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24-Cr- 54 ORNL EVAL-NOV89 HETRICK,D.C. & N.M. LARSON,FU ORNL/TM DIST-JAN09 20090105 ----JEFF-311 MATERIAL 2437 -----INCIDENT NEUTRON DATA ------ENDF-6 FORMAT *************************** JEFF-3.1.1 ************************* ** ** ** Original data taken from: JEFF-3.1 ** ** ** ****************************************************************** ***************************** JEFF-3.1 ************************* ** ** ** Original data taken from: JEFF-3.0 ** ** ** ****************************************************************** ***************************** JEFF-3.0 ************************* DATA TAKEN FROM :- ENDF/B-VI.3 (DIST-JUN90) ****************************************************************** **************************************************************** ENDF/B-VI MOD 3, October 1997 (V. McLane, NNDC) 1. Residual nucleus and AWR corrected in File 6, MT=16. 2. File 1 comments revised. **************************************************************** ENDF/B-VI MOD 2, July 1991. 1. The secondary particle distributions for MF=6,MT=51-54 were corrected to center-of-mass, from laboratory coordinates. 2. The elastic transformation matrix was removed. **************************************************************** ENDF/B-VI MOD 1 Evaluation, November 1989. D. Hetrick, D. Larson, N. Larson, C. Fu, ORNL This work employed the Hauser-Feshbach code TNG [1,2,3]. The TNG code provides energy and angular distributions of particles emitted in the compound and pre-compound reactions, ensures consistency among all reactions, and maintains energy balance. Details pertinent to the contents of this evaluation will be published at a later date. Description of files ------------------------------------------- (MF-MT) 1-451 General information, references, and definitions. 2-151 Resonance parameters; used to provide the total, scattering, and capture cross sections from 1.E-5 eV to 900 keV. The resonance parameters are taken from Agrawal et al. [4] and Allen and Musgrove [5], and readjusted to attempt to match the thermal values. A background file in 3-1 is used from 11-900 keV. Note that the flag has been set to allow user calculation of the angular distributions from the R-Matrix resonance parameters, if the user wants angular distributions on a finer energy grid than given in 4-2. 3-1 Total cross section; given by resonance parameters up to 900 keV with negative energy resonances adjusted to give measured thermal scattering and capture cross sections. Above 900 keV, isotopic data used to 4.0 MeV from Harvey and Agrawal [6] and from 4.0-20.0 MeV high resolution natural Cr transmission measurements were used from Larson et al. [7]. 3-2 Elastic scattering cross sections were obtained by subtracting the nonelastic from the total 3-3 Nonelastic cross section; sum of 3-4, 3-16, 3-102, 3-103, and 3-107. 3-4 Total inelastic cross section; sum of 3-51, 3-52, ... ...,3-54, and 3-91 3-16 (n,2n) cross section; calculated by the TNG code [1,2,3]. No data available. 3-51 to 3-54 Inelastic scattering exciting levels; results are from TNG [1,2,3]. 3-91 Inelastic scattering exciting the continuum; Calculated by TNG. 3-102 (n,g) capture cross section; given by resonance parameters up to 900 keV; from 900 keV to 20 MeV, TNG calculations were used but normalized to measured average capture between 100 keV and 900 keV. TNG calculations included a precompound component and weighted cross sections from all isotopes of Cr give 0.82 mb at 14.5 MeV, in agreement with the measurement of 0.75 mb for natural Cr. 3-103 (n,p) cross section; calculated by the TNG code [1,2,3] Calculations agree well with data. 3-107 (n,a) cross section; calculated by the TNG code [1,2,3]. Calculations agree well with data. 4-2 Angular distributions of secondary neutrons for elastic scattering; from ENDF/B-V. If desired, angular distributions can be calculated by the user on a finer energy grid from the R-Matrix resonance parameters in 2-151. 6-16 (n,2n) reaction; includes simple constant yields for the neutron and 53Cr residual, and energy dependent yield based on TNG calculated gamma-ray spectra for the gamma ray; TNG calculated normalized distributions are given for each product. Isotropy is assumed. 6-51 through 6-54 Inelastic scattering exciting levels; assumed isotropic. 6-91 Inelastic scattering exciting the continuum; includes simple constant yields for the neutron and 54Cr residual and energy dependent yield based on TNG calculated gamma- ray spectra for the gamma ray; TNG calculated normalized distributions are given for each. Isotropy is assumed. 6-103 (n,p) reaction; includes simple constant yields for p and 54V residual, and energy dependent yield based on calculated gamma-ray spectra for gamma ray; calculated normalized distributions are given for each product. Isotropy is assumed. 6-107 (n,a) reaction; includes simple constant yields for a and 51Ti residual, and energy dependent yield based on calculated gamma-ray spectra for gamma ray; calculated normalized distributions are given for each product. Isotropy is assumed. 12-51 through 12-54 Branching ratios for the levels are given. 12-102 (n,g) capture; TNG calculated. 14-51 through 14-54 and 14-102 Gamma ray angular distributions assumed to be isotropic. 15-102 (n,g) capture; TNG calculated. ---------------------------------------------------------------- Uncertainty files An LB=8 section is included for all non-derived files as required by ENDF/B-VI. 33-1 Uncertainties are derived from 1.E-5 to 100 eV. From 100 eV to 20 MeV they are explicit, using LB=0,1 and 8. 33-2 From 1.E-5 to 100 eV, uncertainties are explicit, based upon thermal uncertainty and other data. From 100 eV to 20 MeV the files are derived. 33-3 From 1.E-5 to 900 keV uncertainties are derived. From 900 keV to 20 MeV uncertainties are explicit, using LB=1 and 8. 33-4 Uncertainties are all derived. 33-16 Uncertainties for (n,2n) are explicit, estimated from TNG. 33-51 through 3-91 Uncertainties for inelastic scattering are explicit, based on data and calculation uncertainties. 33-102 Uncertainties are explicit, based on thermal data at low energies, and calculated results above 900 keV. 33-103 Uncertainties estimated from TNG. 33-107 Uncertainties estimated from TNG. ---------------------------------------------------------------- REFERENCES: [1] C.Y. Fu, "A consistent nuclear model for compound and precompound reactions with conservation of angular momentum," Oak Ridge National Laboratory report ORNL/TM-7042 (1980) and Nucl.Sci.Eng. 100, 61 (1988). [2] C.Y Fu, "Development and application of multi-step Hauser-Feshbach/pre-equilibrium model theory," Neutron Cross Sections from 10 to 50 MeV, Symp., Upton, N.Y., May 12-14, 1980, Brookhaven National Laboratory report BNL-NCS-51425 (1980) p.675. [3] K. Shibata and C.Y. Fu, "Recent Improvements of the TNG Statistical Model Code", Oak Ridge National Laboratory report ORNL/TM-10093 (1986). [4] H.M. Agrawal, J.B. Garg, and J.A. Harvey, Phys. Rev. C 30, 1880 (1984). [5] B.J. Allen and A.R. De L. Musgrove, "S-wave Resonance Parameters in the Structural Materials," Neutron Data of Structural Materials for Fast Reactors, Proc. Specialists' Meeting, Geel, Belgium, Dec. 5-8, 1977. [6] J.A. Harvey and H.M. Agrawal, private comm., 1988. [7] D.C. Larson, J.A. Harvey, and N.W. Hill, private comm., 1988; data available at NNDC.Back |