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000218010 0247_ $$2doi$$a10.1103/PhysRevLett.120.204801
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000218010 0247_ $$2ISSN$$a1079-7114
000218010 0247_ $$2ISSN$$a1092-0145
000218010 0247_ $$2datacite_doi$$a10.15120/GSI-2019-00081
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000218010 041__ $$aEnglish
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000218010 1001_ $$0P:(DE-HGF)0$$aScott, G. G.$$b0$$eCorresponding author
000218010 245__ $$aDual Ion Species Plasma Expansion from Isotopically Layered Cryogenic Targets
000218010 260__ $$aCollege Park, Md.$$bAPS$$c2018
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000218010 500__ $$a"Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI."
000218010 520__ $$aA dual ion species plasma expansion scheme from a novel target structure is introduced, in which a nanometer--thick layer of pure deuterium exists as a buffer species at the target--vacuum interface of a hydrogen plasma. Modeling shows that by controlling the deuterium layer thickness, a composite H+ /D+ ion beam can be produced by target normal sheath acceleration (TNSA), with an adjustable ratio of ion densities, as high energy proton acceleration is suppressed by the acceleration of a spectrally peaked deuteron beam. Particle in cell modeling shows that a (4.3 +/- 0.7) MeV per nucleon deuteron beam is accelerated, in a directional cone of half angle 9 degrees. Experimentally, this was investigated using state of the art cryogenic targetry and a spectrally peaked deuteron beam of (3.4 +/- 0.7) MeV per nucleon was measured in a cone of half angle 7 degrees-9 degrees, while maintaining a significant TNSA proton component.
000218010 536__ $$0G:(DE-HGF)POF3-6211$$a6211 - Extreme States of Matter: From Cold Ions to Hot Plasmas (POF3-621)$$cPOF3-621$$fPOF III$$x0
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000218010 7001_ $$0P:(DE-HGF)0$$aCarroll, D. C.$$b1
000218010 7001_ $$0P:(DE-HGF)0$$aAstbury, S.$$b2
000218010 7001_ $$0P:(DE-HGF)0$$aClarke, R. J.$$b3
000218010 7001_ $$0P:(DE-HGF)0$$aHernandez-Gomez, C.$$b4
000218010 7001_ $$0P:(DE-HGF)0$$aKing, M.$$b5
000218010 7001_ $$0P:(DE-HGF)0$$aAlejo, A.$$b6
000218010 7001_ $$0P:(DE-HGF)0$$aArteaga, I. Y.$$b7
000218010 7001_ $$0P:(DE-HGF)0$$aDance, R. J.$$b8
000218010 7001_ $$0P:(DE-HGF)0$$aHigginson, A.$$b9
000218010 7001_ $$0P:(DE-HGF)0$$aHook, S.$$b10
000218010 7001_ $$0P:(DE-HGF)0$$aLiao, G.$$b11
000218010 7001_ $$0P:(DE-HGF)0$$aLiu, H.$$b12
000218010 7001_ $$0P:(DE-HGF)0$$aMirfayzi, S. R.$$b13
000218010 7001_ $$0P:(DE-HGF)0$$aRusby, D. R.$$b14
000218010 7001_ $$0P:(DE-HGF)0$$aSelwood, M. P.$$b15
000218010 7001_ $$0P:(DE-HGF)0$$aSpindloe, C.$$b16
000218010 7001_ $$0P:(DE-HGF)0$$aTolley, M. K.$$b17
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000218010 7001_ $$0P:(DE-HGF)0$$aZemaityte, E.$$b19
000218010 7001_ $$0P:(DE-HGF)0$$aBorghesi, M.$$b20
000218010 7001_ $$0P:(DE-HGF)0$$aKar, S.$$b21
000218010 7001_ $$0P:(DE-HGF)0$$aLi, Y.$$b22
000218010 7001_ $$0P:(DE-HGF)0$$aRoth, M.$$b23
000218010 7001_ $$0P:(DE-HGF)0$$aMcKenna, P.$$b24
000218010 7001_ $$0P:(DE-HGF)0$$aNeely, D.$$b25
000218010 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.120.204801$$gVol. 120, no. 20, p. 204801$$n20$$p204801$$tPhysical review letters$$v120$$x1079-7114$$y2018
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