Coherent Rabi dynamics of a superradiant spin ensemble in a microwave cavity

dc.bibliographicCitation.firstPage031002
dc.bibliographicCitation.issue3
dc.bibliographicCitation.journalTitlePhysical Review Xeng
dc.bibliographicCitation.volume7
dc.contributor.authorRose, B.C.
dc.contributor.authorTyryshkin, A.M.
dc.contributor.authorRiemann, H.
dc.contributor.authorAbrosimov, N.V.
dc.contributor.authorBecker, P.
dc.contributor.authorPohl, H.-J.
dc.contributor.authorThewalt, M.L.W.
dc.contributor.authorItoh, K.M.
dc.contributor.authorLyon, S.A.
dc.date.accessioned2023-01-27T09:31:11Z
dc.date.available2023-01-27T09:31:11Z
dc.date.issued2017
dc.description.abstractWe achieve the strong-coupling regime between an ensemble of phosphorus donor spins in a highly enriched 28Si crystal and a 3D dielectric resonator. Spins are polarized beyond Boltzmann equilibrium using spin-selective optical excitation of the no-phonon bound exciton transition resulting in N=3.6×1013 unpaired spins in the ensemble. We observe a normal mode splitting of the spin-ensemble–cavity polariton resonances of 2g√N=580  kHz (where each spin is coupled with strength g) in a cavity with a quality factor of 75 000 (γ≪κ≈60  kHz, where γ and κ are the spin dephasing and cavity loss rates, respectively). The spin ensemble has a long dephasing time (T∗2=9  μs) providing a wide window for viewing the dynamics of the coupled spin-ensemble–cavity system. The free-induction decay shows up to a dozen collapses and revivals revealing a coherent exchange of excitations between the superradiant state of the spin ensemble and the cavity at the rate g√N. The ensemble is found to evolve as a single large pseudospin according to the Tavis-Cummings model due to minimal inhomogeneous broadening and uniform spin-cavity coupling. We demonstrate independent control of the total spin and the initial Z projection of the psuedospin using optical excitation and microwave manipulation, respectively. We vary the microwave excitation power to rotate the pseudospin on the Bloch sphere and observe a long delay in the onset of the superradiant emission as the pseudospin approaches full inversion. This delay is accompanied by an abrupt π-phase shift in the peusdospin microwave emission. The scaling of this delay with the initial angle and the sudden phase shift are explained by the Tavis-Cummings model.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/11135
dc.identifier.urihttp://dx.doi.org/10.34657/10161
dc.language.isoeng
dc.publisherCollege Park, Md. : APS
dc.relation.doihttps://doi.org/10.1103/physrevx.7.031002
dc.relation.essn2160-3308
dc.rights.licenseCC BY 4.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/4.0
dc.subject.ddc530
dc.subject.otherMesoscopicseng
dc.subject.otherQuantum physicseng
dc.subject.otherStrongly correlated materialseng
dc.titleCoherent Rabi dynamics of a superradiant spin ensemble in a microwave cavityeng
dc.typeArticleeng
dc.typeTexteng
tib.accessRightsopenAccess
wgl.contributorIKZ
wgl.subjectPhysikger
wgl.typeZeitschriftenartikelger
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