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Spin properties of very shallow nitrogen vacancy defects in diamond

B. K. Ofori-Okai, S. Pezzagna, K. Chang, M. Loretz, R. Schirhagl, Y. Tao, B. A. Moores, K. Groot-Berning, J. Meijer, and C. L. Degen
Phys. Rev. B 86, 081406(R) – Published 13 August 2012
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Abstract

We investigate spin and optical properties of individual nitrogen vacancy centers located within 1–10 nm from the diamond surface. We observe stable defects with a characteristic optically detected magnetic-resonance spectrum down to the lowest depth. We also find a small but systematic spectral broadening for defects shallower than about 2 nm. This broadening is consistent with the presence of a surface paramagnetic impurity layer [Tisler et al., ACS Nano 3, 1959 (2009)] largely decoupled by motional averaging. The observation of stable and well-behaved defects very close to the surface is critical for single-spin sensors and devices requiring nanometer proximity to the target.

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  • Received 4 January 2012

DOI:https://doi.org/10.1103/PhysRevB.86.081406

©2012 American Physical Society

Authors & Affiliations

B. K. Ofori-Okai1, S. Pezzagna2, K. Chang3, M. Loretz3, R. Schirhagl3, Y. Tao1,3, B. A. Moores3, K. Groot-Berning2, J. Meijer2, and C. L. Degen3,*

  • 1Department of Chemistry, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA
  • 2RUBION, Ruhr-Universitaet Bochum, Universitaetsstrasse 150, 44780 Bochum, Germany
  • 3Department of Physics, ETH Zurich, Schafmattstrasse 16, 8093 Zurich, Switzerland

  • *degenc@ethz.ch

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Issue

Vol. 86, Iss. 8 — 15 August 2012

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