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Production of a 23S Helium Beam

dc.contributor.authorFry, E. S.en_US
dc.contributor.authorWilliams, W. L.en_US
dc.date.accessioned2010-05-06T22:15:32Z
dc.date.available2010-05-06T22:15:32Z
dc.date.issued1969-09en_US
dc.identifier.citationFry, E. S.; Williams, W. L. (1969). "Production of a 23S Helium Beam." Review of Scientific Instruments 40(9): 1141-1143. <http://hdl.handle.net/2027.42/70500>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70500
dc.description.abstractBeams of metastable helium produced by electron bombardment generally contain atoms in both the 21S and 23S states. It is important in many experiments to distinguish between these states, or at least to know the population ratio. A beam of 23S and ground state helium atoms has been produced by electron bombardment and subsequent resonant quenching of 21S atoms with 21S−21P 2 μ radiation. This radiation mixes the 21S and 21P states, the latter decaying primarily to the 11S state by emission of 584 Å radiation. The quenching has been studied as a function of beam atom velocity. The results indicate that beams of metastable helium containing less than 1% 21S atoms can be produced.en_US
dc.format.extent3102 bytes
dc.format.extent248078 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleProduction of a 23S Helium Beamen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumHarrison M. Randall Laboratory of Physics, The University of Michigan, Ann Arbor, Michigan 48104en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70500/2/RSINAK-40-9-1141-1.pdf
dc.identifier.doi10.1063/1.1684181en_US
dc.identifier.sourceReview of Scientific Instrumentsen_US
dc.identifier.citedreferenceE. E. Muschlitz, Jr., Science 159, 599 (1968).en_US
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dc.identifier.citedreferenceW. L. Williams and E. S. Fry, Phys. Rev. Lett. 20, 1335 (1968); E. S. Fry and W. L. Williams, Bull. Amer. Phys. Soc. 13, 1397 (1968).en_US
dc.identifier.citedreferenceWe are indebted to C. W. Hendee of Bendix Corp. for supplying the Channeltron multipliers used in this work.en_US
dc.identifier.citedreferenceD. P. Donnelly, J. C. Pearl, R. A. Heppner, and J. C. Zorn, Rev. Sci. Instrum. 40, 1242 (1969).en_US
dc.identifier.citedreferenceF. C. Fehsenfeld, K. M. Evenson, and H. P. Broida, NBS Rep. 8701 (1964).en_US
dc.identifier.citedreferenceJ. B. French and J. W. Locke, in Rarefied Gas Dynamics, C. L. Brundin, Ed. (Academic Press Inc., New York, 1967), p. 1461.en_US
dc.identifier.citedreferenceW. E. Lamb, Jr. and R. C. Retherford, Phys. Rev. 79, 549 (1950).en_US
dc.identifier.citedreferenceB. Schiff and C. L. Pekeris, Phys. Rev. 134, A638 (1964).en_US
dc.owningcollnamePhysics, Department of


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