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Paramagnetic Attraction of Impurity-Helium SolidsImpurity-helium solids are formed when a mixture of impurity and helium gases enters a volume of superfluid helium. Typical choices of impurity gas are hydrogen deuteride, deuterium, nitrogen, neon and argon, or a mixture of these. These solids consist of individual impurity atoms and molecules as well as clusters of impurity atoms and molecules covered with layers of solidified helium. The clusters have an imperfect crystalline structure and diameters ranging up to 90 angstroms, depending somewhat on the choice of impurity. Immediately following formation the clusters aggregate into loosely connected porous solids that are submerged in and completely permeated by the liquid helium. Im-He solids are extremely effective at stabilizing high concentrations of free radicals, which can be introduced by applying a high power RF dis- charge to the impurity gas mixture just before it strikes the super fluid helium. Average concentrations of 10(exp 19) nitrogen atoms/cc and 5 x 10(exp 18) deuterium atoms/cc can be achieved this way. It shows a typical sample formed from a mixture of atomic and molecular hydrogen and deuterium. It shows typical sample formed from atomic and molecular nitrogen. Much of the stability of Im-He solids is attributed to their very large surface area to volume ratio and their permeation by super fluid helium. Heat resulting from a chance meeting and recombination of free radicals is quickly dissipated by the super fluid helium instead of thermally promoting the diffusion of other nearby free radicals.
Document ID
20050186711
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Bernard, E. P.
(Cornell Univ. Ithaca, NY, United States)
Boltnev, R. E.
(Branch of Inst. of Energy Problems of Chemical Physics Moscow, Russia)
Khmelenko, V. V.
(Cornell Univ. Ithaca, NY, United States)
Lee, D. M.
(Cornell Univ. Ithaca, NY, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Proceedings of the 2003 NASA/JPL Workshop on Fundamental Physics in Space
Subject Category
Nonmetallic Materials
Funding Number(s)
CONTRACT_GRANT: NAG3-2871
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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