36-Kr- 78

 36-KR- 78 JNDC       EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.        
                      DIST-MAR02 REV2-FEB02            20020222   
----JENDL-3.3         MATERIAL 3625                               
-----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                                                           
90-03 NEW EVALUATION FOR JENDL-3 WAS COMPLETED BY JNDC FPND       
      W.G./1/                                                     
                                                                  
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 0.8 KEV        
    RESONANCE PARAMETERS FOR THREE POSITIVE LEVELS WERE BASED ON  
    MUGHABGHAB ET AL./2/  RESONANCE LEVELS AT 0.1719 KEV AND ABOVE
    1.136 KEV WERE ABANDONED, BECAUSE THEY BELONG POSSIBLY TO     
    KR-80.  THE VALUES OF NEUTRON ORBITAL ANGULAR MOMENTUM L AND  
    TOTAL SPIN J WERE ASSUMED TO BE 0 AND 0.5 FOR ALL RESONANCE   
    LEVELS, RESPECTIVELY.  SCATTERING RADIUS WAS ALSO TAKEN FROM  
    THE GRAPH (FIG. 1, PART A) GIVEN BY MUGHABGHAB ET AL.  A      
    NEGATIVE RESONANCE WAS ADDED SO AS TO REPRODUCE THE THERMAL   
    CAPTURE CROSS SECTION OF 6.2+-0.9 BARNS GIVEN BY MUGHABGHAB ET
    AL.                                                           
                                                                  
  UNRESOLVED RESONANCE REGION : 0.8 KEV - 100 KEV                 
    THE NEUTRON STRENGTH FUNCTIONS, S0 AND S2 WERE CALCULATED WITH
    OPTICAL MODEL CODE CASTHY/3/, AND S1 WAS BASED ON THE         
    SYSTEMATICS OF MUGHABGHAB ET AL.  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.                                          
                                                                  
  TYPICAL VALUES OF THE PARAMETERS AT 70 KEV:                     
    S0 = 0.580E-4, S1 = 1.700E-4, S2 = 0.730E-4, SG = 13.0E-4,    
    GG = 0.230 EV, R  = 7.556 FM.                                 
                                                                  
  CALCULATED 2200-M/S CROSS SECTIONS AND RES. INTEGRALS (BARNS)   
                     2200 M/S               RES. INTEG.           
      TOTAL          14.03                     -                  
      ELASTIC         7.829                    -                  
      CAPTURE         6.200                    25.8               
                                                                  
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/4/ 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 R0, RS AND RSO OF IIJIMA-KAWAI POTENTIAL/5/.
  THE OMP'S FOR CHARGED PARTICLES ARE AS FOLLOWS:                 
     PROTON   = PEREY/6/                                          
     ALPHA    = HUIZENGA AND IGO/7/                               
     DEUTERON = LOHR AND HAEBERLI/8/                              
     HELIUM-3 AND TRITON = BECCHETTI AND GREENLEES/9/             
  PARAMETERS FOR THE COMPOSITE LEVEL DENSITY FORMULA OF GILBERT   
  AND CAMERON/10/ WERE EVALUATED BY IIJIMA ET AL./11/  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
  /12/.                                                           
                                                                  
  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)/13/ AND AND NUCLEAR DATA   
    SHEETS/14/.                                                   
                                                                  
           NO.      ENERGY(MEV)    SPIN-PARITY                    
           GR.       0.0             0  +                         
            1        0.4550          2  +                         
            2        1.0172          0  +                         
            3        1.1195          4  +                         
            4        1.1479          2  +                         
            5        1.5647          3  +                         
            6        1.6538          3  +                         
            7        1.7559          2  +                         
            8        1.7729          2  +                         
            9        1.8729          4  +                         
           10        1.9778          6  +                         
           11        2.0075          0  -                         
           12        2.2341          2  +                         
           13        2.2407          2  +                         
           14        2.2998          5  +                         
           15        2.3990          3  -                         
           16        2.4134          2  +                         
           17        2.4434          1  -                         
           18        2.4718          2  +                         
           19        2.5080          0  +                         
           20        2.5733          2  +                         
           21        2.6561          0  +                         
           22        2.6776          3  -                         
           23        2.7315          6  +                         
           24        2.7498          5  -                         
           25        2.7641          3  -                         
           26        2.8821          3  -                         
           27        2.8828          1  -                         
           28        2.9925          0  +                         
           29        2.9933          8  +                         
      LEVELS ABOVE 2.999 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/15/ AND NORMALIZED TO 1 MILLI-BARN AT 14 MEV.       
                                                                  
    THE GAMMA-RAY STRENGTH FUNCTION (10.3E-04) WAS ADJUSTED TO    
    REPRODUCE THE CAPTURE CROSS SECTION OF 200 MILLI-BARNS AT 100 
    KEV MEASURED BY WALTER ET AL./16/                             
                                                                  
  MT = 16  (N,2N) 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 =106  (N,HE3) CROSS SECTION                                  
  MT =107  (N,ALPHA) CROSS SECTION                                
  MT =111  (N,2P) CROSS SECTION                                   
    THESE REACTION CROSS SECTIONS WERE CALCULATED WITH THE        
    PREEQUILIBRIUM AND MULTI-STEP EVAPORATION MODEL CODE PEGASUS. 
                                                                  
    THE KALBACH'S CONSTANT K (=  85.5) WAS ESTIMATED BY THE       
    FORMULA DERIVED FROM KIKUCHI-KAWAI'S FORMALISM/17/ 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)       245.00  MB (MEASURED BY KONDAIAH+/18/)         
      (N,P)        131.00  MB (SYSTEMATICS OF FORREST/19/)        
      (N,ALPHA)     39.30  MB (SYSTEMATICS OF 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.  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  = 46.0-0.25E           R0 = 5.7      A0 = 0.62         
        WS = 7.0                  RS = 6.2      AS = 0.35         
        VSO= 7.0                  RSO= 5.7      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    
 ---------------------------------------------------------------  
 34-SE- 74     1.290E+01 8.620E-01 1.070E+00 9.612E+00 2.860E+00  
 34-SE- 75     1.391E+01 8.500E-01 9.741E+00 8.707E+00 1.430E+00  
 34-SE- 76     1.315E+01 8.900E-01 1.097E+00 1.082E+01 3.310E+00  
 34-SE- 77     1.438E+01 8.000E-01 7.140E+00 8.015E+00 1.430E+00  
                                                                  
 35-BR- 75  *  1.407E+01 8.667E-01 1.329E+01 9.176E+00 1.430E+00  
 35-BR- 76  *  1.467E+01 8.553E-01 9.334E+01 7.957E+00 0.0        
 35-BR- 77  *  1.440E+01 8.442E-01 7.380E+00 9.395E+00 1.880E+00  
 35-BR- 78     1.394E+01 7.570E-01 2.113E+01 5.482E+00 0.0        
                                                                  
 36-KR- 76  *  1.425E+01 8.553E-01 3.339E+00 1.024E+01 2.600E+00  
 36-KR- 77     1.359E+01 8.250E-01 7.930E+00 7.711E+00 1.170E+00  
 36-KR- 78     1.322E+01 8.690E-01 1.155E+00 1.019E+01 3.050E+00  
 36-KR- 79     1.369E+01 8.400E-01 9.969E+00 8.080E+00 1.170E+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 6.780 FOR KR- 78 AND 5.0 FOR KR- 79.               
                                                                  
REFERENCES                                                        
 1) KAWAI, M. ET AL.: PROC. INT. CONF. ON NUCLEAR DATA FOR SCIENCE
    AND TECHNOLOGY, MITO, P. 569 (1988).                          
 2) MUGHABGHAB, S.F. ET AL.: "NEUTRON CROSS SECTIONS, VOL. I,     
    PART A", ACADEMIC PRESS (1981).                               
 3) IGARASI, S.: J. NUCL. SCI. TECHNOL., 12, 67 (1975).           
 4) IIJIMA, S. ET AL.: JAERI-M 87-025, P. 337 (1987).             
 5) IIJIMA, S. AND KAWAI, M.: J. NUCL. SCI. TECHNOL., 20, 77      
    (1983).                                                       
 6) PEREY, F.G: PHYS. REV. 131, 745 (1963).                       
 7) HUIZENGA, J.R. AND IGO, G.: NUCL. PHYS. 29, 462 (1962).       
 8) LOHR, J.M. AND HAEBERLI, W.: NUCL. PHYS. A232, 381 (1974).    
 9) 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).                                                       
10) GILBERT, A. AND CAMERON, A.G.W.: CAN. J. PHYS., 43, 1446      
    (1965).                                                       
11) IIJIMA, S., ET AL.: J. NUCL. SCI. TECHNOL. 21, 10 (1984).     
12) GRUPPELAAR, H.: ECN-13 (1977).                                
13) ENSDF: EVALUATED NUCLEAR STRUCTURE DATA FILE (JUNE 1987).     
14) NUCLEAR DATA SHEETS, 33, 189 (1981).                          
15) BENZI, V. AND REFFO, G.: CCDN-NW/10 (1969).                   
16) WALTER, G., ET AL.: KFK-3652, 1 (1984).                       
17) KIKUCHI, K. AND KAWAI, M.: "NUCLEAR MATTER AND NUCLEAR        
    REACTIONS", NORTH HOLLAND (1968).                             
18) KONDAIAH, E., ET AL.: NUCL. PHYS., A120, 337 (1968)           
19) FORREST, R.A.: AERE-R 12419 (1986).