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Positronium formation in the noble gases

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dc.contributor.authorMcEachran, Robert
dc.contributor.authorStauffer, A D
dc.date.accessioned2015-12-13T22:22:45Z
dc.date.issued2013
dc.date.updated2016-02-24T09:07:02Z
dc.description.abstractWe present results based upon our ab initio relativistic optical potential method for the simulation of positronium formation in the noble gases neon, argon, krypton and xenon. The method used in this simulation is based upon an approach, first suggested
dc.identifier.issn0953-4075
dc.identifier.urihttp://hdl.handle.net/1885/72402
dc.publisherInstitute of Physics Publishing
dc.sourceJournal of Physics B: Atomic, Molecular and Optical Physics
dc.subjectKeywords: Differential cross section; Energy regions; Ionization cross section; Ionization thresholds; Optical potential; Positronium formation; Small scattering angles; Theoretical approach; Binding energy; Experiments; Inert gases; Ionization of gases; Positrons
dc.titlePositronium formation in the noble gases
dc.typeJournal article
local.bibliographicCitation.issue7
local.contributor.affiliationMcEachran, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationStauffer, A D, York University
local.contributor.authoruidMcEachran, Robert, u1817446
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020201 - Atomic and Molecular Physics
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationf5625xPUB3228
local.identifier.citationvolume46
local.identifier.doi10.1088/0953-4075/46/7/075203
local.identifier.scopusID2-s2.0-84875674790
local.identifier.thomsonID000316556800010
local.type.statusPublished Version

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