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Dispersive readout of reconfigurable ambipolar quantum dots in a silicon-on-insulator nanowire

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arxiv 2009.13944 v1 pith:AQQZJITG submitted 2020-09-29 cond-mat.mes-hall

classification cond-mat.mes-hall
keywords dotsquantumsiliconambipolarholesabilitychanneldouble
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We report on ambipolar gate-defined quantum dots in silicon on insulator (SOI) nanowires fabricated using a customised complementary metal-oxide-semiconductor (CMOS) process. The ambipolarity was achieved by extending a gate over an intrinsic silicon channel to both highly doped n-type and p-type terminals. We utilise the ability to supply ambipolar carrier reservoirs to the silicon channel to demonstrate an ability to reconfigurably define, with the same electrodes, double quantum dots with either holes or electrons. We use gate-based reflectometry to sense the inter-dot charge transition(IDT) of both electron and hole double quantum dots, achieving a minimum integration time of 160(100) $\mu$s for electrons (holes). Our results present the opportunity to combine, in a single device, the long coherence times of electron spins with the electrically controllable holes spins in silicon.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 54 citations worldwide. Full citation record

  1. A study of the large-scale formation in the environment of A3266: Infalling groups, filaments, and a premerger cold front

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    A 3.6σ X-ray filament of length ~1.1 Mpc connects A3266 to a cool-core NW group that hosts a premerger cold front, with filament gas hotter and denser than pristine WHIM.

  2. The Peculiar Mini-Halo in the Shapley Supercluster Member Abell 3558

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    The diffuse radio emission in A3558 is a peculiar mini-halo with a new northern extension, a steep spectrum of 1.18, and a sublinear radio-X-ray correlation that steepens with frequency, consistent with sloshing-induc...

  3. A new shock in the pre-merging cluster pair 1E2215-2216

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    A faint shock front with Mach number about 1.2 was found south of galaxy cluster 1E2215 using new XMM-Newton and archival Chandra X-ray data.

  4. Origin of the Sloshing Spiral in the Abell 2107 Galaxy Cluster

    astro-ph.CO 2026-07 conditional novelty 5.0 of 10

    A previously unknown sloshing spiral with three cold fronts is discovered in the ICM of the apparently relaxed cluster Abell 2107, pointing to a past off-axis merger with a possibly dark perturber.

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