B.J. Allen

The neutron capture cross section of natural silicon

Abstract The neutron capture cross section of natural silicon has been measured to 1500 keV using the capture cross section facility at the 40 m station of the Oak Ridge Electron Linear Accelerator. Analysis of the present data, in combination with existing total cross section information, has provided almost complete resonance data for 28Si. On the other hand, the capture kernel only ( gΓ n Γ γ Γ ) has been obtained for neutron capture resonances in 29Si and 30Si. A strong positive correlation has been observed between the radiative width and the corresponding reduced neutron width for p-wave resonances in 28Si, confirming significant valence effects. It is noted that a quantitative valence calculation provides only an approximate estimate of the valence strength for this nucleus. It was not possible to confirm from the present measurements, reported asymmetry observed in two resonances in the 29Si(γ, n) reaction.

Average neutron resonance parameters and radiative capture cross sectins for the isotopes of molybdenum

Abstract The neutron capture cross sections of the stable molybdenum isotopes have been measured with high energy resolution (ΔE/E ≲ 0.2 %), between 3 and 90 keV neutron energy, at the 40 m station of ORELA. Average resonance parameters are extracted for s- and p-wave resonances. The s-wave neutron strength function is close to 0.5 × 10−4 for all isotopes, but the p-wave strength function exhibits a well defined peak near A t~ 95. Both s- and p-wave radiative widths decrease markedly as further neutrons are added to the closed shell. The p-wave radiative widths are generally greater than the s-wave widths showing the presence of non-statistical γ-decay mechanisms. Valence neutron theory fails to explain the magnitude of the p- to s-wave radiative width disparity and doorway state processes are invoked. In particular, the data for 98Mo appear to violate the usual valence theory, since the correlations between radiative and neutron strengths are small. Further, the radiative widths are smaller than can be explained on the valence model. An explanation for the loss of valence strength is advanced. Interpolated resonance parameters allow an estimate for the unknown cross section for 99Mo(n, γ).

Valence neutron capture in 54Fe

Abstract The neutron capture cross section of 54 Fe has been measured with 0.2% energy resolution from 2.5 to 500 keV. A large and significant correlation is observed between the s-wave reduced neutron widths and the corresponding total radiative widths. The valence model readily accounts for this correlations as well as over half the average value of the s-wave radiative widths.

Resonance neutron capture in 56Fe

Abstract The neutron capture cross section of 56 Fe has been measured with 0.2–0.3% energy resolution from 2.5 keV up to the inelastic neutron scattering threshold. Results are compared with recent total cross-section data and average parameters are derived for s-, p- and d-wave resonances. The low correlation coefficient observed between the s-wave reduced neutron and radiative widths is consistent with the minor contribution of the valence capture mechanism as calculated in the framework of the optical model. Broad E1 and M1 doorway states for s-, p- and d-wave resonances are postulated to explain the cross-section data and γ-ray spectra up to 1 MeV.

AVERAGED INTENSITIES OF PRIMARY GAMMA RAYS AFTER keV NEUTRON CAPTURE IN COPPER.

Abstract The averaged intensities of high-energy gamma rays in copper have been measured with a Ge(Li) detector after the capture of 10–60 keV neutrons. The capture spectra represent the average strengths of transitions from a large number of resonances. They bear no relation to the thermal result, thus supporting the view that the latter proceeds through a non-compound nucleus mechanism. The ground state transition does not dominate the keV capture spectrum and the intensities indicate the presence of an E γ 3 energy dependence.

keV neutron capture in nickel

Abstract A Ge(Li) spectrometer has been used to observe gamma-ray transitions in three nickel isotopes after the capture of neutrons by natural nickel in the 10–95 keV energy range. Transitions to both l n = 1 and l n = 3 levels are observed, and the strengths of the high-energy transitions relative to thermal capture intensities are found to be substantially reduced. The energy dependence of the transition strengths in 59 Ni over a 3 MeV range is consistent with a statistical-model capture mechanism. The isotopic cross sections of nickel are estimated, and evidence is presented which discounts the presence of a dominant doorway state in the region of the binding energy of 63 Ni.

The neutron total and capture cross sections of 92, 94Zr☆

Abstract The neutron total and capture cross sections of92,94Zr have been measured at the 80 and 40 m flight stations, respectively, on the Oak Ridge Electron Linear Accelerator (ORELA). Resonance analysis of the total cross sections gave values of s, p 3 2 and p 1 2 strength functions. Strong intermediate structure was observed in the p 3 2 cross section of 92Zr. Significant single particle transitions identified in the p-wave capture cross section indicate the importance of the valence process for both nuclei. It is noted that the intermediate structure in the p 3 2 total cross section leads to enhanced valence effects in the capture cross section. The effects of non statistical E1 transitions following particle-hole annihilation in the compound states were not observed in either the 92Zr or 94Zr capture cross sections as they had been in that for 90Zr.

Valence neutron capture in 88Sr

Abstract The neutron capture cross section of 88Sr has been measured with high energy resolution between 2.5 and 400 keV using the capture cross-section facility at the 40 m station on the Oak Ridge Electron Linear Accelerator. Strong positive correlations have been observed between the reduced neutron and radiative widths for both p 3 2 and p 1 2 resonances. The valence process dominates the p-wave neutron capture mechanism. Comparison of calculated valence effects, using the optical model formulation of the valence theory, with the experimental data, indicates a reliability in the calculation of approximately 25%.

Resonant neutron capture in 40Ca

Abstract The neutron capture cross section of 40 Ca has been measured with ≈ 0.2 % energy resolution below E n = 300 keV. Resonance parameters have been extracted for many new p- and d-wave resonances. Gamma-ray spectra were also measured following capture in one doublet and two resolved resonances below 50 keV. Strong feeding of low-lying p-wave levels was observed in all cases. Calculations showed that valence transitions were inadequate to account for the observed dominance of these transitions and a further mechanism is required. The average resonance parameters obtained from the data are as follows: 〈 D 〉 = 37 + 4keV, 10 4 S 1 = 0.16 ± 0.05, 10 4 S 2 = 2.0 ± 0.7. The average radiative widths and standard deviations of their distributions were found to be strongly l -dependent as follows: 〈 Γ γ 〉 s = 1.5 ± 0.9 eV, 〈 Γ γ 〉 p = 0.36 ± 0.09 eV and 〈 Γ γ 〉 d = 0.7 ± 0.4 eV.

keV Neutron capture cross sections of 134Ba and 136Ba

Abstract The neutron capture cross sections of 134 Ba and 136 Ba have been measured in the energy region 3 to 100 keV. The following average quantities were deduced from the extracted resonance parameters: 〈 D 〉 = 127±10eV, 10 4 S 0 = 0.85±0.3, 10 4 S 1 = 0.8, 〈 Γ γ 〉 = 120±20 meV for 134 Ba. Analysis of the 136 Ba data gave 〈 Γ γ 〉 = 125±30meV for s-wave neutrons. The average 30 keV capture cross sections for these two s-process nuclei were found to be 225±35 mb for 134 Ba and 61±10 mb for 136 Ba .