Solid deuterium surface degradation at ultracold neutron sources

A. Anghel, T. L. Bailey, G. Bison, B. Blau, L. J. Broussard, S. M. Clayton, C. Cude-Woods, M. Daum, A. Hawari, N. Hild, P. Huffman, T. M. Ito, K. Kirch, E. Korobkina, B. Lauss, K. Leung, E. M. Lutz, M. Makela, G. Medlin, C. L. MorrisR. W. Pattie, D. Ries, A. Saunders, P. Schmidt-Wellenburg, V. Talanov, A. R. Young, B. Wehring, C. White, M. Wohlmuther, G. Zsigmond

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

Solid deuterium (sD 2 is used as an efficient converter to produce ultracold neutrons (UCN). It is known that the sD 2 must be sufficiently cold, of high purity and mostly in its ortho-state in order to guarantee long lifetimes of UCN in the solid from which they are extracted into vacuum. Also the UCN transparency of the bulk sD 2 material must be high because crystal inhomogeneities limit the mean free path for elastic scattering and reduce the extraction efficiency. Observations at the UCN sources at Paul Scherrer Institute and at Los Alamos National Laboratory consistently show a decrease of the UCN yield with time of operation after initial preparation or later treatment (“conditioning”) of the sD 2. We show that, in addition to the quality of the bulk sD 2 , the quality of its surface is essential. Our observations and simulations support the view that the surface is deteriorating due to a build-up of D 2 frost-layers under pulsed operation which leads to strong albedo reflections of UCN and subsequent loss. We report results of UCN yield measurements, temperature and pressure behavior of deuterium during source operation and conditioning, and UCN transport simulations. This, together with optical observations of sD 2 frost formation on initially transparent sD 2 in offline studies with pulsed heat input at the North Carolina State University UCN source, results in a consistent description of the UCN yield decrease.

Original languageEnglish
Article number148
JournalEuropean Physical Journal A
Volume54
Issue number9
DOIs
StatePublished - Sep 1 2018

Funding

This work was supported in part by the US Department of Energy under Grant No. DE-FG02-97ER41042 and the US National Science Foundation under grant number NSF-1615153. PSI acknowledges the support by the Swiss National Science Foundation Projects 200020 137664, 200020 149813, and 200020 163413, support by the proton accelerator operations and UCN source operations groups, support by P. Erismann, M. Meier and C. Zoller, and access to the computing grid infrastructure PL-Grid [58]. We acknowledge Jan Bacca for helping proofread the paper.

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