Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/114917
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dc.contributor.authorDakka, M.A.-
dc.contributor.authorTsiminis, G.-
dc.contributor.authorGlover, R.D.-
dc.contributor.authorPerrella, C.-
dc.contributor.authorMoffatt, J.-
dc.contributor.authorSpooner, N.A.-
dc.contributor.authorSang, R.T.-
dc.contributor.authorLight, P.S.-
dc.contributor.authorLuiten, A.N.-
dc.date.issued2018-
dc.identifier.citationPhysical Review Letters, 2018; 121(9)-
dc.identifier.issn0031-9007-
dc.identifier.issn1079-7114-
dc.identifier.urihttp://hdl.handle.net/2440/114917-
dc.description.abstractWe demonstrate the generation of metastable krypton in the long-lived 1s^{5} state using laser excitation. The atoms are excited through a two-photon absorption process into the 2p^{6} state using a pulsed optical parametric oscillator laser operating near 215 nm, after which the atoms decay quickly into the metastable state with a branching ratio of 75%. The interaction dynamics are modeled using density matrix formalism and, by combining this with experimental observations, we are able to calculate photoionization and two-photon absorption cross sections. When compared to traditional approaches to metastable production, this approach shows great potential for high-density metastable krypton production with minimal heating of the sample. Here, we show metastable production efficiencies of up to 2% per pulse. The new experimental results gained here, when combined with the density matrix model we have developed, suggest that fractional efficiencies up to 30% are possible under optimal conditions.-
dc.description.statementofresponsibilityM. A. Dakka, G. Tsiminis, R. D. Glover, C. Perrella, J. Moffatt, N. A. Spooner, R. T. Sang, P. S. Light, and A. N. Luiten-
dc.language.isoen-
dc.publisherAmerican Physical Society-
dc.rights© 2018 American Physical Society-
dc.source.urihttp://dx.doi.org/10.1103/physrevlett.121.093201-
dc.titleLaser-based metastable krypton generation-
dc.typeJournal article-
dc.identifier.doi10.1103/PhysRevLett.121.093201-
dc.relation.granthttp://purl.org/au-research/grants/arc/LE160100027-
dc.relation.granthttp://purl.org/au-research/grants/arc/DE120102028-
pubs.publication-statusPublished-
dc.identifier.orcidTsiminis, G. [0000-0002-4321-3837]-
dc.identifier.orcidGlover, R.D. [0000-0002-7828-1426]-
dc.identifier.orcidPerrella, C. [0000-0002-6140-9323]-
dc.identifier.orcidSpooner, N.A. [0000-0002-8534-3816]-
dc.identifier.orcidLight, P.S. [0000-0003-3873-7991]-
dc.identifier.orcidLuiten, A.N. [0000-0001-5284-7244]-
Appears in Collections:Aurora harvest 3
Physics publications

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