60-Nd-142

 60-ND-142 JNDC       EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.        
                      DIST-SEP90 REV2-NOV93                       
----JENDL-3.2         MATERIAL 6025                               
-----INCIDENT NEUTRON DATA                                        
------ENDF-6 FORMAT                                               
HISTORY                                                           
84-10 EVALUATION FOR JENDL-2 WAS MADE BY JNDC FPND W.G./1/        
90-03 MODIFICATION FOR JENDL-3 WAS MADE/2/.                       
93-11 JENDL-3.2 WAS MADE BY JNDC FPND W.G.                        
                                                                  
     *****   MODIFIED PARTS FOR JENDL-3.2   ********************  
      (2,151)       RESOLVED RESONANCE PARAMETERS                 
     ***********************************************************  
                                                                  
                                                                  
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 26.0 KEV) 
    RESONANCE PARAMETERS WERE TAKEN FROM JENDL-2/3/ AFTER THE     
    FOLLOWING MODIFICATION.                                       
       EVALUATION FOR JENDL-2 WAS MADE BY MAINLY ON THE BASIS OF  
    THE DATA MEASURED BY TELLIER/4/ AND MUSGROVE ET AL./5/        
    RESONANCE ENERGIES WERE ADJUSTED TO THOSE OF TELLIER.  AVERAGE
    RADIATION WIDTHS WERE ASSUMED TO BE 0.078 EV FOR S-WAVE AND   
    SOME LARGE P-WAVE RESONANCES AND TO BE 0.046 EV FOR P-WAVE    
    ONES.                                                         
       FOR JENDL-3, PARAMETERS OF A NEGATIVE RESONANCE WAS        
    MODIFIED SO AS TO REPRODUCE THE THERMAL CAPTURE CROSS SECTION 
    OF 18.7+-0.7 BARNS/6/ AND THE RESONANCE INTEGRAL.  HOWEVER,   
    THE CALCULATED RESONANCE INTEGRAL IS STILL TOO SMALL.         
      FOR JENDL-3.2, THESE RESONANCE PARAMETERS WERE MODIFIED SO  
    AS TO REPRODUCE THE CAPTURE AREA DATA MEASURED AT ORNL, BY    
    TAKING ACCOUNT OF THE CORRECTION FACTOR (0.967) ANNOUNCED BY  
    ALLEN ET AL./7/.  THE PARAMETERS OF A NEGATIVE RESONANCE AND  
    SCATTERING RADIUS WERE ADJUSETED TO GET BETTER AGREEMENT WITH 
    RECOMMENDED THERMAL CROSS SECTIONS/8/.                        
                                                                  
  UNRESOLVED RESONANCE REGION : 26 KEV - 100 KEV                  
    THE NEUTRON STRENGTH FUNCTIONS S0 AND S1 WERE BASED ON THE    
    COMPILATION OF MUGHABGHAB ET AL./8/, AND S2 WAS CALCULATED    
    WITH OPTICAL MODEL CODE CASTHY/9/.  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 WIDTHS GG(S) AND GG(P) WERE BASED  
    ON THE COMPILATION OF MUGHABGHAB ET AL.                       
                                                                  
  TYPICAL VALUES OF THE PARAMETERS AT 70 KEV:                     
    S0 = 1.500E-4, S1 = 0.400E-4, S2 = 1.700E-4, SG(S)= 1.24E-4,  
    SG(P)=0.828E-4, GG(S)=0.064 EV, GG(P)= 0.044 EV, R= 5.805 FM. 
                                                                  
  CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS)   
                     2200 M/S               RES. INTEG.           
      TOTAL          26.400                    -                  
      ELASTIC         7.700                    -                  
      CAPTURE        18.700                     8.68              
                                                                  
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/10/ STANDING ON A PREEQUILIBRIUM AND MULTI-STEP    
  EVAPORATION MODEL.  THE OMP'S FOR NEUTRON GIVEN IN TABLE 1 WERE 
  ADOPTED FROM THE PARAMETERS DETERMINED BY IIJIMA AND KAWAI/11/  
  FOR ND-143.  THE OMP'S FOR CHARGED PARTICLES ARE AS FOLLOWS:    
     PROTON   = PEREY/12/                                         
     ALPHA    = HUIZENGA AND IGO/13/                              
     DEUTERON = LOHR AND HAEBERLI/14/                             
     HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/15/            
  PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT   
  AND CAMERON/16/ WERE EVALUATED BY IIJIMA ET AL./17/  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
  /18/.                                                           
                                                                  
  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./19/.           
                                                                  
           NO.      ENERGY(MEV)    SPIN-PARITY    DWBA CAL.       
           GR.       0.0             0  +                         
            1        1.5757          2  +             *           
            2        2.0844          3  -             *           
            3        2.1010          4  +                         
            4        2.2090          6  +                         
            5        2.2172          0  +                         
            6        2.3400          2  +                         
            7        2.3846          1  +                         
            8        2.5833          2  +                         
            9        2.8000          4  +                         
           10        2.8459          2  +                         
           11        2.9780          0  +                         
      LEVELS ABOVE 3.008 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/20/.  DEFORMATION PARAMETERS (BETA2 = 0.0926 AND 
    BETA3 = 0.109) WERE BASED ON THE DATA COMPILED BY RAMAN ET    
    AL./21/ AND SPEAR/22/, 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/23/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV.       
                                                                  
    THE GAMMA-RAY STRENGTH FUNCTION (0.969E-4) WAS ADJUSTED TO    
    REPRODUCE THE CAPTURE CROSS SECTION OF 59.0 MILLI-BARNS AT 30 
    KEV MEASURED BY MUSGROVE ET AL./5,7/                          
                                                                  
  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 =103  (N,P) CROSS SECTION                                    
  MT =104  (N,D) CROSS SECTION                                    
  MT =105  (N,T) CROSS SECTION                                    
  MT =106  (N,HE3) 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 (= 213.8) WAS ESTIMATED BY THE       
    FORMULA DERIVED FROM KIKUCHI-KAWAI'S FORMALISM/24/ 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)         13.80  MB (RECOMMENDED BY FORREST/25/)        
      (N,ALPHA)      6.80  MB (RECOMMENDED BY FORREST)            
                                                                  
  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  = 45.76                R0 = 6.73     A0 = 0.6          
        WS = 6.97                 RS = 6.417    AS = 0.45         
        VSO= 7.0                  RSO= 6.678    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-138  *  1.618E+01 5.580E-01 2.611E-01 5.011E+00 1.870E+00  
 58-CE-139     1.374E+01 6.450E-01 9.282E-01 4.685E+00 1.170E+00  
 58-CE-140     1.413E+01 6.541E-01 3.376E-01 5.852E+00 2.020E+00  
 58-CE-141     1.714E+01 5.150E-01 7.134E-01 3.957E+00 1.170E+00  
                                                                  
 59-PR-139  *  1.630E+01 5.556E-01 2.158E+00 3.843E+00 7.000E-01  
 59-PR-140     1.448E+01 6.430E-01 7.927E+00 3.814E+00 0.0        
 59-PR-141     1.400E+01 6.500E-01 1.810E+00 4.559E+00 8.500E-01  
 59-PR-142     1.595E+01 6.150E-01 1.201E+01 3.974E+00 0.0        
                                                                  
 60-ND-140  *  1.641E+01 5.532E-01 2.596E-01 5.024E+00 1.880E+00  
 60-ND-141     1.477E+01 6.091E-01 9.537E-01 4.587E+00 1.180E+00  
 60-ND-142     1.288E+01 6.710E-01 2.250E-01 5.526E+00 2.030E+00  
 60-ND-143     1.826E+01 4.710E-01 5.220E-01 3.613E+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 5.579 FOR ND-142 AND 7.227 FOR ND-143.             
                                                                  
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    (1987)                                                        
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