54-Xe-130 JAEA EVAL-FEB22 S.Kunieda, A.Ichihara, K.Shibata+ DIST-DEC21 20100316 ----JENDL-5 MATERIAL 5443 -----INCIDENT NEUTRON DATA ------ENDF-6 FORMAT History 09-11 Re-evaluation was performed for JENDL-4.0 10-03 Compiled by S.Kunieda 21-11 revised by O.Iwamoto (MF8/MT4,16,17,22,28,32,102-104,107) JENDL/AD-2017 adopted (MF8/MT105,106) added (MF9/MT102,107) JENDL/AD-2017 adopted (MF10/MT16,103) JENDL/AD-2017 based 21-11 above 20 MeV, JENDL/ImPACT-2018 merged by O.Iwamoto 21-11 (MF6/MT5) recoil spectrum added by O.Iwamoto MF= 1 General information MT=451 Descriptive data and directory MF= 2 Resonance parameters MT=151 Resolved and unresolved resonance parameters - Resolved resonance region (MLBW formula): below 3.6 keV Resonance parameters of the positive 16 levels compiled in JENDL-3.3 were reexaminated on the basis of the measurements by Ribon et al./1/. As a result, a missing level at 2431.5 eV was found, and only one level at 126 eV measured by Mann et al./2/ was adopted as the 1st positive level. The orbital angular momentum l was assumed to be 0 for 18 resonance levels. The neutron widths were derived from the g*(neutron width) and total spin j=0.5 measured by Ribon et al. The radiation widths for the 6 levels were given by the measurements. For the remaining 11 levels whose radiation width was unknown, the weighted average 117.4762 eV derived from the radiation widths of the above 6 levels were adopted. The scattering radius was taken from the graph (fig. 1, Part A) given by Mughabghab et al./3/. A negative resonance level was added at -400 eV so as to reproduce the thermal capture cross section recommended by Mughabghab /4/. - Unresolved resonance region: 3.6 keV - 300 keV The parameters were obtained by fitting to the total and capture cross sections calculated by the POD code /5/. The ASREP code /6/ was employed in this evaluation. The unresolved parameters should be used only for self-shielding calculation. Thermal cross sections & resonance integrals at 300 K ---------------------------------------------------------- 0.0253 eV res. integ. (*) (barns) (barns) ---------------------------------------------------------- Total 1.75366E+01 Elastic 1.27253E+01 n,gamma 4.81133E+00 2.87879E+01 ---------------------------------------------------------- (*) Integrated from 0.5 eV to 10 MeV. MF= 3 Neutron cross sections MT= 1 Total cross section Sum of partial cross sections. MT= 2 Elastic scattering cross section The OPTMAN /7/ & POD /5/ calculations. MT= 3 Non-elastic cross section Sum of partial non-elastic cross sections. MT= 4,51-91 (n,n') cross section The OPTMAN /7/ & POD /5/ calculations. MT= 16 (n,2n) cross section MT= 17 (n,3n) cross section MT= 22 (n,na) cross section MT= 28 (n,np) cross section MT= 32 (n,nd) cross section Calculated by the POD code /5/. MT=102 Capture cross section Calculated by the POD code /5/. The value of gamma-ray strength function was determined to reproduce experimental capture cross sections measured by Reifarth et al /8/. 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,a) cross section Calculated by the POD code /5/. MT=203 (n,xp) cross section Sum of (n,np) and (n,p) MT=204 (n,xd) cross section Sum of (n,nd) and (n,d) MT=205 (n,xt) cross section MT=206 (n,xHe3) cross section Calculated by the POD code /5/. MT=207 (n,xa) cross section Sum of (n,na) and (n,a) MF= 4 Angular distributions of emitted neutrons MT= 2 Elastic scattering The OPTMAN /7/ & POD /5/ calculations. MF= 6 Energy-angle distributions of emitted particles MT= 16 (n,2n) reaction MT= 17 (n,3n) reaction MT= 22 (n,na) reaction MT= 28 (n,np) reaction MT= 32 (n,nd) reaction Neutron spectra calculated by the POD code /5/. MT= 51-90 (n,n') reaction Neutron angular distributions calculated by OPTMAN /7/ & POD /5/. MT= 91 (n,n') reaction Neutron spectra calculated by the POD code /5/. MT= 203 (n,xp) reaction MT= 204 (n,xd) reaction MT= 205 (n,xt) reaction MT= 206 (n,xHe3) reaction MT= 207 (n,xa) reaction Light-ion spectra calculated by the POD code /6/. MF=12 Gamma-ray multiplicities MT= 3 Non-elastic gamma emission Calculated by the POD code /5/. MF=14 Gamma-ray angular distributions MT= 3 Non-elastic gamma emission Assumed to be isotropic. MF=15 Gamma-ray spectra MT= 3 Non-elastic gamma emission Calculated by the POD code /5/. *************************************************************** * Nuclear Model Calculations with POD Code /5/ * *************************************************************** 1. Theoretical models The POD code is based on the spherical optical model, the distorted-wave Born approximaiton (DWBA), one-component exciton preequilibrium model, and the Hauser-Feshbach-Moldauer statis- tical model. With the preequilibrium model, semi-empirical pickup and knockout process can be taken into account for composite-particle emission. The gamma-ray emission from the compound nucleus can be calculated within the framework of the exciton model. The code is capable of reading in particle transmission coefficients calculated by separate spherical or coupled-channel optical model code. In this evaluation, the OPTMAN code /7/ was employed for neutrons, while the ECIS code /9/ was adopted for charged particles. 2. Optical model & parameters Neutrons: Model: The coupled-channel method based on the rigid-rotor model was adopted. Deformation parameter beta2 was taken from ref./10/ OMP : Coupled-channel optical potential /11/ was applied. Protons: Model: Spherical OMP : Koning and Delaroche /12/ Deuterons: Model: Spherical OMP : Bojowald et al. /13/ Tritons: Mode: Spherical OMP : Becchetti and Greenlees /14/ He-3: Model: Spherical OMP : Becchetti and Greenlees /14/ Alphas: Model: Spherical OMP : A simplified folding model potential /15/ (The nucleon OMP was taken from Ref./11/.) 3. Level scheme of Xe-130 ------------------------------------ No. Ex(MeV) J PI CC ------------------------------------ 0 0.00000 0 + * 1 0.53609 2 + * 2 1.12215 2 + 3 1.20461 4 + * 4 1.59030 4 - 5 1.63253 3 + 6 1.79354 0 + 7 1.80818 4 + 8 1.94409 6 + * 9 2.01709 0 + 10 2.05960 5 - 11 2.08196 4 + 12 2.10338 4 - 13 2.15021 2 + 14 2.17164 5 + 15 2.22352 4 + 16 2.24298 3 + 17 2.29610 2 + 18 2.30779 2 + 19 2.31000 5 - 20 2.34596 6 - 21 2.36208 5 + 22 2.37520 7 - 23 2.38622 4 - 24 2.42717 4 + 25 2.44203 6 - 26 2.49412 1 - 27 2.50223 1 + 28 2.53340 2 - 29 2.54445 1 + ------------------------------------ Levels above 2.55445 MeV are assumed to be continuous. 4. Level density parameters Energy-dependent parameters of Mengoni-Nakajima /16/ were used ---------------------------------------------------------- Nuclei a* Pair Esh T E0 Ematch Elv_max 1/MeV MeV MeV MeV MeV MeV MeV ---------------------------------------------------------- Xe-131 16.786 1.048 -0.172 0.686 -1.237 7.025 0.700 Xe-130 16.030 2.105 0.158 0.675 0.108 7.673 2.544 Xe-129 16.580 1.057 0.970 0.676 -1.490 7.279 0.589 Xe-128 15.820 2.121 1.127 0.604 0.631 6.688 1.430 I -130 15.945 0.000 -0.675 0.824 -3.544 8.206 0.070 I -129 15.256 1.057 -0.097 0.711 -0.934 6.797 1.204 I -128 16.654 0.000 0.643 0.666 -2.328 5.906 0.345 Te-128 15.820 2.121 -0.935 0.757 -0.307 8.631 2.488 Te-127 18.544 1.065 0.107 0.594 -0.817 6.052 0.764 Te-126 16.022 2.138 0.369 0.688 -0.104 8.045 2.182 ---------------------------------------------------------- 5. Gamma-ray strength functions M1, E2: Standard Lorentzian (SLO) E1 : Generalized Lorentzian (GLO) /17/ 6. Preequilibrium process Preequilibrium is on for n, p, d, t, He-3, and alpha. Preequilibrium capture is on. References 1) Ribon, P. et al.: CEA-N-1149 (1969). 2) Mann, D.P. et al.: Phys. Rev., 116, 1516 (1959). 3) Mughabghab, S.F. et al.: "Neutron Cross Sections, Vol. I, Part A", Academic Press (1981). 4) S.F.Mughabghab, "Atlas of Neutron Resonances", Elsevier (2006). 5) A.Ichihara et al., JAEA-Data/Code 2007-012 (2007). 6) Y.Kikuchi et al., JAERI-Data/Code 99-025 (1999) [in Japanese]. 7) E.Soukhovitski et al., JAERI-Data/Code 2005-002 (2005). 8) Reifarth et al., Phys. Rev. C66, 064603 (2002). 9) J.Raynal, CEA Saclay report, CEA-N-2772 (1994). 10) S.Raman et al., At. Data and Nucl. Data Tables 78, 1 (1995) 11) S.Kunieda et al., J. Nucl. Sci. Technol. 44, 838 (2007). 12) A.J.Koning, J.P.Delaroche, Nucl. Phys. A713, 231 (2003). 13) Bojowald et al., Phys. Rev. C 38, 1153 (1988). 14) F.D.Becchetti,Jr., G.W.Greenlees, "Polarization Phenomena in Nuclear Reactions," p.682, The University of Wisconsin Press (1971). 15) D.G.Madland, NEANDC-245 (1988), p. 103. 16) A.Mengoni, Y.Nakajima, J. Nucl. Sci. Technol. 31, 151 (1994). 17) M.Brink, Ph.D thesis, Oxford University, 1955.