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Creation of nitrogen-vacancy centers in chemical vapor deposition diamond for sensing applications

journal contribution
posted on 2024-11-02, 20:06 authored by Tingpeng Luo, Lukas Lindner, Brett Johnson, Marco Capelli
The nitrogen-vacancy (NV) center in diamond is a promising quantum system for magnetometry applications exhibiting optical readout of minute energy shifts in its spin sub-levels. Key material requirements for NV ensembles are a high NV- concentration, a long spin coherence time and a stable charge state. However, these are interdependent and can be difficult to optimize during diamond growth and subsequent NV creation. In this work, we systematically investigate the NV center formation and properties in bulk chemical vapor deposition (CVD) diamond. The nitrogen flow during growth is varied by over four orders of magnitude, resulting in a broad range of single substitutional nitrogen concentrations of 0.2-20 parts per million. For a fixed nitrogen concentration, we optimize electron-irradiation fluences with two different accelerated electron energies, and we study defect formation via optical characterizations. We discuss a general approach to determine the optimal irradiation conditions, for which an enhanced NV concentration and an optimum of NV charge states can both be satisfied. We achieve spin-spin coherence times T 2 ranging from 45.5 to 549 μs for CVD diamonds containing 168 to 1 parts per billion NV- centers, respectively. This study shows a pathway to engineer properties of NV-doped CVD diamonds for improved sensitivity.

Funding

ARC Centre of Excellence for Quantum Computation and Communication Technology

Australian Research Council

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History

Related Materials

  1. 1.
    DOI - Is published in 10.1088/1367-2630/ac58b6
  2. 2.
    ISSN - Is published in 13672630

Journal

New Journal of Physics

Volume

24

Number

33030

Issue

3

Start page

1

End page

16

Total pages

16

Publisher

Institute of Physics

Place published

United Kingdom

Language

English

Copyright

© 2022 The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence.,Institute of Physics and Deutsche Physikalische Gesellschaft.

Former Identifier

2006115065

Esploro creation date

2022-05-28

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