• Open Access

Efficient high-fidelity flying qubit shaping

Benedikt Tissot and Guido Burkard
Phys. Rev. Research 6, 013150 – Published 8 February 2024

Abstract

Matter qubit to traveling photonic qubit conversion is the cornerstone of numerous quantum technologies such as distributed quantum computing, as well as several quantum internet and networking protocols. We formulate a theory for stimulated Raman emission which is applicable to a wide range of physical systems, including quantum dots, solid-state defects, and trapped ions, as well as various parameter regimes. We find the upper bound for the photonic pulse emission efficiency of arbitrary matter qubit states for imperfect emitters and show a path forward to optimizing the fidelity. Based on these results, we propose a paradigm shift from optimizing the drive to directly optimizing the temporal mode of the flying qubit using a closed-form expression. Protocols for the production of time-bin encoding and spin-photon entanglement are proposed. Furthermore, the mathematical idea to use input-output theory for pulses to absorb the dominant emission process into the coherent dynamics, followed by a non-Hermitian Schrödinger equation approach, has great potential for studying other physical systems.

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  • Received 21 December 2022
  • Revised 18 May 2023
  • Accepted 11 January 2024

DOI:https://doi.org/10.1103/PhysRevResearch.6.013150

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Quantum Information, Science & TechnologyAtomic, Molecular & Optical

Authors & Affiliations

Benedikt Tissot* and Guido Burkard

  • Department of Physics, University of Konstanz, D-78457 Konstanz, Germany

  • *benedikt.tissot@uni-konstanz.de
  • guido.burkard@uni-konstanz.de

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Issue

Vol. 6, Iss. 1 — February - April 2024

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