52-Te-120 JNDC       EVAL-MAR90 JNDC FP NUCLEAR DATA W.G.        
                      DIST-MAY10                       20091211   
----JENDL-4.0         MATERIAL 5225                               
-----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.       
90-03 New evaluation for JENDL-3 was completed by JNDC FPND       
09-12 JENDL-4.0.                                                  
      Compiled by A.Ichihara (jaea/ndc).                          
      *****   modified parts for JENDL-4.0   *******************  
      (2,151)      Unresolved resonance parameters were updated.  
mf = 1  General information                                       
  mt=451 Comments and dictionary                                  
mf = 2  Resonance parameters                                      
  mt=151 Resolved and unresolved resonance parameters             
  No resolved resonance parameters                                
  Unresolved resonance region : 68 eV - 300 keV                   
    The neutron strength functions, S0, S1 and S2 were calculated 
    with optical model code CASTHY/2/.  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 = 0.970e-4, S1 = 1.700e-4, S2 = 1.100e-4, Sg = 7.72e-4,    
    Gg = 0.100 eV, R  = 5.376 fm.                                 
    The unresolved resonance parameters were recalculated using   
    the ASREP code/18/.                                           
    The parameters should be used only for self-shielding         
    Thermal cross sections and resonance integrals at 300 K       
                     0.0253 eV           res. integ. (*)          
                      (barns)              (barns)                
     Total            6.014E+00                                   
     Elastic          3.656E+00                                   
     n,gamma          2.341E+00             2.25E+01              
       (*) Integrated from 0.5 eV to 10 MeV.                      
mf = 3  Neutron cross sections                                    
  Below 68 eV, the capture and elastic scattering cross sections  
  were assumed to be in 1/v form and constant, respectively.  The 
  capture cross section at 0.0253 was adopted from Ref./3/ and    
  the elastic scattering cross section was estimated from r = 5.4 
  fm.  Unresolved resonance parameters were given in the energy   
  range from 68 eV to 300 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 so as to reproduce a systematic trend of the total   
  cross section by changing r0 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
  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 Nuclear Data       
           no.      energy(MeV)    spin-parity                    
           gr.       0.0             0  +                         
            1        0.5604          2  +                         
            2        1.1031          0  +                         
            3        1.1615          4  +                         
            4        1.2017          2  +                         
            5        1.7762          6  +                         
            6        1.8635          3  +                         
            7        2.0834          3  -                         
            8        2.1085          1  +                         
      Levels above 2.202 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 (7.41e-04) was determined from
    the systematics of radiation width (0.1 eV) and the average   
    s-wave resonance level spacing (135 eV) calculated from the   
    level density parameters.                                     
  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 (= 135.2) was estimated by the       
    formula derived from Kikuchi-Kawai's formalism/16/ 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)         26.60  mb (systematics of Forrest/17/)        
      (n,alpha)     12.30  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.                               
                DEPTH (MEV)       RADIUS(FM)    DIFFUSENESS(FM)   
         ----------------------   ------------  ---------------   
        V  = 45.97-0.199E         R0 = 6.481    A0 = 0.62         
        WS = 6.502                RS = 6.926    AS = 0.35         
        VSO= 7.0                  RSO= 6.49     ASO= 0.62         
TABLE 2  LEVEL DENSITY PARAMETERS                                 
 50-SN-116     1.529E+01 6.680E-01 3.763E-01 7.111E+00 2.510E+00  
 50-SN-117     1.583E+01 5.960E-01 1.352E+00 4.804E+00 1.190E+00  
 50-SN-118     1.633E+01 6.140E-01 3.341E-01 6.448E+00 2.340E+00  
 50-SN-119     1.635E+01 5.990E-01 1.772E+00 5.050E+00 1.190E+00  
 51-SB-117  *  1.902E+01 6.089E-01 5.934E+00 6.380E+00 1.320E+00  
 51-SB-118  *  1.880E+01 6.064E-01 4.497E+01 4.927E+00 0.0        
 51-SB-119  *  1.858E+01 6.040E-01 5.801E+00 5.944E+00 1.150E+00  
 51-SB-120  *  1.834E+01 6.016E-01 3.366E+01 4.659E+00 0.0        
 52-TE-118  *  1.918E+01 6.064E-01 9.376E-01 7.533E+00 2.460E+00  
 52-TE-119     1.819E+01 6.210E-01 6.418E+00 6.117E+00 1.140E+00  
 52-TE-120     1.700E+01 5.940E-01 3.471E-01 6.309E+00 2.290E+00  
 52-TE-121     1.800E+01 6.200E-01 5.720E+00 6.022E+00 1.140E+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 6.375 for Te-120 and 5.0 for Te-121.               
 1) Kawai, M. et al.: Proc. Int. Conf. on Nuclear Data for Science
    and Technology, Mito, p. 569 (1988).                          
 2) Igarasi, S.: J. Nucl. Sci. Technol., 12, 67 (1975).           
 3) Mughabghab, S.F. et al.: "Neutron Cross Sections, Vol. I,     
    Part A", Academic Press (1981).                               
 4) Iijima, S. et al.: JAERI-M 87-025, p. 337 (1987).             
 5) Iijima, S. and Kawai, M.: J. Nucl. Sci. Technol., 20, 77      
 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.      
10) Gilbert, A. and Cameron, A.G.W.: Can. J. Phys., 43, 1446      
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, 17, 39 (1976).                           
15) Benzi, V. and Reffo, G.: CCDN-NW/10 (1969).                   
16) Kikuchi, K. and Kawai, M.: "Nuclear Matter and Nuclear        
    Reactions", North Holland (1968).                             
17) Forrest, R.A.: AERE-R 12419 (1986).                           
18) Y.Kikuchi et al., JAERI-Data/Code 99-025 (1999)               
    [in Japanese].