRY ET AL./23/ 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 = 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 --------------------------------------------------------------- 47-AG-111 1.955E+01 5.810E-01 6.505E+00 5.835E+00 1.140E+00 47-AG-112 * 1.857E+01 6.210E-01 4.959E+01 5.129E+00 0.0 47-AG-113 * 1.837E+01 6.185E-01 5.132E+00 6.321E+00 1.320E+00 47-AG-114 * 1.816E+01 6.161E-01 3.785E+01 4.871E+00 0.0 48-CD-112 1.797E+01 6.190E-01 6.327E-01 7.351E+00 2.500E+00 48-CD-113 1.973E+01 5.760E-01 4.397E+00 6.018E+00 1.360E+00 48-CD-114 1.910E+01 6.010E-01 5.651E-01 7.611E+00 2.680E+00 48-CD-115 2.072E+01 5.570E-01 4.805E+00 5.966E+00 1.360E+00 49-IN-113 1.885E+01 5.070E-01 1.371E+00 4.280E+00 1.140E+00 49-IN-114 1.632E+01 5.290E-01 6.292E+00 2.752E+00 0.0 49-IN-115 1.600E+01 6.510E-01 2.555E+00 5.941E+00 1.320E+00 49-IN-116 1.710E+01 5.650E-01 1.250E+01 3.562E+00 0.0 --------------------------------------------------------------- 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 8.461 FOR IN-115 AND 5.0 FOR IN-116. 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) HACKEN, G., ET AL.: PHYS. REV., C10, 1910 (1974). 4) CORVI, F. AND STEFANON, M.: NUCL. PHYS., A233, 185 (1974). 5) IGARASI, S. AND FUKAHORI, T.: JAERI 1321 (1991). 6) MUGHABGHAB, S.F. ET AL.: "NEUTRON CROSS SECTIONS, VOL. I, PART A", ACADEMIC PRESS (1981). 7) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987). 8) IIJIMA, S. AND KAWAI, M.: J. NUCL. SCI. TECHNOL., 20, 77 (1983). 9) PEREY, F.G: PHYS. REV. 131, 745 (1963). 10) HUIZENGA, J.R. AND IGO, G.: NUCL. PHYS. 29, 462 (1962). 11) LOHR, J.M. AND HAEBERLI, W.: NUCL. PHYS. A232, 381 (1974). 12) 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). 13) GILBERT, A. AND CAMERON, A.G.W.: CAN. J. PHYS., 43, 1446 (1965). 14) IIJIMA, S., ET AL.: J. NUCL. SCI. TECHNOL. 21, 10 (1984). 15) GRUPPELAAR, H.: ECN-13 (1977). 16) LEDERER, C.M., ET AL.: "TABLE OF ISOTOPES, 7TH ED.", WILEY- INTERSCIENCE PUBLICATION (1978). 17) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969). 18) KOMPE, D.: NUCL. PYS., A133, 513 (1969). 19) SHORIN, V.S., ET AL.: YADERNYA FIZIKA, 19, 5 (1974). 20) KONONOV, V.N. ET AL.: YADERNYA KONSTANTY, 22, 29 (1977). 21) KIKUCHI, K. AND KAWAI, M.: "NUCLEAR MATTER AND NUCLEAR REACTIONS", NORTH HOLLAND (1968). 22) FORREST, R.A.: AERE-R 12419 (1986). 23) SANTRY,D.C., ET AL.: CAN. J. PHYS., 54, 757 (1976)Back |