Non-Markovian Spin-Bath Dynamics of a Single Nitrogen-Vacancy Center in Diamond
ORAL
Abstract
For many experiments in quantum information science, it is essential to protect quantum coherence from environmental decoherence sources. While stochastic (Markovian) processes of the decoherence have been studied extensively, non-Markovian processes are often overlooked since they are not captured by simple models. In principle, non-Markovian environmental bath dynamics can present a perspective for understanding and combating quantum decoherence.
We plan to investigate non-Markovian spin-bath dynamics of single nitrogen-vacancy (NV) centers in type-Ib and type-IIa diamond [1]. We show that a simple phenomenological model known as the post-Markovian master equation (PMME) can be used to capture a non-Markovian component of the spin-bath dynamics. We utilize PMME and quantum state tomography measurements to probe non-Markovian spin dynamics of the single NV center. Moreover, the trace-norm distance between two different initial states will be used to quantify the degree of non-Markovianity observed in the NV spin dynamics.
We plan to investigate non-Markovian spin-bath dynamics of single nitrogen-vacancy (NV) centers in type-Ib and type-IIa diamond [1]. We show that a simple phenomenological model known as the post-Markovian master equation (PMME) can be used to capture a non-Markovian component of the spin-bath dynamics. We utilize PMME and quantum state tomography measurements to probe non-Markovian spin dynamics of the single NV center. Moreover, the trace-norm distance between two different initial states will be used to quantify the degree of non-Markovianity observed in the NV spin dynamics.
*This work was supported by the National Science Foundation (CHE-2004252 with partial co-funding from the Quantum Information Science program in the Division of Physics, ECCS-2204667).
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Publication: 1. C. Selco, D. Lidar and S. Takahashi, manuscript in preparation (2022).
Presenters
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Cooper M Selco
- University of Southern California
- Department of Physics & Astronomy, University of Southern California