Abstract
Ensembles of nitrogen-vacancy (NV) center spins in diamond offer a robust, precise, and accurate magnetic sensor. As their applications move beyond the laboratory, practical considerations including size, complexity, and power consumption become important. Here, we compare two commonly employed NV magnetometry techniques—continuous-wave (CW) versus pulsed magnetic resonance—in a scenario limited by the total available optical power. We develop a consistent theoretical model for the magnetic sensitivity of each protocol that incorporates NV photophysics—in particular, including the incomplete spin polarization associated with limited optical power; after comparing the models’ behavior to experiments, we use them to predict the relative DC sensitivity of CW versus pulsed operation for an optical-power-limited, shot-noise-limited NV ensemble magnetometer. We find a ∼2−3× gain in sensitivity for pulsed operation, which is significantly smaller than seen in power-unlimited, single-NV experiments [Phys. Rev. B 84, 195204 (2011)PRBMDO0163-182910.1103/PhysRevB.84.195204]. Our results provide a resource for practical sensor development, informing protocol choice and identifying optimal operation regimes when optical power is constrained.
Funder
Canada Foundation for Innovation
Canada Research Chairs
Natural Sciences and Engineering Research Council of Canada
National Research Council of Canada
Subject
Atomic and Molecular Physics, and Optics,Statistical and Nonlinear Physics