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56-Ba-138 JNDC EVAL-MAR90 JNDC FP NUCLEAR DATA W.G. DIST-JAN09 20090105 ----JEFF-311 MATERIAL 5649 -----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/. 93-10 JENDL-3.2 WAS MADE BY JNDC FPND W.G. ***** MODIFIED PARTS FOR JENDL-3.2 ******************** (2,151) RESOLVED RESONANCE PARAMETERS (3,102) RE-NORMALIZATION (3,2), (3,4), (3,51-91) AND ANGULAR DISTRIBUTIONS SMALL EFFECTS OF THE RE-NORMALIZATION OF CAPTURE CROSS SECTION. ( < 0.3% ) *********************************************************** MF = 1 GENERAL INFORMATION MT=451 COMMENTS AND DICTIONARY MF = 2 RESONANCE PARAMETERS MT=151 RESOLVED AND UNRESOLVED RESONANCE PARAMETERS RESOLVED RESONANCE PARAMETERS FOR MLBW FORMULA (BELOW 100 KEV) FOR JENDL-2, EVALUATION WAS MADE BY KIKUCHI /3/ MAINLY ON THE BASIS OF THE DATA MEASURED BY MUSGROVE ET AL./4/ UP TO 92 KEV. ABOVE 100 KEV, NEUTRON WIDTHS WERE ADOPTED FROM BILPUCH ET AL./5/ AVERAGE CAPTURE WIDTHS WERE ASSUMED TO BE 0.055+- 0.020 EV FOR S-WAVE RESONANCES AND 0.045+-0.020 EV FOR P-WAVE ONES, AND TO BE 0.095 EV IN THE ENERGY RANGE ABOVE 100 KEV. A NEGATIVE RESONANCE WAS ADDED AT -6.22 KEV SO AS TO REPRODUCE THE CAPTURE CROSS SECTION OF 0.360+-0.036 BARNS AT 0.0253 EV/6/. FOR JENDL-3, 10 RESONANCES WERE NEWLY ASIGNED BY TAKING THE EXPERIMENTAL DATA BY MIZUMOTO/7/ IN THE ENERGY RANGE FROM 648 EV TO 63.12 KEV. TOTAL SPIN J OF SOME RESONANCES WAS TENTA- TIVELY ESTIMATED WITH A RANDOM NUMBER METHOD NO UNRESOLVED RESONANCE REGION CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS) 2200 M/S RES. INTEG. TOTAL 5.9090 - ELASTIC 5.5499 - CAPTURE 0.3591 0.265 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/8/, BY TAKING ACCOUNT OF COMPETING REACTIONS, OF WHICH CROSS SECTIONS WERE CALCULATED WITH PEGASUS/9/ 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 BA-NAT. TOTAL CROSS SECTION BY CHANGING WS AND RSO OF IIJIMA-KAWAI POTENTIAL /10/. 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/. NO. ENERGY(MEV) SPIN-PARITY DWBA CAL. GR. 0.0 0 + 1 1.4359 2 + * 2 1.8987 4 + 3 2.0907 6 + 4 2.1896 2 + 5 2.2032 6 + 6 2.2180 2 + 7 2.3077 4 + 8 2.4156 5 + 9 2.4457 3 + 10 2.5832 1 + 11 2.5840 4 + 12 2.6396 2 + 13 2.7795 4 + 14 2.8517 3 + 15 2.8810 3 - * 16 2.9315 1 + 17 2.9912 3 + 18 3.0500 2 + 19 3.1560 4 + LEVELS ABOVE 3.164 MEV WERE ASSUMED TO BE OVERLAPPING. FOR THE LEVELS WITH AN ASTERISK, THE CONTRIBUTION OF DIRECT INELASTIC SCATTERING CROSS SECTIONS WAS CALCULATED BY THE DWUCK-4 CODE/19/. DEFORMATION PARAMETERS (BETA2 = 0.0925 AND BETA3 = 0.118) WERE BASED ON THE DATA COMPILED BY RAMAN ET AL./20/ AND SPEAR/21/, RESPECTIVELY. 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 (2.54E-06) WAS ADJUSTED TO THE CAPTURE CROSS SECTION OF 2.7 MILLI-BARNS AT 700 KEV SO AS TO REPRODUCE THE CROSS SECTION MEASURED BY JOHNSRUD ET AL./23/ AND STAVISSKIJ AND TOLSTIKOV/24/ 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 =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 (= 144.6) WAS ESTIMATED BY THE FORMULA DERIVED FROM KIKUCHI-KAWAI'S FORMALISM/25/ AND LEVEL DENSITY PARAMETERS. FINALLY, THE (N,2N), (N,P) AND (N,ALPHA) CROSS SECTIONS WERE NORMALIZED TO THE FOLLOWING VALUES AT 14.5 MEV: (N,2N) 1750.00 MB (SYSTEMATICS OF WEN DEN LU+/26/) (N,P) 2.80 MB (MEASURED BY IKEDA+/27/) (N,ALPHA) 2.10 MB (MEASURED BY IKEDA+) 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. CONTRIBUTION OF DIRECT INELASTIC SCATTERING WAS CALCULATED WITH DWUCK-4. FOR OTHER REACTIONS, ISOTROPIC DISTRIBUTIONS 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 = 41.8 R0 = 6.89 A0 = 0.62 WS = 2.95+0.789E RS = 7.098 AS = 0.35 VSO= 7.0 RSO= 6.89 ASO= 0.62 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 --------------------------------------------------------------- 54-XE-134 1.400E+01 6.300E-01 3.184E-01 5.224E+00 1.820E+00 54-XE-135 1.550E+01 5.565E-01 7.506E-01 4.010E+00 1.120E+00 54-XE-136 1.400E+01 6.500E-01 3.270E-01 5.679E+00 1.970E+00 54-XE-137 1.550E+01 5.565E-01 7.470E-01 4.010E+00 1.120E+00 55-CS-135 1.343E+01 6.537E-01 1.831E+00 4.203E+00 7.000E-01 55-CS-136 1.400E+01 6.000E-01 4.424E+00 2.967E+00 0.0 55-CS-137 1.336E+01 6.200E-01 9.986E-01 3.836E+00 8.500E-01 55-CS-138 1.470E+01 5.737E-01 4.715E+00 2.858E+00 0.0 56-BA-136 1.610E+01 6.500E-01 5.721E-01 6.928E+00 2.280E+00 56-BA-137 1.645E+01 5.640E-01 5.394E-01 4.905E+00 1.580E+00 56-BA-138 1.390E+01 7.200E-01 4.123E-01 7.233E+00 2.430E+00 56-BA-139 2.022E+01 4.800E-01 5.326E-01 4.629E+00 1.580E+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 7.914 FOR BA-138 AND 5.0 FOR BA-139. 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) MUSGROVE, A.R. DE L., ET AL.: AUST. J. PHYS., 32, 213 (1979). 5) BILPUCH, E.G., ET AL.: ANN. PHYS., 14, 387 (1961). 6) MUGHABGHAB, S.F. ET AL.: "NEUTRON CROSS SECTIONS, VOL. I, PART A", ACADEMIC PRESS (1981). 7) MIZUMOTO, M.: J. NUCL. SCI. ENG., 25, 757 (1988). 8) IGARASI, S. AND FUKAHORI, T.: JAERI 1321 (1991). 9) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987). 10) IIJIMA, S. AND KAWAI, M.: J. NUCL. SCI. TECHNOL., 20, 77 (1983). 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) KUNZ, P.D.: PRIVATE COMMUNICATION. 20) RAMAN, S., ET AL.: ATOM. DATA AND NUCL. DATA TABLES 36, 1 (1987) 21) SPEAR, R.H.: ATOM. DATA AND NUCL. DATA TABLE, 42, 55 (1989). 22) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969). 23) JOHNSRUD, A.E. ET AL.: PHYS. REV., 116, 927 (1959). 24) STAVISSKIJ, JU.JA. AND TOLSTIKOV, V.A.: AT. ENERGIJA, 10, 508 (1961). EXFOR 40642004. 25) KIKUCHI, K. AND KAWAI, M.: "NUCLEAR MATTER AND NUCLEAR REACTIONS", NORTH HOLLAND (1968). 26) WEN DEN LU AND FINK, R.W.: PHYS. REV., C4, 1173 (1971). 27) IKEDA, Y. ET AL.: JAERI 1312 (1988).Back |