Abstract
We consider an electronic spin, such as a nitrogenvacancy center in diamond, weakly coupled to a large number of nuclear spins and subjected to the Rabi driving with a periodically alternating phase. We show that by switching the driving phase synchronously with the precession of a given nuclear spin, the interaction to this spin is selectively enhanced, while the rest of the bath remains decoupled. The enhancement is of resonant character. The key feature of the suggested scheme is that the width of the resonance is adjustable and can be greatly decreased by increasing the driving strength. Thus, the resonance can be significantly narrowed, by a factor of 10–100 in comparison with the existing detection methods. Significant improvement in selectivity is explained analytically and confirmed by direct numerical manyspin simulations. The method can be applied to a wide range of solidstate systems.
Introduction
Detecting a single nuclear spin is an ultimate goal in nuclear magnetic resonance, actively pursued using various techniques^{1,2,3,4,5,6,7,8}. Moreover, onebyone detection, characterization and manipulation of individual nuclear spins in solids is vital for harnessing them as a resource for quantum information processing^{9,10,11,12,13,14,15,16,17,18,19,20}. The crucial problem, hindering the progress in this area, is to separate the weak signal, produced by a given weakly coupled nuclear spin, from the much stronger background created by all other spins and by the ambient magnetic noise. I.e., the detector must possess high selectivity to separate the signal of the target spin from the action of other spins and from magnetic noise.
It has been recently shown that an electron spin of the nitrogenvacancy (NV) centers in diamond is an excellent nuclear spin detector^{5,6,7,8,21,22,23,24,25,26,27}. By applying the dynamical decoupling protocols to the NV spin (pulse^{5,6,7} or continuous^{8,27}), the individual nuclear spins around the NV center can be detected one by one in a resonant manner: the NV spin becomes decoupled from all nuclear spins, except the one which satisfies a stringent resonance condition. The resonating nuclear spin strongly affects the NV spin motion and hence can be detected and the width of the resonances produced by different nuclear spins determines selectivity. However, in all current schemes this width is naturally limited, being determined by the strength of the hyperfine coupling between the target nuclear spin and the NV spin.
Overcoming this limitation and drastically narrowing the resonances in a systematic way, in order to significantly improve the detection selectivity, is of much importance. Here we present a scheme which achieves that goal. It employs the periodically changing Rabi driving on the NV center’s spin (multiple rotary echo)^{28,29,30} with a specially chosen period to detect the nuclear spins. The width of a resonance, corresponding to detection of a given nuclear spin is inversely proportional to the Rabi driving strength and therefore can be directly adjusted in experiment. As a result, the resonance peak width is narrowed by a factor of 10 − 100 in comparison with the existing schemes. This narrowing greatly enhances the resolution, which is very important for accurate characterization of the nuclearspin environment of the NV center^{6,7,8,12,13} and for NVbased nuclear magnetic resonance at nanoscale^{21,25,26}. Thus, our approach combines excellent protection from magnetic noise offered by the rotary echo and greatly enhanced selectivity in detection of individual nuclear spins. This approach can also be used with other electronic spins as detectors, e.g. spins of dopant atoms in semiconductors or other defect centers in various materials.
Results
We consider the electronic spin S = 1 of the NV center subjected to a moderate (tens to hundreds of Gauss) static bias field along the symmetry axis. The NV spin possesses three wellseparated states m_{NV} = 0, 1 and −1 (denoted below as ) and is manipulated by applying the microwave driving at resonance with the transition between the states and , as shown in Fig. 1; the level remains idle and will be further ignored. The NV spin is coupled to a nuclear spin I: e.g., a ^{13}C nuclear spins in diamond (I = 1/2), coupled to the NV center via dipolar interaction. To simplify consideration, we temporarily omit the coupling of the NV spin to other ^{13}C spins in the sample, considering the case of many nuclear spins later (see also Supplementary Information). In the coordinate frame rotating with the frequency of the resonant microwave driving, the system is described by the Hamiltonian
where and describe the NV spin and I_{x,z} are the operators of the target nuclear spin, h is the Rabi driving field (usually, few to few tens of MHz), ω_{L} is the Larmor frequency of the nuclear spin, and are the components of the hyperfine coupling and we assume ħ = 1 throughout the text.
During the rotary echo experiment the direction of the Rabi driving field (i.e. the phase of driving) periodically changes between +x (along the xaxis) and −x (opposite to the xaxis), as shown in Fig. 1. Here we consider symmetrized protocol, consisting of N rotary echo cycles; within each cycle the driving field is along +x during the two outer segments, each of duration T and is along −x during the inner segment of duration 2T. Therefore, the Hamiltonian (1) describes the two outer segments of the rotary echo cycle and the Hamiltonian for the inner segment is obtained by replacing h → −h. Below, we denote these two Hamiltonians as H_{+} and H_{−}, respectively, so the evolution operator for a single cycle is
and the full Ncycle protocol is described by the evolution operator U(N) = U^{N}. Generally, periodic switching of the Rabi field in the regime of strong driving leads to highly efficient decoupling of the NV electronic spin from the surrounding spins^{29,30,31}. However, in a special resonant regime, where the Rabi field is switched synchronously with the Larmor precession of the target nuclear spin, quantum states of the NV center spin and the target nuclear spin become entangled. After many rotaryecho cycles, , this entanglement becomes detectable despite the weak coupling between the NV and target spins. This approach is close in spirit to the “stroboscopic matching” idea^{32}.
To qualitatively understand this phenomenon, we analyze the evolution of the system assuming small coupling , so that the zeroorder Hamiltonians are . The corresponding zeroorder evolution operator is given by
where . I.e., the nucleus and the NV center are practically decoupled: over one cycle, the nuclear spin rotates around the zaxis by the angle 2φ and this rotation does not depend on the state of the NV spin. However, if the driving is switched in resonance with the nuclear spin precession, so that the switching time has a special value,
then sin2φ = 0 and the operator U_{0} is unity, i.e. the effect of the zeroorder Hamiltonian is null after one cycle. Then the smaller higherorder corrections will become important, since their effect will accumulate over many rotary echo cycles, undisturbed by the zeroorder terms. The detailed analysis (details are given in Supplementary Information) shows that in this resonance case the nuclear spin evolution changes drastically: the rotation axis tilts towards y axis, the rotation angle per cycle is of order of and most importantly, the nuclear spin entangles with the NV spin through the operator . I.e., at resonance the nuclear spin rotates in different directions depending on whether the NV spin is in the state or , where are the eigenstates of S_{y} with the eigenvalues S_{y} = ±1/2, respectively.
We consider an experiment where the NV spin is prepared in the state m_{NV} = 1 and the operator S_{z}(N) is measured after N rotary echo cycles. At resonance, the initial coherent superposition is decohered in the basis as a result of entanglement with the unpolarized nuclear spin, so that the resonance can be detected by sudden onset of strong decay of S_{z}(N) Analytical solution, which remains valid at long times , is derived as explained in the Methods section, also see Supplementary Information for details. The result is:
and in the vicinity of the resonance and , where ϕ = hT. The signal envelope as a function of the switching time T (or the angle φ) has Lorentzian shape with the width (for ) and the depth . To maximize the depth, the driving should be adjusted to have ϕ = hT = πm with integer m. This also minimizes interference between different nuclear spins and the influence of the fluctuations in the driving power, see Supplementary Information and below we always assume this condition satisfied. Typical dependence of the signal on T is shown in Fig. 2, where the resonances at T_{k=1} and T_{k=2} are clearly seen. The analytical solution (5) is very precise: it practically coincides with the direct numerical simulation of the twospin system described by the Hamiltonian (1).
For a weakly coupled nucleus, located sufficiently far from the NV center, the hyperfine coupling is determined primarily by dipolar interaction, so that , where R is the vector connecting the positions of the NV center and the nucleus and γ_{e} and γ_{n} are the electronic and nuclear gyromagnetic ratios, respectively. Therefore, the nuclei from different locations produce the peaks at different values of T and hence can be resolved.
To test our approach and to illustrate its performance under realistic circumstances, we performed direct simulations of the rotaryecho detection for the NV center coupled to 14 nuclear spins of ^{13}C randomly located in diamond lattice. The simulation results, given in Fig. 3 for k = 3, clearly show the sharp, wellresolved peaks, corresponding to different nuclei, with selectivity in subkHz region, even for very modest driving h ~ 2π · 5 MHz (see also Supplementary Information for more details). Some nuclei, located at the symmetryrelated positions in the lattice, have the same and hence the same resonance value of T; to resolve them, the static bias field should be tilted away from the symmetry axis of the NV center^{6}. The simulations also confirm our conclusion (see Supplementary Information) that the NVmediated interaction between the nuclear spins, caused by the driving, does not noticeably affect the detection efficiency.
For a fixed total interrogation time t_{N} = 4NT, the resonance width determines selectivity of the protocol, i.e. the ability to resolve two nuclei with close hyperfine couplings and (i.e. , ). High selectivity of the suggested scheme is determined by the small width of the resonances achieved at , this width is and decreases as driving h increases (for estimates here and below we neglect the difference between and , taking ). The resonance width ΔT should be compared to the distance between the korder resonances from two nuclear spins, which is . Thus, the resonances are resolved when . For a typical experiment, detecting ^{13}C spins, with the bias field of 400 G (ω_{L} = 2π · 428 kHz) and driving of h = 2π · 10 MHz, for k = 3, the condition of resolved resonances is .
Note that the protocols discussed in this work are, in fact, twodimensional, with the signal depending on some adjustable parameter (T for our scheme, τ for the pulse dynamical decoupling, etc.) and on the total interrogation time. Analyzing the latter dependence was proposed^{8} as a way to increase resolution; this option can also be used within the pulse dynamical decoupling detection and within the protocol presented here. However, the resulting improvement strongly depends on experimental details and is beyond the scope of the present paper.
Discussion
The fact that the resonance width can be adjusted by simply changing the driving h is a key feature of the proposed protocol, which leads to great improvement in selectivity. In the currently existing detection schemes, the width of the resonance is naturally limited, being determined by the coupling constants and . The scheme proposed here is the first, to our knowledge, where the width of the resonances can be tuned at experimentalist’s will; this allows narrowing of the resonances by a factor of 10–100 in comparison with other existing schemes (see Supplementary Information for details), albeit at the expense of the longer interrogation time. Also, stronger driving greatly improves the coherence time of the NV spin^{29,30,31}. Moreover, using the rotary echo protocol with the optimal choice of driving h significantly reduces the impact of slow fluctuations in the driving strength, which is an important limiting factor for the HartmannHahn double resonance detection^{8,32}.
Above we omitted the NV center’s own ^{14}N (or ^{15}N) nuclear spin: we assume that it is 100% polarized in the state with a given m_{I} and that the driving is applied at the frequency of the corresponding transition. Without such polarization, the hyperfine levels which are not in resonance with the Rabi driving field are quickly decohered, since the onsite hyperfine coupling (2.15 MHz for ^{14}N and 3.03 MHz for ^{15}N) is comparable to a typical driving strength, so that overall detection quality degrades (see Supplementary Information). Fortunately, polarization of the NV’s own nuclear spin can be easily achieved in different ways^{12,15,33,34,35} and incorporated in the experimental protocol.
Concluding, we presented a scheme for onebyone detection of the nuclear spins weakly coupled to an electron spin (e.g. the NV center in diamond), using the rotary echo protocol. The key feature of this scheme is the ability to experimentally adjust and thus greatly narrow, the width of the resonance peaks corresponding to the detected nuclear spins. When compared with the existing approaches, the scheme proposed here provides significant improvement in the selectivity of the nuclear spin detection, albeit being more demanding to the quality of experimental setup (see Supplementary Information) in terms of the fast switching of the driving phase and the timing precision (~0.5 ns, determined by the width of the resonant peak) and increased interrogation time (equal to 4NT, about 1 ms per run for parameters used in Fig. 3). Moreover, the scheme discussed here and the considerations above, are not specific to the NV center and can be applied to a wide range of other electronnuclear systems, such as dopant atoms in semiconductors and other color centers, using the electron spins as probes for the surrounding nuclei.
Methods
Analytical Calculations
NV center is subjected to the static magnetic field parallel to its quantization axis and to a strong driving rf field at the frequency of the transition between the two lowest sublevels, m_{NV} = 0 and m_{NV} = 1 ( and , respectively) and coupled to a ^{13}C nuclear spin I = 1/2 via dipoledipole interaction; the sublevel m_{NV} = −1 is idle and thus ignored. Within the secular approximation, in the frame rotating with the frequency of the rf field, the system’s Hamiltonian is
where , h is the Rabi driving field, ω_{L} is the Larmor frequency of the nuclear spin and A_{i} are the components of the hyperfine field created by the NV spin at the nuclear spin position. The coupling constants are , where R is the vector connecting NV center and the nuclear spin, i = x, y, z, γ_{e} and γ_{n} are the electronic and nuclear gyromagnetic ratios and δ_{ij} is the Kronecker’s symbol. For a remote nucleus, the coupling strength is small, so . Introducing the operator , with appropriate rotation of the nuclear spin coordinate axes, the Hamiltonian becomes
where and and the terms are neglected, since they only slightly renormalize ω_{L}, and . We parametrize and , where θ is the angle between the hyperfine field and the NV symmetry axis and is related to the polar angle, θ_{R}, of the vector R through and .
The evolution operator U of a single rotary echo cycle is given by Eq. 2 of the main text. We analyze dynamics by finding lnU to the first order in the small parameter g = ω_{h}/h. We achieve that by relating the Hamiltonian H of Eq. 1 and the noninteracting (zeroorder) Hamiltonian (see Eq. 3). This is done in two steps; first we apply to H_{0} the SchriefferWolfe type transformation via the unitary operator and obtain
where we neglected terms of the order g^{2}ω_{L}, g^{2}ω_{h} and higher. Next transformation, with , eliminates the last term in the equation above and we find that . Correspondingly, for the evolution operator we have , where
with H_{0±} = H_{0}(±h); here W_{1} disappears as it commutes with W_{0} and is even with respect to the sign change of h. Expanding W_{0} in terms of small g, we find U and rewrite it as a single exponential,
where ϕ = hT and the coefficients r_{x} = −sinθ cosφ sinϕ, r_{y} = sinθ sinφ cosϕ and r_{z} = −cosθ sinϕ; the total sign ± should be chosen to be the same as the sign of cos2φ, whereas the parameter is given by tanγ = tan2φ. The rotary echo signal after N cycles is found by evaluating the trace, ; by writing U as a single exponential, U^{N} is evaluated in a straightforward but lengthy manner (see Supplementary Information for details), giving the results mentioned in the main text.
Numerical Simulations
The numerical simulations were performed for one electron spin of the NV center and 14 nuclear spins ^{13}C located at the sites of the diamond lattice. To make the system reasonably realistic, the lattice sites for the first six nuclear spins were taken as close as possible to the spins detected in ref. 5. The rest of the spins were placed randomly on the diamond lattice, with the restriction that the resulting density of the ^{13}C spins corresponds to their natural abundance of 1.08%. The simulations were performed in the rotating frame, using the Hamiltonian with 14 nuclear spins:
The electron spin of the NV center was assumed to be localized at the midpoint between the positions of the nitrogen atom and the vacancy. The hyperfine interaction between the jth nuclear spin and the electron spin were assumed to be of purely dipoledipole nature and the interaction constants and were calculated using the simulated locations of the nuclear spins. Additional numerical results and comparison with the pulsebased detection method are given in Supplementary Information.
Additional Information
How to cite this article: Mkhitaryan, V. V. et al. Highly selective detection of individual nuclear spins with rotary echo on an electron spin probe. Sci. Rep. 5, 15402; doi: 10.1038/srep15402 (2015).
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Acknowledgements
We thank R. Hanson, T. H. Taminiau, M. Raikh and H. Terletska for helpful and important discussions. This work was supported by the Department of Energy—Basic Energy Sciences under Contract No. DEAC0207CH11358.
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V.V.D. and F.J. conceived the method, V.V.M. and V.V.D. performed analytical and numerical studies. All authors analyzed and discussed the results and participated in writing the manuscript.
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Mkhitaryan, V., Jelezko, F. & Dobrovitski, V. Highly selective detection of individual nuclear spins with rotary echo on an electron spin probe. Sci Rep 5, 15402 (2015). https://doi.org/10.1038/srep15402
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DOI: https://doi.org/10.1038/srep15402
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