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

Author(s): Rose, BC; Tyryshkin, AM; Riemann, H; Abrosimov, NV; Becker, P; et al

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dc.contributor.authorRose, BC-
dc.contributor.authorTyryshkin, AM-
dc.contributor.authorRiemann, H-
dc.contributor.authorAbrosimov, NV-
dc.contributor.authorBecker, P-
dc.contributor.authorPohl, H-J-
dc.contributor.authorThewalt, MLW-
dc.contributor.authorItoh, KM-
dc.contributor.authorLyon, Stephen A-
dc.date.accessioned2021-10-08T20:15:48Z-
dc.date.available2021-10-08T20:15:48Z-
dc.date.issued2017-7-10en_US
dc.identifier.citationRose, BC, Tyryshkin, AM, Riemann, H, Abrosimov, NV, Becker, P, Pohl, H-J, Thewalt, MLW, Itoh, KM, Lyon, SA. (2017). Coherent Rabi dynamics of a superradiant spin ensemble in a microwave cavity. Physical Review X, 7 (10.1103/PhysRevX.7.031002en_US
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1g276-
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 p-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.en_US
dc.language.isoen_USen_US
dc.relation.ispartofPhysical Review Xen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleCoherent Rabi dynamics of a superradiant spin ensemble in a microwave cavityen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.1103/PhysRevX.7.031002-
dc.date.eissued2017-7-10en_US
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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