Correlated-electron systems support a wealth of magnetic excitations, ranging from conventional spin waves to exotic fractional excitations in low-dimensional or geometrically frustrated spin systems1,2. Probing such excitations on nanometre length scales is essential for unravelling the underlying physics and developing new spintronic nanodevices3,4,5,6. Despite recent progress with real-space techniques7,8,9,10,11,12,13, a wide range of interesting magnetic phenomena in correlated-electron materials remains experimentally inaccessible because of the required combination of resolution, magnetic-field sensitivity and environmental compatibility.

The S=1 electronic spin of the nitrogen-vacancy (NV) centre in diamond is an atom-sized magnetic field sensor that can be brought within a few nanometres of a sample and readily interrogated with optically detected magnetic resonance14. NV centre magnetometry15,16 has provided unprecedented room-temperature magnetic imaging with nanometre-scale resolution14,17,18,19 and single-proton-spin sensitivity20, and has been used to study nanoscale biomagnetism21,22. However, NV centres have only recently emerged as probes of collective spin dynamics in correlated-electron systems19,23. In this work, we demonstrate that single-NV magnetic imaging is a powerful tool for nanometre-scale, quantitative, and non-perturbative detection of spin-wave excitations. We present complementary measurement techniques to study spin-wave excitations over a broad range of magnetic fields and frequencies, as well as a method to characterize spin–spin correlations. These methods may be directly applied to open problems of current interest, such as real-space imaging of skyrmion core dynamics24 or imaging spin-wave excitations in atomically assembled magnets10 as a function of temperature.


Spin waves in a ferromagnetic microdisc

As a model system, we consider a ferromagnetic microdisc (Ni81Fe19) fabricated on top of a diamond chip that contains NV centres implanted at 50 nm below the surface (Fig. 1a,b). We use an on-chip coplanar waveguide to generate microwave magnetic fields to control the NV spin state and to drive spin-wave excitations in the disc. We optically address individual NV centres using a scanning confocal microscope (Fig. 1b) and read out the NV spin state through spin-dependent photoluminescence (Supplementary Note 1).

Figure 1: Nanoscale probing of the magnetic fields generated by a ferromagnetic microdisc.
figure 1

(a), As a model system to study magnetic excitations, we consider a ferromagnetic microdisc (Ni81Fe19, diameter 6 μm, thickness 30 nm) fabricated on top of a diamond surface. NV centres implanted at 50 nm below the surface sense the local magnetic fields BM generated by the magnetization M. (b) Scanning confocal microscopy image showing a photoluminescence map of NV centres close to the disc. Scale bar, 3 μm. The external static magnetic field Bext is applied along the axis of target NV centres. (c) Optically detected electron spin resonance (ESR) traces of the ms=0↔+1 transition of NVA (close to the disc) and NVref (at 11 μm from the disc centre), where ms denotes the spin-projection onto the NV-axis, f is the drive frequency, and γ=2.8 MHz/G. From the ESR frequency of NVref we extract the external magnetic field Bext. From the difference between NVA and NVref we extract the disc stray field at the site of NVA. The dashed circle indicates power broadening caused by amplification of the drive field by a spin-wave excitation. (d) Projection onto the NV axis B of the measured disc stray field as a function of external field, showing opposite behaviour at the sites of NVA and NVB. The sign of the field is relative to Bext. Error bars represent±1 standard deviation determined statistically from typically 100 repetitions of the same measurement. (e) Calculated spatial profile of the projection of the disc stray field onto the NV axis in a plane 50 nm below the disc. Bext=700 G. (f) Numerically calculated projection of the disc stray field onto the NV axis as a function of the external field at the sites of NVA and NVB, in qualitative good agreement with the measurements in d.

Characterizing the static magnetization

Characterization of the static magnetization forms the basis for understanding the excitations of a magnetic system. Using individual NV centres close to the disc, we locally characterize the magnetization as a function of an externally applied static magnetic field Bext (see Methods). We measure the electron spin resonance (ESR) frequency of an NV centre close to the disc (NVA in Fig. 1b) and a reference NV centre (NVref) far from the disc (Fig. 1c). By comparing these ESR frequencies and knowing the NV gyromagnetic ratio γ=2.8 MHz G−1, we determine the stray magnetic field of the disc at the location of NVA (see Methods). Figure 1d shows the projection of this disc stray field onto the NV axis, B, as a function of Bext.

The local nature of the disc’s magnetization becomes clear by comparing the measured disc stray field at two locations (NVA and NVB, Fig. 1b). At both NVA and NVB, this field opposes the external field (Fig. 1d), as expected from a numerically calculated spatial field profile based on a micromagnetics simulation of the disc’s magnetization (Fig. 1e, see also Supplementary Note 2 and Supplementary Fig. 1). However, as Bext is decreased, the change in the disc stray field at NVA is remarkably opposite to that at NVB (Fig. 1d). This behaviour is qualitatively in good agreement with numerical simulations of the disc’s magnetization and the associated disc stray field as a function of Bext (Fig. 1f). These calculations indicate that as Bext is decreased, the magnetization becomes less homogeneous, with spins at the disc’s edge reorienting first. The opposite behaviour of the disc stray field at NVA and NVB is a direct result of the differently varying local magnetization (Methods), and would not be observed in a far-field measurement.

Resonant detection of spin-wave excitations

Spin-wave excitations consist of collectively precessing spins in a magnetically ordered system. It was recently proposed25 that detection of the time-varying stray magnetic fields generated by spin-wave excitations in small ferromagnets may be exploited to strongly amplify the sensitivity of single NV-centre magnetometry. Here we employ a resonant detection technique to locally sense the spin-wave stray magnetic field, demonstrating the first single-spin detection of on-chip magnetic-field amplification by a ferromagnet. We apply a microwave (MW) magnetic field to drive spin-wave excitations in the disc, choosing the MW frequency such that it is resonant with the ESR frequency of a target NV centre. The spins in the disc respond and generate a magnetic field at the site of NVi which interferes with the drive field BD. Transformed into a frame, rotating at the ESR frequency f, these fields are represented by and bD respectively, and sum (inset Fig. 2b) to give the total field driving spin rotations (Rabi oscillations) of NVi at a rate . As we tune the NV ESR frequency using Bext, we observe a striking difference between the Rabi frequency of nearby NV centres (NVi=A,B,C, see Fig. 1b) and the Rabi frequency of a far-away, reference NVref (Fig. 2a). This difference becomes even clearer by plotting the ratio , which corrects for any frequency-dependent delivery of MWs through our setup (Fig. 2b).

Figure 2: Resonant detection of driven spin-wave excitations.
figure 2

(a), Measured Rabi frequency as a function of ESR frequency for three NV centres close to the disc (NVA, NVB and NVC, see Fig. 1b) and reference NV centre NVref far from the disc. We tune the NV ESR frequency using the external magnetic field Bext and drive Rabi oscillations by applying a MW magnetic field at the ESR frequency. The ESR frequency range below (above) 2.87 GHz corresponds to the ms=0↔−1 (ms=0↔+1) transition. (b), Ratio of the Rabi frequency of NVi (i=A,B,C) over the Rabi frequency of NVref, as measured in a. Pronounced resonances are visible where the NV centre ESR frequency matches the numerically calculated ferromagnetic resonance (FMR) of the disc, which occurs at the vertical dashed lines (see c). The grey inset depicts the interference between the a.c. magnetic field generated by a spin-wave excitation at the site of NVi (i=A,B,C) and the driving field bD in a frame rotating at the NV centre ESR frequency. (c) Measured ESR frequencies and numerically calculated FMR frequency as a function of external magnetic field Bext.

Numerical calculations of the spin-wave spectrum of the disc (Supplementary Note 2) indicate that the resonances in Fig. 2b occur when the NV centre ESR frequency matches the frequency of the lowest order spin-wave resonance of the disc (Fig. 2c). This mode—the ferromagnetic resonance (FMR)—is efficiently excited because the driving field is spatially uniform (Supplementary Note 2 and Supplementary Fig. 2). The observed resonance is described by

where , and θ( f ) is the angle between and bD determined by the dynamic susceptibility of the ferromagnet and the location of the NV centre. To illustrate the validity of this model, we fit the resonances in Fig. 2b using equation (1), assuming a simple, single-mode damped oscillator response for r( f ) and θ( f ) (Supplementary Note 3). The resulting Fano-lineshape accurately describes the observed interference for NVA and NVC, demonstrating that this technique is sensitive to both the amplitude and phase of the spin-wave magnetic field. Possible deviations from this model, such as the double-peak structure of NVB, may result from frequency dependence of the spatial profile of the spin-wave excitation or fabrication-related imperfections. The amplification of the MW field also explains the power broadening of the ESR spectra at low applied magnetic fields Bext, as observed in Fig. 1c.

Non-resonant detection of spin-wave excitations

Characterizing the magnetic excitation spectrum in a correlated-electron system, as well as addressing other problems of interest such as imaging magnetic vortex8,9 or skyrmion core dynamics24, requires a detection scheme that operates over a broad frequency range. To this end, we developed an off-resonant detection technique that can detect a sample’s spin dynamics even when the NV centre ESR frequency is far detuned from the frequency of these dynamics. The idea is to drive spin-wave excitations in the sample with a microwave magnetic field and detect the resulting change in the stray magnetic field by applying a multipulse sensing sequence to the NV centre (Fig. 3a)26.

Figure 3: Non-resonant, field-dependent detection of driven spin-wave excitations.
figure 3

(a) Measurement sequence. The first π/2 pulse prepares an NV spin superposition, which is input into an echo sequence with two π pulses. Synchronized with this sequence, we apply microwave (MW) driving at frequency f during the central 2τ period of free evolution to excite spin-wave excitations in the disc. We read out the final phase ϕ of the NV spin state by measuring the projection on the x and y axis. (b) Experimentally determined effective magnetic field Beff at NVB and NVA as a function of MW-driving frequency f and external static magnetic field Bext. Beff is normalized by the square of the drive field measured on-chip using NVref. The dashed line is a numerical calculation of the ferromagnetic resonance (FMR) of the disc. For NVA, the a.c. Stark effect is visible as an enhanced signal in an 300-MHz frequency band between the ESR frequency and the dashed-dotted line over the entire magnetic field range. We use the sign of the Stark effect to determine the sign of Beff in these measurements. Scale bar, 1 μm. (c) Numerically calculated spatial profile of the time-averaged change in the disc’s longitudinal magnetization ΔMx relative to the saturation magnetization MS under spatially uniform driving with a 5 G MW field and the associated stray magnetic field ΔB in the NV-plane, for two MW frequencies close to the FMR f1=fFMR−0.1 GHz and f2=fFMR−0.3 GHz. We use an external static field Bext=450 G, corresponding to the highest field used in the measurements in b, at which we expect the disc magnetization to be the most homogeneous and resemblant of the calculated magnetization. (d) Comparison of measured and calculated FMR lineshapes at Bext=450 G for NVB and NVA. The sign, amplitude and width of the lineshapes accurately match the calculations. The 4% difference in frequency presumably results from a difference in the disc’s saturation magnetization and/or fabrication-related imperfections. Error bars represent ±1 standard deviation determined statistically from typically100 repetitions of the same measurement.

To understand the off-resonant detection scheme in Fig. 3a, it is crucial to realize that during the excitation of a spin-wave resonance, the time-averaged longitudinal magnetization of the disc is reduced (because the precessing spins are tilted away from their equilibrium state), causing a change in the time-averaged disc stray field (Supplementary Fig. 3). By applying the MW driving only during the central 2τ period (Fig. 3a), the disc stray field is modulated in sync with the multipulse sensing sequence applied to the NV centre, leading to a phase shift ϕ on the final NV spin state. At the end of the sequence, we read out this phase and relate it to an effective magnetic field Beff=ϕ/(γT) oriented along the NV axis and averaged over the duration T of the MW driving. We note that the excitation of a spin-wave resonance also generates rapidly oscillating magnetic fields with typical frequencies in the GHz range (recall Fig. 2). However, such frequencies are above the detection capabilities of the scheme in Fig. 3a, because it would require applying the NV spin-control pulses at GHz repetition rates26. Although an exceptional situation occurs for frequencies close to the NV ESR frequency, where the NV spin may pick up a phase through the dynamical (that is, a.c.) Stark effect27, the Stark effect quickly diminishes for increasing detuning with the NV ESR frequency and we estimate it to play a minor role in our measurements (Supplementary Note 4 and Supplementary Fig. 4).

On the application of the measurement scheme in Fig. 3a to NVA and NVB, we observe a clear resonance that agrees well with numerical calculations of the FMR frequency of the disc (Fig. 3b, Supplementary Note 2). In Fig. 3b, Beff is normalized by the square of the drive field |bD|2 measured on-chip using NVref to correct for a frequency dependence in the setup transmission (Methods and Supplementary Note 5). The resonance follows a Kittel-like law , where A is a free parameter, characteristic of spin-wave excitations in a thin ferromagnet with in-plane magnetization. We therefore conclude that the observed resonance corresponds to the FMR of the disc. Furthermore, we observe striking differences in the lineshape of the resonances detected with NVA and NVB (Fig. 3b). To gain more insight into the origin of these differences, we now analyse the influence of the NV centre spatial location in these measurements.

Importantly, the reduction in time-averaged longitudinal magnetization associated with the excitation of a spin-wave mode is not homogeneous in space, but occurs within a specific spatial region of the disc in accordance with the spin-wave mode profile7. The location of an NV centre with respect to this profile determines the sign and magnitude of the corresponding change in magnetic field ΔB(f) that is felt by the NV centre (parallel to its axis). Because of the close proximity of the NV centres, ΔB(f) strongly depends on the NV-centre location (Fig. 3c). In addition, the spatial mode profile depends on frequency (Fig. 3c), affecting the lineshape of ΔB(f). At Bext=450 G we find a remarkably good agreement of the sign, width, and shape of the measured FMR signal with calculations (Fig. 3d) given geometrical uncertainties related to the optical resolution (400 nm), disc fabrication, NV implantation depth, and oxidation. However, we note that these calculations and/or our model do not account for the change in FMR lineshape observed at NVA as we decrease Bext. Such strong sensitivity on location highlights the unique possibilities NV centres offer to study spin dynamics quantitatively and with nanometre-scale resolution.

Detection of spin noise

Spin noise contains valuable information about a system’s magnetic excitation spectrum and is present even in the absence of driving28,29. Here we spectrally probe spin noise in the disc by measuring the spin relaxation rates of a proximal NV centre (NVA), which depend on the strength of the magnetic field generated by the spin noise at the NV centre ESR frequencies30,31. As we lower Bext and thereby change the NV ESR frequencies relative to the spin–noise spectrum, we first find the ms=0↔+1 and then the ms=0↔−1 relaxation rate (where ms denotes the projection of the spin state onto the NV axis) to increase by over an order of magnitude (Fig. 4a,b), indicating a marked increase in the noise at the ESR frequencies.

Figure 4: Probing the spin–noise spectrum.
figure 4

(a) Spin relaxation measurements for NVA at three different external static magnetic fields Bext. The NV centre is prepared in each of its three spin eigenstates (ms=0, −1, +1), and the spin-dependent photoluminescence is measured as a function of waiting time t. We extract the ms=0↔+1 and the ms=0↔−1 relaxation rates by fitting with a three-level model. (b) Measured NV spin relaxation rates as a function of Bext. As we lower Bext, the ms=0↔+1 and the ms=0↔−1 relaxation rates consecutively increase by about an order of magnitude. Dots are measured data. Solid lines are fits based on a model of the magnetic noise spectrum at the site of the NV centre, from which we obtain d=35(5) nm. Error bars represent±1 standard deviation determined by the fit-uncertainty in the fitted relaxation rates. (c) Calculated magnetic noise spectrum at d=35 nm above an infinite magnetic plane as a function of external magnetic field Bext. The increasing NV spin-state relaxation rates for decreasing Bext observed in b are due to the increase in noise spectral density at the NV ESR frequencies, which are denoted by the yellow and white dashed line for the ms=0↔+1 and ms=0↔−1 transition, respectively.

Qualitatively, this behaviour can be understood by realizing that at high magnetic field, the NV ESR frequencies are below the FMR frequency (recall Fig. 2c) and therefore in the gap of the spin-wave spectrum. In contrast, at low magnetic field the ESR frequencies are above the FMR frequency where spin waves do exist and generate noise. For a more quantitative understanding, we calculate the magnetic-noise spectrum at a distance d from an infinite, two-dimensional (2D) magnetic plane (Fig. 4c, see Methods). We use a general framework describing the noise spectrum at the site of a sensor spin in terms of the spin–spin susceptibility and a k-space filter function associated with the dipolar coupling to the spins in the magnet (see Methods). This filter function contains a kernel k2e−2kd that peaks at k=1/d, where d is the NV–disc distance and k is a wavenumber characterizing spatial fluctuations of the magnetization. This kernel reflects that a homogeneous magnetization (k=0) does not generate a magnetic field anywhere outside the plane. Likewise, the magnetic field generated by a spatially rapidly varying magnetization characterized by k>>d is exponentially suppressed. Clearly, the noise at the site of the NV centre is dominated by spin–spin correlations on the scale of d. Since the NV centre is far away from the disc’s edges compared with d, we can approximate the disc by an infinite plane. Furthermore, we approximate the dynamic susceptibility as being dominated by exchange interactions because of the small value of d (Supplementary Note 6). This model excellently describes the measured increase in spin noise at the NV ESR frequencies as we lower Bext (Fig. 4b). From fitting, we obtain d=35(5) nm (Supplementary Note 6). However, we note that the model underestimates the disc’s thickness by more than an order of magnitude as detailed in Supplementary Note 6, possibly resulting from the model’s 2D nature. It would be interesting to perform further experiments in which the NV-magnet distance and/or magnet thickness are varied to further develop and test the concepts of NV-relaxometry of spin waves. These relaxation measurements can be extended with and T2 spectroscopy techniques32 to characterize a spin–noise spectrum over a range of frequencies at a fixed value of magnetic field.


In this work, the ferromagnetic microdisc was fabricated directly on top of the surface of a diamond containing NV centres. As such, the NV centres were fixed in space with respect to the disc. This configuration enables a determination of the lateral NV position to about 400 nm (set by the optical diffraction limit), and allows local detection of magnetic excitations with spatial variations on the scale of the 50-nm NV–disc distance. A variety of techniques may be used to improve the lateral imaging resolution to the few-nanometre scale: for example, optical superresolution methods33, real-space magnetic field gradients created by scanned magnetic tips34, and Fourier-imaging techniques similar to conventional MRI35. Because of the point-like nature of the NV centre, the ultimate imaging resolution is given by how close one can bring an NV centre to a sample and how well one can control its position with respect to the sample. As shown in several recent studies (see, for example, refs 20, 32), NV centres can readily exist at just a few nanometres below the diamond surface. Although the proximity of a metallic sample may quench fluorescence for emitter-metal distances below 10 nm (ref. 36), this should allow studies of, for example, a skyrmion lattice. Looking ahead, the complementary NV magnetometry techniques, demonstrated here for spin waves in a ferromagnetic disc, open up exciting possibilities to explore a wide variety of magnetic excitations in nanoscopic systems under ambient conditions. The techniques are directly applicable to imaging highly localized spin-wave excitations such as edge modes in nanomagnets37 or, when combined with THz sources38, high-energy excitations in patterned high-coercivity ferromagnets or in antiferromagnets. We envision nanometre-scale studies of magnetic vortices and skyrmions, atomically engineered quantum magnets10 and spin ice. In addition, these techniques can be applied to characterize the magnetic fields generated by edge currents in quantum Hall systems and topological insulators13.


Application of Bext

We apply the static external field Bext along the axis of target NV centres to assure good optical spin contrast (Supplementary Note 7). Bext is thus oriented at an angle of 54° with respect to the plane of the disc. Throughout this work, we select NV centres with equally oriented crystal axes. To avoid hysteresis in the disc, in all measurements we first apply a large field (Bext>700 G) and then sweep the field down in small steps.

D.c. magnetometry

The ESR frequencies of an NV centre in a magnetic field B are determined by the Hamiltonian , where Si=x,y,z are Pauli spin matrices for a spin 1, D is the zero-field splitting, and z denotes the direction of the NV centre crystal axis. We use this Hamiltonian to calculate the projection of the magnetic field onto the NV-axis from the measured ESR frequencies (Fig. 1c,d), as described in detail in Supplementary Note 7.

Normalization procedure

To obtain the signal in Fig. 3, we apply the pulse sequence in Fig. 3a and normalize the photoluminescence (PL) on spin readout using two reference measurements. In these measurements, we apply the sequence of Fig. 3a without the MW drive field and with the final π/2-pulse around the x or the –x axis, which yields minimum and maximum PL values. Using these bounds we normalize the PL measured at the end of the pulse sequence in Fig. 3a to obtain Beff (Supplementary Fig. 5). We then divide Beff by the square of the driving field |bD|2, which we independently determine by measuring the Rabi frequency of NVref as a function of the ESR frequency (Supplementary Fig. 6). The measured linear scaling of Beff with the MW-source power validates this normalization procedure (Supplementary Fig. 7). The normalization is described in detail in Supplementary Note 5.

Stray-field characterization of magnetization and spin noise

In this section, we describe the properties of stray-field magnetometry of magnetization and spin noise which are relevant for the experiments presented in this work. In particular, we will show that the NV centre probes the spatial variations in the magnetization on the scale of the NV–disc distance, and we will derive the model used for the calculations of the field-dependent magnetic noise spectrum at the NV-site shown in Fig. 4 (for more details, see Supplementary Note 6).

An NV spin at a distance d from the surface of the disc is mostly sensitive to local variations in the magnetization on the scale of d. Intuitively, this can be easily understood: on one hand, a homogeneously magnetized infinite plane generates no stray field. On the other hand, the stray field generated by variations in the magnetization on a scale much smaller than d averages out at a distance d. More formally, it can be shown that the stray field B(r0) at position r0=(ρ0,d) (Supplementary Fig. 7) produced by a certain 2D spin texture S(ρj) is given by:

with D(ρj -ρ0,d) being the dipolar tensor. We note that by ‘two-dimensional spin texture’ we imply a spin texture that varies in the plane but not along the thickness of the film. We consider a thin magnetic film having a saturation magnetization Ms and thickness t. We move to the continuous limit by calling Γ=MSt/(gLμBS) the number of magnetic dipoles per unit surface. Here μB is the Bohr magneton, gL the Landé g-factor of the local spin S. We obtain:

where k is a 2D vector in reciprocal space, and φ0φk is the angle between the in-plane ρ0 and the k vector. Provided with such a formalism, we adopt cylindrical coordinates and compute the Fourier transform of the components of the dipolar tensor:

where S(k) is the spatial Fourier transform of S(ρ), φ–φk is the angle between ρ and the k vector, and φk is the angle between k and z (Supplementary Fig. 8). We see that stray-field detection works as a spatial Fourier filter, with a kernel given by:

The NV-centre stray-field sensor is point-like, contrary to, for example, nano-SQUIDs or Magnetic-Resonance Force Microscopy probes. Therefore, the stray field computed with equation (3), after a proper projection along the NV axis, directly describes how spatial modulations of the local magnetization couple to the NV spin. We obtain the following general set of conclusions, in principle valid for any S(ρ) distribution. First, all the elements in the kernel contain the term k exp(-dk), which peaks at k=1/d. Stray-field magnetometry is insensitive to Fourier components of the magnetization whose spatial frequency coincides with the condition D(k,d)=0. Accordingly, an NV center cannot detect stray field originating from a uniformly magnetized (k=0) surface or from a spin structure that varies in space within distances much shorter than d. The region of maximum sensitivity corresponds to wavevectors k1/d, which in a 2D region of k-space defines an annulus. We refer to this region in k-space as detection annulus of the technique. Second, the in-plane stray-field component orthogonal to the wavevector k is always zero. We note that in equation (3) we have assumed that all the magnetic moments along the thickness t have the same distance d from the NV centre.

The formalism just described can be used to derive a general expression for the stray magnetic-field noise generated by spin noise in a thin magnetic film. Spin fluctuations δSj(t) in the disc will produce a time-dependent field δB′(r0,t) at the NV site, which can be written as:

Here we inserted a rotation matrix to express the field in an xyz′ frame which has the z′ axis parallel to the NV axis (that is, the xyz′ frame is in general rotated by an angle θ around the y axis with respect to the xyz frame, see Supplementary Fig. 8). We first compute the spectral density of the stray magnetic-field noise at energy ωα,β along a general direction η:

which has units of T2Hz−1. Here denotes an ensemble average over the magnet’s spin degree of freedom. An expression for the stray magnetic-field noise can be obtained by inserting equation (6) into equation (7):

where we have defined S={Sx,x,Sy,y,Sz,z}, with:


and the are the matrix elements of equation (5).

The matrix N(k,d) filters in k-space the spin fluctuations of the magnetic thin film. Note that the integral in equation (8) contains a kernel k2exp(−2dk) for all the components of the N(k,d) matrix. The detection annulus changes therefore slightly with respect to the case of static magnetometry.

The model linking the relaxation rates of the NV centre to the spin–noise in the disc is discussed in Supplementary Note 6. In particular, the field-dependent noise spectrum and associated NV-relaxation rates shown in Fig. 4c are obtained from the expression:

where T=300 K is the temperature, , W is the width of the FMR excitation, Δ its field-dependent gap, D the spin stiffness and S the value of the local spin.

Additional information

How to cite this article: van der Sar, T. et al. Nanometre-scale probing of spin waves using single electron spins. Nat. Commun. 6:7886 doi: 10.1038/ncomms8886 (2015).