Determining the Asymptotic D- to S-State Ratio for Light Nuclei

dc.contributor.authorStephenson, E.J.
dc.contributor.authorCupps, V.
dc.contributor.authorFoster, C.C.
dc.contributor.authorHall, J.R.
dc.contributor.authorJacobs, W.W.
dc.contributor.authorJones, W.P.
dc.contributor.authorKaitchuck, M.D.
dc.contributor.authorLondergan, J.T.
dc.contributor.authorPickar, M.
dc.contributor.authorSchwandt, P.
dc.date.accessioned2007-11-07T18:17:29Z
dc.date.available2007-11-07T18:17:29Z
dc.date.issued1981
dc.descriptionThis work was supported by the National Science Foundation Grants NSF PHY 78-22774 A03, NSF PHY 81-14339, and by Indiana University
dc.format.extent471711 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationAnnual Scientific and Technical Report, 1981, p. 59-62.
dc.identifier.urihttps://hdl.handle.net/2022/2763
dc.language.isoen_US
dc.publisherIndiana University Cyclotron Facility
dc.rightsThis work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivs 2.5 License
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/2.5
dc.subjectasymptote
dc.subjectratio
dc.subjectlight
dc.subjectnuclei
dc.titleDetermining the Asymptotic D- to S-State Ratio for Light Nuclei
dc.typeArticle

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