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  4. From x-ray telescopes to neutron scattering: Using axisymmetric mirrors to focus a neutron beam

From x-ray telescopes to neutron scattering: Using axisymmetric mirrors to focus a neutron beam

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Author(s)
Khaykovich, Boris
•
Gubarev, M. V.
•
Bagdasarova, Yelena S.
•
Ramsey, B. D.
•
Moncton, David E.
Date Issued
December 2010
Journal
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Publisher
Elsevier
Citation
Khaykovich, B. et al. “From x-ray telescopes to neutron scattering: Using axisymmetric mirrors to focus a neutron beam.” Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 631.1 (2011): 98-104.
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Author's final manuscript
Abstract
We demonstrate neutron beam focusing by axisymmetric mirror systems based on a pair of mirrors consisting of a confocal ellipsoid and hyperboloid. Such a system, known as a Wolter mirror configuration, is commonly used in x-ray telescopes. The axisymmetric Wolter geometry allows nesting of several mirror pairs to increase collection efficiency. We have implemented a system containing four nested Ni mirror pairs, which was tested by focusing a polychromatic neutron beam at the MIT Reactor. In addition, we have carried out extensive ray-tracing simulations of the mirrors and their performance in different situations. The major advantages of the Wolter mirrors are nesting for large angular collection, and aberration-free performance. We discuss how these advantages can be utilized to benefit various neutron scattering methods, such as imaging, SANS, and time-of-flight spectroscopy.
MIT Department
Massachusetts Institute of Technology. Department of Physics
MIT Nuclear Reactor Laboratory
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/61704
DOI of Published Version
https://doi.org/10.1016/j.nima.2010.11.110
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