60-Nd-150

 60-ND-150 JNDC       EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.        
                      DIST-MAR02 REV3-FEB02            20020222   
----JENDL-3.3         MATERIAL 6049                               
-----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/.                       
93-10 MODIFICATION FOR JENDL-3.2 WAS MADE.                        
      CONTRIBUTION OF THE DIRECT INELASTIC SCATTERING WAS         
      REPLACED BY A COUPLED-CHANNEL CALCULATION.                  
                                                                  
**** MODIFIED PARTS FOR JENDL-3.2 ********************************
(3,2),(3,4),(3,51),(3,52),(3,54),(3,56),(3,58)                    
(4,51),(4,52),(4,54),(4,56),(4,58)                                
******************************************************************
                                                                  
                                                                  
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 13.69 KEV)
    RESONANCE PARAMETERS WERE TAKEN FROM JENDL-2/3/.              
      NEUTRON WIDTHS WERE ADOPTED FROM TELLIER/4/.  RADIATION     
    WIDTHS WERE TAKEN FROM THE RECOMMENDATION BY MAGHABGHAB AND   
    GARBER/5/. THE AVERAGE RADIATION WIDTH OF 0.070 EV WAS ASSUMED
    FOR LEVELS WHICH HAD NO MEASURED RADIATION WIDTH.  A NEGATIVE 
    RESONANCE WAS ADDED SO AS TO REPRODUCE THE CAPTURE CROSS      
    SECTION OF 1.2+-0.2 BARNS AT 0.0253 EV /6/.                   
                                                                  
  UNRESOLVED RESONANCE REGION : 13.69 KEV - 100 KEV               
    UNRESOLVED RESONANCE PARAMETERS WERE ADOPTED FROM JENDL-2.    
    THE NEUTRON STRENGTH FUNCTIONS, S0, 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.                                                      
                                                                  
  TYPICAL VALUES OF THE PARAMETERS AT 70 KEV:                     
    S0 = 2.600E-4, S1 = 0.667E-4, S2 = 3.500E-4, SG = 3.39E-4,    
    GG = 0.037 EV, R  = 7.993 FM.                                 
                                                                  
  CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS)   
                     2200 M/S               RES. INTEG.           
      TOTAL           5.982                    -                  
      ELASTIC         4.780                    -                  
      CAPTURE         1.202                    15.9               
                                                                  
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 BY IIJIMA AND KAWAI/9/ TO REPRODUCE A SYSTEMATIC     
  TREND OF THE TOTAL CROSS SECTION.  THE OMP'S FOR CHARGED        
  PARTICLES ARE AS FOLLOWS:                                       
     PROTON   = PEREY/10/                                         
     ALPHA    = HUIZENGA AND IGO/11/                              
     DEUTERON = LOHR AND HAEBERLI/12/                             
     HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/13/            
  PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT   
  AND CAMERON/14/ WERE EVALUATED BY IIJIMA ET AL./15/  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
  /16/.                                                           
                                                                  
  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./17/.           
                                                                  
           NO.      ENERGY(MEV)    SPIN-PARITY    CC CAL.         
           GR.       0.0             0  +                         
            1        0.1301          2  +           *             
            2        0.3815          4  +           *             
            3        0.6767          0  +                         
            4        0.7212          6  +           *             
            5        0.8514          2  +                         
            6        0.9300          3  -           *             
            7        1.0624          2  +                         
            8        1.1307          8  +           *             
            9        1.1386          4  +                         
           10        1.3535          4  +                         
      LEVELS ABOVE 1.45 MEV WERE ASSUMED TO BE OVERLAPPING.       
                                                                  
    FOR THE LEVELS WITH AN ASTERISK, THE CONTRIBUTION OF DIRECT   
    INELASTIC SCATTERING CROSS SECTIONS WAS CALCULATED BY THE     
    ECIS-88 CODE/18/.  DEFORMATION PARAMETERS (BETA2 = 0.2848 AND 
    BETA3 = 0.070) WERE BASED ON THE DATA COMPILED BY RAMAN ET    
    AL./19/ AND SPEAR/20/, RESPECTIVELY.  THE COUPLING OF G.S.    
    ROTATIONAL BAND (0+,2+,4+,6+,8+,10+) AND OCTUPOLE VIBRATIONAL 
    BAND (1-,3-,5-) WAS CONSIDERED.  IN THE CC CALCULATION, THE   
    IMAGINARY SURFACE STRENGTH WAS REDUVED TO 7.35 MEV.           
                                                                  
  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/21/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV.       
                                                                  
    THE GAMMA-RAY STRENGTH FUNCTION (3.01E-04) WAS ADJUSTED TO    
    REPRODUCE THE CAPTURE CROSS SECTION OF 153 MILLI-BARNS AT 30  
    KEV MEASURED BY KONONOV ET AL./22/                            
                                                                  
  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 (=  10.0) WAS DETERMINED TO REPRODUCE
    ENERGY DEPENDENCE OF THE (N,2N) CROSS SECTION MEASURED BY     
    FREHAUT ET AL./23/                                            
                                                                  
    FINALLY, THE (N,P) CROSS SECTION WAS NORMALIZED TO THE        
    FOLLOWING VALUE AT 14.5 MEV:                                  
      (N,P)          1.61  MB (SYSTEMATICS OF FORREST/24/)        
    THE (N,2N) CROSS SECTION WAS DETERMINED BY EYE-GUIDING OF     
    THE DATA MEASURED BY FREHAUT 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.  CONTRIBUTION OF DIRECT INELASTIC       
  SCATTERING WAS CALCULATED WITH ECIS-88.  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  = 47.94                R0 = 6.748    A0 = 0.6          
        WS = 9.13                 RS = 7.598    AS = 0.45         
        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  SYST A(1/MEV)  T(MEV)    C(1/MEV)  EX(MEV)   PAIRING    
 ---------------------------------------------------------------  
 58-CE-146     1.918E+01 6.037E-01 1.355E+00 7.176E+00 2.160E+00  
 58-CE-147  *  2.514E+01 5.363E-01 2.925E+01 6.672E+00 1.170E+00  
 58-CE-148  *  2.454E+01 5.338E-01 2.640E+00 7.549E+00 2.280E+00  
 58-CE-149  *  2.392E+01 5.314E-01 1.525E+01 6.206E+00 1.170E+00  
                                                                  
 59-PR-147     2.440E+01 4.420E-01 3.742E+00 4.298E+00 9.900E-01  
 59-PR-148     1.996E+01 4.690E-01 1.108E+01 2.807E+00 0.0        
 59-PR-149  *  2.470E+01 5.314E-01 2.403E+01 6.371E+00 1.110E+00  
 59-PR-150  *  2.408E+01 5.290E-01 1.412E+02 5.027E+00 0.0        
                                                                  
 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  
 60-ND-150     2.415E+01 5.280E-01 1.867E+00 7.314E+00 2.290E+00  
 60-ND-151     2.618E+01 4.800E-01 1.152E+01 5.656E+00 1.180E+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 10.32 FOR ND-150 AND 5.0 FOR ND-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.: PROC. INT. CONF. ON NUCLEAR DATA FOR SCIENCE
    AND TECHNOLOGY, MITO, P. 569 (1988).                          
 3) KIKUCHI, Y. ET AL.: JAERI-M 86-030 (1986).                    
 4) TELLIER, H.: CEA-N-1459 (1971).                               
 5) MUGHABGHAB, S.F. AND GARBER, D.I.: "NEUTRON CROSS SECTIONS,   
    VOL.1, RESONANCE PARAMETERS", BNL 325, 3RD ED., VOL. 1,       
    (1973).                                                       
 6) FEDOROVA, A.F., ET AL.: "PROC. 3RD ALL-UNION CONF. ON NEUTRON 
    PHYSICS, KIEV 1975", VOL. 1, 169.                             
 7) IGARASI, S.: J. NUCL. SCI. TECHNOL., 12, 67 (1975).           
 8) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987).             
 9) IIJIMA, S. AND KAWAI, M.: J. NUCL. SCI. TECHNOL., 20, 77      
    (1983).                                                       
10) PEREY, F.G: PHYS. REV. 131, 745 (1963).                       
11) HUIZENGA, J.R. AND IGO, G.: NUCL. PHYS. 29, 462 (1962).       
12) LOHR, J.M. AND HAEBERLI, W.: NUCL. PHYS. A232, 381 (1974).    
13) 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).                                                       
14) GILBERT, A. AND CAMERON, A.G.W.: CAN. J. PHYS., 43, 1446      
    (1965).                                                       
15) IIJIMA, S., ET AL.: J. NUCL. SCI. TECHNOL. 21, 10 (1984).     
16) GRUPPELAAR, H.: ECN-13 (1977).                                
17) MATSUMOTO, J.: PRIVATE COMMUNICATION (1981).                  
18) RAYNAL, J.: PRIVATE COMMUNICATION.                            
19) RAMAN, S., ET AL.: ATOM. DATA AND NUCL. DATA TABLES 36, 1     
    (1987)                                                        
20) SPEAR, R.H.: ATOM. DATA AND NUCL. DATA TABLE, 42, 55 (1989).  
21) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969).                   
22) KONONOV, V.N., ET AL.: SOV. J. NUCL. PHYS., 27, 5 (1978).     
23) FREHAUT, J., ET AL.: SYMP. ON NEUTRON CROSS SECTIONS FROM     
    10-50MEV, BNL, P.399 (1980).                                  
24) FORREST, R.A.: AERE-R 12419 (1986).