Measurement of thermal neutron radiative capture cross-sections of the 14N and 19F by in-beam γ-spectroscopy method with reactor neutrons

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Abstract

The cross-sections of the 14N(n) 15N and 19F(n) 20F reactions were measured by γ-spectroscopy method with the target placed at the end of a neutron guide of the WWR-M reactor (PNPI, Gatchina). The neutron spectrum was measured by the TOF method. The maximum of the spectrum is located at 0.028(2) eV and FWHM is about 0.03 eV. Cross-section of radiative neutron capture in aluminium and absolute γ-intensities of the 1779 and 1633 keV γ-lines from beta decay of the 28Al and 20F, respectively, and the prompt 1678 and 1885 keV γ-lines from the 14N(n,γ) 15N reaction were taken as standards. The thermal neutron radiative cross-sections of the 14N and 19F were measured to be 0.0795(13) and 0.00950(15)b, respectively. New value of the γ-intensity of the 1678 keV γ-line from the 14N(n,γ) 15N reaction has been proposed.

Introduction

The determination of the neutron radiative capture cross-sections (NRCCS) by the measurement of intensities of prompt γ-rays from the (n,γ)-reaction has a high level of discrimination against impurity effects in objects which are available as chemical compounds only. It is just the case for nitrogen and fluorine. This method compares the (n,γ)-spectrum of the element with unknown cross-section with the (n,γ)-spectrum of a standard. Knowledge of the decay schemes for both nuclei is required to determine the NRCCS.

The thermal NRCCS of the 14N was measured by this method at McMaster University Reactor [1] and at Los Alamos Omega West Reactor [2]. Targets consisting of melamin were placed in the tangential facility with Maxwellian neutron spectrum [1] and in thermal column [2] of these reactors. The corresponding value of the 19F was measured at Los Alamos [3] with Teflon target in the same conditions as in Ref. [2]. These research groups used for the NRCCS's determination a considerable amount of σγ and γ-intensity standards which was taken from a literature. It should be noted that the neutron spectrum in Los Alamos experiments had approximately Maxwellian form, with the most probable neutron velocity being 2400 m/s. Authors of McMaster and Los Alamos works presented the final NRCCS values reduced to the most probable neutron velocity Vn=2200m/s (En=0.0253eV).

Described in the present study is the application of this method for the 14N and 19F NRCCS measurements performed at the external thermal neutron beam of the WWR-M reactor (PNPI, Gatchina) with narrow, not Maxwellian form, neutron spectrum (maximum at En=0.028(2)eV, FWHM about 0.03 eV and the most probable neutron velocity Vn=2200m/s). The NRCCS values were determined using significantly less number of standards than in above-mentioned works (Refs. [1], [2], [3]).

Section snippets

Foundation of method

Capture γ-ray spectroscopy method involves the detection of the prompt γ-rays emitted following neutron capture and of photons accompanying beta decay of the residual nuclei. The essence of the method is a comparison of the areas of γ-lines resulting from neutron capture in isotope under investigation and in isotope used as standard. As both isotopes should be irradiated in one and the same neutron flux, the homogeneous mixture of their chemical compounds is used as a target. Such a target is

Neutron spectrum

Neutron guide installed inside biological shielding brings the thermal neutrons out of the reactor. The neutron spectrum measured by the TOF method is shown in Fig. 1. The shape of the spectrum is not Maxwellian. It is narrow and contains neither epithermal nor fast neutrons, the maximum is located at 0.028(2) eV and FWHM is about 0.03 eV. The neutron flux at the sample site amounts to 2×107 n cm−2 s−1.

Detection efficiency

The energy dependence of HPGe γ-detector efficiency was determined using a set of radioactive

Nitrogen cross-section

The absolute intensities of the 1678 and 1885 keV γ-transitions from the 14N(n,γ) 15N reaction were measured at Los Alamos [2] and McMaster [7] reactors. The data from both works agree closely except the data for the 1678 keV γ-line, for which the intensities differ by 0.73(20)γ/100n. We prefer the Los Alamos [2] value because:

  • (i)

    it was obtained with γ-spectrometer operated both in Compton-suppressed and pair mode, whereas McMaster measurements [7] were performed using only the pair mode, with low γ

Conclusion

The method described could be applied for the refinement (up to 1.5–2%) of the known NRCCS's of isotopes, provided that both appropriate absolute γ-intensities and cross-section standards are available. The application of this method is restricted mainly by the scarcity of the absolute γ-intensity standards of high accuracy (1–2%) in the range 1.5–11 MeV. The precision of majority of these values at the moment does not exceed 10–20% and cannot be used as standards. There are few nuclei where

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