Status of the NIST spin filter project
Journal of Neutron Research, 1996
Abstract Polarized 3He has long been recognized as a promising candidate for producing beams of p... more Abstract Polarized 3He has long been recognized as a promising candidate for producing beams of polarized neutrons by selective absorption of one neutron spin state from an initially unpolarized beam. This technique has advantages over the traditional supermirror technique in that the neutron beams produced have less divergence added by the polarization technique (an advantage for SANS applications), lower backgrounds from gamma production (mainly important for fundamental physics research), and most importantly. 3He can polarize thermal and epi-thermal neutrons as well as cold neutrons. We are pursuing parallel efforts at NIST to produce a practical spin filter either by polarizing 3He using spin-exchange with optically pumped alkali vapors or by direct optical pumping of metastable. 3He followed by compression with a mechanical pump. The status and prospects of both of these projects are reported in this paper.
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Papers by Alan Thompson
yields are comparable to the yields from some liquid and solid neutron scintillators. At noble gas pressures of 107 kPa, the number of photons produced per neutron absorbed following irradiation of a 1200 nm thick 10B film was 14 000 for xenon, 11 000 for krypton, and 6000 for argon. The absolute scintillation yields from the experimental configuration were calculated using data from (1) experimental irradiations, (2) thin-film characterizations, (3) photomultiplier tube calibrations, and (4) photon collection modeling. Both the boron films and the photomultiplier tube were characterized at the National Institute of Standards and Technology. Monte Carlo modeling of the reaction cell provided estimates of the photon collection efficiency and the transport behavior of 10B(n,a)7Li reaction products escaping the thin films. Scintillation yields increased with gas pressure due to increased ionization and excitation densities of the gases from the 10B(n,a)7Li reaction products, increased frequency of three-body, excimer-forming collisions, and reduced photon emission volumes (i.e., larger solid angle) at higher pressures. Yields decreased for thicker 10B thin films due to higher average energy loss of the 10B(n,a)7Li reaction products escaping the films. The relative standard uncertainties in the measurements were determined to lie between 14% and 16%. The observed scintillation signal demonstrates that noble gas excimer scintillation is promising for use in practical neutron detectors.