50-Sn-124

 50-SN-124 JNDC       EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.        
                      DIST-SEP90 REV2-MAR93                       
----JENDL-3.2         MATERIAL 5061                               
-----INCIDENT NEUTRON DATA                                        
------ENDF-6 FORMAT                                               
HISTORY                                                           
90-03 NEW EVALUATION FOR JENDL-3 WAS COMPLETED BY JNDC FPND       
      W.G./1/                                                     
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 10.7 KEV       
    RESONANCE PARAMETERS AND SCATTERING RADIUS WERE BASED ON      
    MUGHABGHAB ET AL./2/  THE LEVELS WHOSE NEUTRON WIDTH WAS      
    UNKNOWN WERE ASSUMED TO BE P-WAVE RESONANCES, AND A REDUCED   
    NEUTRON WIDTH OF 830 MEV WAS TENTATIVELY GIVEN FOR THESE      
    LEVELS.  NEUTRON ORBITAL ANGULAR MOMENTUM L OF SOME RESONANCES
    WAS ESTIMATED WITH A METHOD OF BOLLINGER AND THOMAS/3/.       
    AVERAGED RADIATION WIDTH OF 140 MEV WAS DERIVED FROM THE      
    SYSTEMATICS OF MEASURED VALUES FOR NEIGHBORING NUCLIDES.  A   
    NEGATIVE RESONANCE WAS ADDED SO AS TO REPRODUCE THE THERMAL   
    CAPTURE AND ELASTIC SCATTERING CROSS SECTIONS GIVEN BY        
    MUGHABGHAB ET AL.                                             
                                                                  
  UNRESOLVED RESONANCE REGION : 10.7 KEV - 100 KEV                
    THE NEUTRON STRENGTH FUNCTION S0 WAS BASED ON THE COMPILATION 
    OF MUGHABGHAB ET AL., AND S1 AND S2 WERE CALCULATED WITH      
    OPTICAL MODEL CODE CASTHY/4/.  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 SYSTEMATICS OF        
    MEASURED VALUES FOR NEIGHBORING NUCLIDES.                     
                                                                  
  TYPICAL VALUES OF THE PARAMETERS AT 70 KEV:                     
    S0 = 0.150E-4, S1 = 2.600E-4, S2 = 0.680E-4, SG = 0.144E-4,   
    GG = 0.140 EV, R  = 5.979 FM.                                 
                                                                  
  CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS)   
                     2200 M/S               RES. INTEG.           
      TOTAL           4.535                    -                  
      ELASTIC         4.400                    -                  
      CAPTURE         0.1355                    7.86              
                                                                  
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/5/ STANDING ON A PREEQUILIBRIUM AND MULTI-STEP     
  EVAPORATION MODEL.  THE OMP'S FOR NEUTRON GIVEN IN TABLE 1 WERE 
  DETERMINED SO AS TO REPRODUCE A SYSTEMATIC TREND OF THE TOTAL   
  CROSS SECTION BY CHANGING RSO OF IIJIMA-KAWAI POTENTIAL/6/. THE 
  OMP'S FOR CHARGED PARTICLES ARE AS FOLLOWS:                     
     PROTON   = PEREY/7/                                          
     ALPHA    = HUIZENGA AND IGO/8/                               
     DEUTERON = LOHR AND HAEBERLI/9/                              
     HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/10/            
  PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT   
  AND CAMERON/11/ WERE EVALUATED BY IIJIMA ET AL./12/  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
  /13/.                                                           
                                                                  
  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 BASED ON EVALUATED NUCLEAR      
    STRUCTURE DATA FILE (1987 VERSION)/14/ AND NUCLEAR DATA       
    SHEETS/15/.                                                   
                                                                  
           NO.      ENERGY(MEV)    SPIN-PARITY                    
           GR.       0.0             0  +                         
            1        1.1316          2  +                         
            2        2.1016          4  +                         
            3        2.1293          0  +                         
            4        2.1294          2  +                         
            5        2.1920          2  +                         
            6        2.2045          5  -                         
            7        2.2215          2  +                         
            8        2.3249          7  -                         
            9        2.3664          2  +                         
           10        2.4264          2  +                         
           11        2.4469          8  +                         
           12        2.5680          6  -                         
           13        2.6024          2  +                         
           14        2.6142          3  -                         
           15        2.6866          0  +                         
           16        2.6887          1  -                         
           17        2.7029          4  +                         
           18        2.8363          2  +                         
           19        2.8751          2  +                         
           20        2.8783          2  +                         
      LEVELS ABOVE 2.9 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/16/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV.       
                                                                  
    THE GAMMA-RAY STRENGTH FUNCTION (0.1286-4) WAS ADJUSTED TO    
    REPRODUCE THE CAPTURE CROSS SECTION OF 8.3 MILLI-BARNS AT 90  
    KEV MEASURED BY TIMOKHOV ET AL./17/                           
                                                                  
  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 (= 215.9) WAS ESTIMATED BY THE       
    FORMULA DERIVED FROM KIKUCHI-KAWAI'S FORMALISM/18/ AND LEVEL  
    DENSITY PARAMETERS.                                           
                                                                  
    FINALLY, THE (N,P) CROSS SECTION WAS NORMALIZED TO THE        
    FOLLOWING VALUE AT 14.5 MEV:                                  
      (N,P)          1.56  MB (SYSTEMATICS OF FORREST/19/)        
                                                                  
  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    
 ---------------------------------------------------------------  
 48-CD-120  *  1.718E+01 6.016E-01 1.880E-01 7.009E+00 2.790E+00  
 48-CD-121  *  1.693E+01 5.992E-01 1.734E+00 5.442E+00 1.360E+00  
 48-CD-122  *  1.667E+01 5.968E-01 2.388E-01 6.394E+00 2.450E+00  
 48-CD-123  *  1.641E+01 5.943E-01 1.268E+00 5.165E+00 1.360E+00  
                                                                  
 49-IN-121     1.601E+01 6.060E-01 1.119E+00 5.277E+00 1.430E+00  
 49-IN-122  *  1.707E+01 5.968E-01 1.737E+01 4.092E+00 0.0        
 49-IN-123     1.470E+01 6.100E-01 1.134E+00 4.483E+00 1.090E+00  
 49-IN-124     1.655E+01 5.240E-01 6.345E+00 2.747E+00 0.0        
                                                                  
 50-SN-122     1.434E+01 7.060E-01 3.423E-01 7.416E+00 2.620E+00  
 50-SN-123     1.509E+01 6.870E-01 3.062E+00 6.032E+00 1.190E+00  
 50-SN-124     1.601E+01 6.160E-01 3.224E-01 6.294E+00 2.280E+00  
 50-SN-125     1.591E+01 6.210E-01 1.927E+00 5.249E+00 1.190E+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 7.975 FOR SN-124 AND 5.0 FOR SN-125.               
                                                                  
REFERENCES                                                        
 1) KAWAI, M. ET AL.: J. NUCL. SCI. TECHNOL., 29, 195 (1992).     
 2) MUGHABGHAB, S.F. ET AL.: "NEUTRON CROSS SECTIONS, VOL. I,     
    PART A", ACADEMIC PRESS (1981).                               
 3) BOLLINGER, L.M. AND THOMAS, G.E.: PHYS. REV., 171,1293(1968). 
 4) IGARASI, S. AND FUKAHORI, T.: JAERI 1321 (1991).              
 5) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987).             
 6) IIJIMA, S. AND KAWAI, M.: J. NUCL. SCI. TECHNOL., 20, 77      
    (1983).                                                       
 7) PEREY, F.G: PHYS. REV. 131, 745 (1963).                       
 8) HUIZENGA, J.R. AND IGO, G.: NUCL. PHYS. 29, 462 (1962).       
 9) LOHR, J.M. AND HAEBERLI, W.: NUCL. PHYS. A232, 381 (1974).    
10) 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).                                                       
11) GILBERT, A. AND CAMERON, A.G.W.: CAN. J. PHYS., 43, 1446      
    (1965).                                                       
12) IIJIMA, S., ET AL.: J. NUCL. SCI. TECHNOL. 21, 10 (1984).     
13) GRUPPELAAR, H.: ECN-13 (1977).                                
14) ENSDF: EVALUATED NUCLEAR STRUCTURE DATA FILE (JUNE 1987).     
15) NUCLEAR DATA SHEETS, 41, 413 (1984).                          
16) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969).                   
17) TIMOKHOV,V.M., ET AL.:???                                     
18) KIKUCHI, K. AND KAWAI, M.: "NUCLEAR MATTER AND NUCLEAR        
    REACTIONS", NORTH HOLLAND (1968).                             
19) FORREST, R.A.: AERE-R 12419 (1986).