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dc.date.accessioned2022-03-12T17:57:04Z
dc.date.available2022-03-12T17:57:04Z
dc.date.created2021-08-18T21:37:24Z
dc.date.issued2021
dc.identifier.citationZimmer, Christian Yzombard, Pauline Camper, Antoine Comparat, Daniel . Positronium laser cooling in a magnetic field. Physical Review A (PRA). 2021
dc.identifier.urihttp://hdl.handle.net/10852/92373
dc.description.abstractWe study realistic 3D laser cooling of positronium (Ps) in the presence of a magnetic field. Triplet and singlet states mixing due to the magnetic field, and dynamical Stark effect, generally produce higher annihilation rates than in the zero-field case. 3D cooling is efficient only at very low field B≲50mT and at high field values B⪆0.7T. Near 100ns long laser pulses, spectrally broad enough to cover most of the Ps Doppler profile and with energy in the mJ range, are required to cool Ps. Simulations based on full diagonalization of the Stark and Zeeman Hamiltonian and a kinetic Monte Carlo algorithm exactly solving the rate equations indicate that an efficient cooling (typically from 300K down to below 50K) is possible even in a magnetic field. We also propose 3D moving molasses cooling that can produce a well-defined monochromatic Ps beam useful for applications.
dc.languageEN
dc.publisherAmerican Physical Society
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titlePositronium laser cooling in a magnetic field
dc.typeJournal article
dc.creator.authorZimmer, Christian
dc.creator.authorYzombard, Pauline
dc.creator.authorCamper, Antoine
dc.creator.authorComparat, Daniel
cristin.unitcode185,15,4,0
cristin.unitnameFysisk institutt
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1927101
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review A (PRA)&rft.volume=&rft.spage=&rft.date=2021
dc.identifier.jtitlePhysical Review A (PRA)
dc.identifier.volume104
dc.identifier.issue2
dc.identifier.doihttps://doi.org/10.1103/PhysRevA.104.023106
dc.identifier.urnURN:NBN:no-94961
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2469-9926
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/92373/1/PhysRevA.104.023106.pdf
dc.type.versionPublishedVersion
cristin.articleid023106
dc.relation.projectNFR/303337


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