He-3 neutron polarising filters - theoretical comparison with supermirrorsand Heusler alloy polarisers

Citation
Ld. Cussen et al., He-3 neutron polarising filters - theoretical comparison with supermirrorsand Heusler alloy polarisers, NUCL INST A, 440(2), 2000, pp. 409-420
Citations number
27
Categorie Soggetti
Spectroscopy /Instrumentation/Analytical Sciences","Instrumentation & Measurement
Journal title
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
ISSN journal
01689002 → ACNP
Volume
440
Issue
2
Year of publication
2000
Pages
409 - 420
Database
ISI
SICI code
0168-9002(20000201)440:2<409:HNPF-T>2.0.ZU;2-2
Abstract
There is currently intense interest in the development of gaseous He-3 neut ron polarising transmission filters. The key areas of development are incre asing the currently achievable levels of nuclear spin polarisation, pi, wit hin the He-3 gas and improving the reliability of the devices. Recent work has identified "quality factors" which can be used to determine the optimum thickness of such filters under various experimental conditions. The best achievable quality factor for a He-3 polariser with a given pi is determine d. It is demonstrated that the optimum filter thickness depends only weakly on pi and is always approximately given by the dimensionless expression rh o sigma lambda t = 3.4 where rho is the density of He-3 atoms in the filter , sigma is the absorption cross section at a wavelength of 1 Angstrom, lamb da is the neutron wavelength in Angstrom and t is the filter thickness. Qua lity factors are calculated for existing types of neutron polariser (superm irrors and Heusler alloy monochromators) as a function of instrumental para meters. These results are used to determine the "break even" point for the new polarisers - the pi needed for the new polarisers to outperform existin g types of polarisers. A quantitative discussion of regimes of usefulness o f the different polariser types for all common instrument types is presente d. (C) 2000 Elsevier Science B.V. All rights reserved.