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dc.contributorUniv Mayor, Fac Estudios Interdisciplinarios, Ctr Invest DAiTA Lab, Chilees
dc.contributor.authorDuarte, H.
dc.contributor.authorDinani, H. T. [Univ Mayor, Fac Estudios Interdisciplinarios, Ctr Invest DAiTA Lab, Chile]
dc.contributor.authorJacques, V.
dc.contributor.authorMaze, J. R.
dc.date.accessioned2023-12-27T21:36:04Z
dc.date.available2023-12-27T21:36:04Z
dc.date.issued2021-03-27
dc.identifier.citationDuarte, H., Dinani, H. T., Jacques, V., & Maze, J. R. (2021). Effect of intersystem crossing rates and optical illumination on the polarization of nuclear spins close to nitrogen-vacancy centers. Physical Review B, 103(19), 195443.es
dc.identifier.issn2469-9950
dc.identifier.issneISSN 2469-9969
dc.identifier.otherWOS: 000655903200006
dc.identifier.urihttps://repositorio.umayor.cl/xmlui/handle/sibum/9175
dc.identifier.urihttps://arxiv.org/pdf/2011.12039.pdf
dc.identifier.urihttps://journals-aps-org.bibliotecadigital.umayor.cl:2443/prb/abstract/10.1103/PhysRevB.103.195443
dc.identifier.urihttps://doi.org/10.1103/PhysRevB.103.195443
dc.identifier.urihttps://journals.aps.org/prb/abstract/10.1103/PhysRevB.103.195443
dc.description.abstractSeveral efforts have been made to polarize the nearby nuclear environment of nitrogen-vacancy (NV) centers for quantum metrology and quantum information applications. Different methods showed different nuclear spin polarization efficiencies and rely on electronic spin polarization associated to the NV center, which in turn crucially depends on the intersystem crossing. Recently, the rates involved in the intersystem crossing have been measured leading to different transition rate models. Here, we consider the effect of these rates on several nuclear polarization methods based on the level anticrossing, and precession of the nuclear population while the electronic spin is in the m(s) = 0 and m(s) = 1 spin states. We show that the nuclear polarization depends on the power of optical excitation used to polarize the electronic spin. The degree of nuclear spin polarization is different for each transition rate model. Therefore, the results presented here are relevant for validating these models and for polarizing nuclear spins. Furthermore, we analyze the performance of each method by considering the nuclear position relative to the symmetry axis of the NV center.es
dc.description.sponsorshipThe authors thank A. Dreau for helpful discussions. H.D. acknowledges support from Conicyt doctorado Grant No. 21100070. H.T.D. acknowledges support from the Fondecytpostdoctorado Grant No. 3170922 and Universidad Mayor through a postdoctoral fellowship. J.R.M. acknowledges support from Fondecyt Regular Grant No. 1180673, Air Force Grant No. FA9550-18-1-0513, ONR Grant No. N6290918-1-2180, and Anid PIA ACT192023. H.T.D., V.J. and J.R.M. acknowledge support from Conicyt-ECOS Grant No. C16E04.es
dc.format.extent10 p., PDFes
dc.language.isoen_USes
dc.publisherAMER PHYSICAL SOCes
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chilees
dc.titleEffect of intersystem crossing rates and optical illumination on the polarization of nuclear spins close to nitrogen-vacancy centerses
dc.typeArtículo o Paperes
umayor.indizadorCOTes
umayor.indexadoWeb of Sciencees
umayor.indexadoScopuses
dc.identifier.doi10.1103/PhysRevB.103.195443
umayor.indicadores.wos-(cuartil)Q2
umayor.indicadores.scopus-(scimago-sjr)SCIMAGO/ INDICE H: 481
umayor.indicadores.scopus-(scimago-sjr)SJR 1,47


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