A spectral anomaly exhibiting pronounced asymmetry is observed in the emission spectrum for nanocavities when they are pumped by the charged boron vacancy VB and have a high Q-factor above a threshold of 10 000. In contrast, cavities without VB centers always exhibit trivial Lorentzian emission. These observations are well explained by the feature of VB that its light–matter interaction is induced by local phonon modes. Moreover, we find that in nanocavities the local phonon modes arise from the coupling between VB lattice phonons and cavity mechanical modes, supported by the spatially resolved spectroscopy of VB and resonant spectroscopy of the cavity photonic mode. Our results reveal a novel system involving the coupling in both the photonic and phononic degrees of freedom between the active material and the nanocavity. Such an emitter–optomechanical interaction system shows great potential in non-trivial quantum photonic devices and provides a platform to interface spin defects, photons, and phonons.

Light–matter interaction between active quantum materials and photons confined in high-Q nanocavities is the central pillar in the study of cavity QED.1–4 Conventional electron–photon coupling is described by the Jaynes–Cummings model and exhibits a trivial symmetric feature with respect to the spectral detuning.5,6 Recently, cavity optomechanics has emerged, in which the coupling between photonic and mechanical modes allows coherent phonons to be controlled via photons or vice versa.7–10 This opens up new perspectives for applications in ultraprecise sensing and metrology,11,12 as well as building non-trivial optical devices with novel functionalities and asymmetric responses.13–16 In addition, the cavity mechanical modes enable new approaches to control active quantum material through the phononic degree of freedom, e.g., tuning the emission energy and linewidth as reported for quantum dots and 2D materials.17–21 The multi-modal coupling paves the way to quantum transduction between different degrees of freedom and opens new avenues in cavity QED.22–24 

Traditional quantum emitters are dominated by zero-phonon emission and can couple directly to local optical fields without the participation of phonons. As such, the native phononic effects are not pronounced, and investigations are usually subjected to the extrinsic mechanical driving.17–19 In contrast, the charged boron vacancy VB in hexagonal boron nitride (hBN) is a recently explored quantum emitter25–29 that has a weak zero-phonon line, with emission instead being dominated by phonon-induced processes.30–33 This is indicative of robust electron–phonon polarons that arise from local phonon modes and couple to the optical field. As such, by creating VB centers in an hBN nanobeam cavity,33 we realize a novel multi-modal interaction involving the coupling in both the photonic and phononic degrees of freedom between the spin defects and the nanocavity.

We investigate the multi-modal interaction system using spatially resolved photoluminescence (PL) and Raman spectroscopy. A spectral anomaly with pronounced asymmetry is observed in the line shape of PL from the cavity photonic mode only when the Q-factor is above a threshold of 104. We construct a numerical model that accounts well for the experiment, based on the fact that the light–matter interaction of VB is induced by local phonon modes,30–33 which differs from the traditional Jaynes–Cummings coupling. Moreover, compared to the standard Lorentzian emission for cavities without VB centers, the spectral anomaly with VB reveals that the local phonon modes in such systems are not isolated but rather arise from the coupling between VB lattice phonons and cavity mechanical modes. This coupling is further supported by spatially correlating the luminescence of VB in freely suspended structures34 and resonantly exciting the cavity photonic mode.9 These results indicate the great potential of hBN nanocavities for applications in non-trivial optical devices.

The structure of our hBN/Si3N4 nanobeam cavity is schematically depicted in Fig. 1(a). The confinement for nanophotonic modes is achieved by locally chirping the photonic crystal periodicity around the cavity center. The cavity photonic mode exhibits a high Q-factor of 105, limited only by the spectral resolution of our detection system.35,36 In addition to the nanophotonic mode, the cavity also hosts nanomechanical modes since the hBN/Si3N4 nanobeam is freely suspended but clamped at both ends.21 We use a 30 keV N+ ion beam of 1013 ions/cm2 fluence (dose) to create VB centers within the volume of the photonic mode. Fabrication procedures are presented in Sec. I A of the supplementary material. Recent works have reported that the zero-phonon line of VB is at 773 nm and exhibits very weak emission intensity, while its phonon-induced emission gives rise to a broad spectrum centered at 800 nm and coupling of local phonon modes to the optical transitions of the VB center.30–33 As such, the system involves coupling between electronic transitions, VB lattice phonons, cavity photons, and cavity nanomechanical modes, as a multi-modal emitter–optomechanical interaction depicted schematically in Fig. 1(b).

FIG. 1.

(a) Schematic of the cavity with or without ion irradiation. The irradiated cavities exhibit a spectral anomaly with a pronounced asymmetric line shape in the cavity emission. In contrast, no asymmetry is observed without irradiation. Raw spectra recorded from four irradiated cavities (C1–C4) and four non-irradiated cavities (N1–N4) are shown as examples. (b) The light–matter interaction between the electronic transition of VB and the cavity photonic mode is induced by local phonon modes. The local phonon modes arise from the coupling between the lattice phonon of VB and the cavity mechanical modes. (c) Calculated emission spectra of cavity mode when the electron–photon coupling is direct (dashed line) or induced by the local phonon modes (solid line). (d) The asymmetry has a threshold cavity Q-factor of 10 000. The insets show the fitting method of cavity emission, including a major peak (red) and a minor replica (blue). The asymmetry is quantified by the relative intensity (peak area) of the replica to the major peak.

FIG. 1.

(a) Schematic of the cavity with or without ion irradiation. The irradiated cavities exhibit a spectral anomaly with a pronounced asymmetric line shape in the cavity emission. In contrast, no asymmetry is observed without irradiation. Raw spectra recorded from four irradiated cavities (C1–C4) and four non-irradiated cavities (N1–N4) are shown as examples. (b) The light–matter interaction between the electronic transition of VB and the cavity photonic mode is induced by local phonon modes. The local phonon modes arise from the coupling between the lattice phonon of VB and the cavity mechanical modes. (c) Calculated emission spectra of cavity mode when the electron–photon coupling is direct (dashed line) or induced by the local phonon modes (solid line). (d) The asymmetry has a threshold cavity Q-factor of 10 000. The insets show the fitting method of cavity emission, including a major peak (red) and a minor replica (blue). The asymmetry is quantified by the relative intensity (peak area) of the replica to the major peak.

Close modal

We begin by comparing the emission spectral line shape observed from the cavities with and without irradiation. All cavities are excited using a 532 nm cw-laser having a spot size of 1μm and a power of 120μW. The cavity photonic mode is hence excited by the emission of VB centers in hBN (irradiated) and/or filtered light arising from other native luminescent defects in the hBN and underlying Si3N4 (non-irradiated). Typical spectra recorded from four representative cavities with and without irradiation are presented in the upper and lower panels of Fig. 1(a), respectively. The emission of vacancies in hBN is very broad, with an FWHM over 150 nm,33 and thereby features as a plane background in the spectra in Fig. 1(a), for which the wavelength range is smaller than 1 nm. The peaks in Fig. 1(a) are from the photonic mode of the cavities. The photonic modes are at a wavelength of 800 nm, which is within the broad phonon sideband emission of VB.33,37,38 

Remarkably, for the N+ irradiated cavities, we observe a strongly asymmetric line shape of cavity emission that is broadened on the short wavelength (high energy) side. In contrast, this spectral anomaly is not observed in the control experiment, i.e., non-irradiated cavities. The asymmetric line shape of cavity emission reveals the non-Lorentzian local density of optical states, which usually arises from multiple coupled heterocavities39–41 or strong photon–phonon coupling.9,13,42 In our sample, the nanobeam cavity does not couple to other neighbor cavities,35 and thereby, the asymmetric line shape is attributed to the photon–phonon coupling. However, the native optomechanical coupling between cavity photons and cavity mechanical modes is not pronounced, which is demonstrated by the symmetric line shape in control experiments without irradiation shown in the lower panels of Fig. 1(a). This reveals the key role of VB in the non-Lorentzian cavity emission. Based on the facts that the VB emission is dominated by phonon-induced processes30–33 and 2D materials support the phononic coupling between the cavity and lattice degree of freedom,21 we explain the strong photon–phonon coupling by the fact that the local phonon modes in the system arise from the coupling between VB lattice phonons and cavity mechanical modes, as depicted in Fig. 1(b). As such, the emission of VB pumps the local phonon modes that also couple to the cavity photonic mode, giving rise to the photon–phonon coupling stronger than the native optomechanical system (control experiments) and the asymmetric line shape. We construct a numerical model with the phonon-induced cavity-VB interaction to reproduce the experimental data. The Hamiltonian of the multi-modal cavity QED system can then be written as
(1)
including the four terms corresponding to the emitter, photon, phonon, and the couplings between them. σA,B (A, B ∈ {X, G}) is the Dirac operator for the emitter with the ground (G) and excited (X) state, a+/a are the ladder operators for cavity photons, and q+/q are the ladder operators for phonons. The coupling term Hc in Hamiltonian is written as
(2)
where He-q describes the electron–phonon coupling with the strength λe-q and Hp-q describes the photon–phonon coupling with the strength λp-q.9,43, He-p describes a phonon-induced electron–photon coupling involving k phonons, based on the fact that VB emission is dominated by phonon-induced processes.30–33 More details of the calculation can be found in Sec. I D of the supplementary material. Using the model in Eq. (2), we calculate the emission from the cavity photonic mode by solving the master equation. Typical results are presented in Fig. 1(c), showing the spectral form at resonance ωa = ωX. The dashed line corresponds to the case of k = 0, which means the electron couples to the phonon, and the photon couples to the phonon, but the electron directly couples to the photon without the participation of the phonon. This limit corresponds to the usual Jaynes–Cummings coupling that considers the coupling between photons and the electronic system but does not include any tripartite (phonon–electronic–photon) coupling. In this case, the emitter has both the bright zero-phonon line and the phonon sideband. The solid line in Fig. 1(c) corresponds to the phonon-induced coupling with k = 4 for the cavity-VB system. This case corresponds to four phonon mediated couplings motivated by Ivády et al.,30 who predicted the Huang–Rhys factor of VB to be 3.5. The results in Fig. 1(c) clearly show that the asymmetry in the emission line shape is suppressed for the case of k = 0 but becomes pronounced with the multipartite interaction. The theoretical calculation agrees well with our experimental observations, indicating how the multipartite interaction plays crucial roles in the non-trivial asymmetry of the cavity line shape.

In addition, we use bi-peak fitting, including a major peak (red) and a minor replica (blue) at the shorter wavelength side, to quantify the asymmetry, as shown by the example in Fig. 1(d) inset. The Voigt peak (convolution of Lorentz and Gaussian peaks) is used for the fitting because the spectral broadening of our detection system results in a convolution of signals by a Gaussian window function with a width of 50 pm.36 After deconvolution, we extract the real Lorentzian linewidth, e.g., with the values of 0.04–0.09 mm for the cavity modes shown in Fig. 1(a), corresponding to the Q-factors of 8 × 104 to 2 × 105. The high Q-factors are owing to the design of the hybrid nanobeam cavity that avoids etching rough photonic crystal nanoholes in hBN.35 The asymmetry is quantified via the intensity ratio of the replica to the major peak, and the results of all measured cavities are presented in Fig. 1(d). By comparison, the solid line in Fig. 1(d) is the calculation result using Eq. (2), which well reproduces the experimental data. As shown, when the cavity Q-factor is smaller than 104, the replica is suppressed, and the cavity emission is a standard Lorentz peak (after deconvolution). In contrast, when the Q-factor exceeds 104, the spectral anomaly arises, and the cavity emission becomes non-Lorentzian. This threshold behavior indicates that the multi-modal light–matter interaction needs to exceed the system decay rate (1/Q) for the spectral anomaly. Despite the model in Eq. (2) being rather simple, it nicely captures the essential physics underpinning our experimental observations, e.g., the phonon-induced coupling as shown in Fig. 1(c) and the threshold for asymmetry as shown by the solid line in Fig. 1(d).

In the phonon-induced coupling model shown in Fig. 1(b), the local phonon modes arising from the coupling between VB lattice phonons and cavity mechanical modes play central roles. To further support this point, we next probe the local phonon modes in their coupling to the photons in cavity photonic mode or the electronic transition of VB individually. We first explore the phonon coupling for cavity photons using resonant Raman spectroscopy and present the results in Fig. 2. We tune a narrowband (1 MHz) cw laser from 730.998 to 731.012 nm over the resonance of a cavity photonic mode, as depicted by the inset in Fig. 2(a). Color lines in Fig. 2(a) are the corresponding Raman spectra excited by the tunable laser. As denoted by the arrows, the sharp peak corresponding to the Eg mode from Si3N444 and the broad peak corresponding to the local vibrational mode from VB45 are observed. Details of the identification of Raman peaks can be found in Sec. II B of the supplementary material. We extract the intensity of Raman peaks and plot it as a function of drive laser detuning from the cavity mode in Fig. 2(c).

FIG. 2.

Probing local phonon modes in the photon–phonon coupling. (a) Inset depicts the resonant Raman spectroscopy that tunes the wavelength of the excitation laser through a cavity photonic mode (black spectrum). The red and blue spectra are Raman signals corresponding to the excitation laser having red and blue detuning, respectively. (b) The enhancement of the Raman peak from the Si3N4 phonon is nearly symmetric with the laser-cavity detuning. In contrast, the enhancement of the Raman peak from VB phonon is asymmetric: it vanishes slowly at blue (heating) and quickly at red (cooling) detunings. The heating and cooling arise from cavity mechanical modes, indicating that the cavity mechanical modes participate in the coupling between cavity photons and VB lattice phonons.

FIG. 2.

Probing local phonon modes in the photon–phonon coupling. (a) Inset depicts the resonant Raman spectroscopy that tunes the wavelength of the excitation laser through a cavity photonic mode (black spectrum). The red and blue spectra are Raman signals corresponding to the excitation laser having red and blue detuning, respectively. (b) The enhancement of the Raman peak from the Si3N4 phonon is nearly symmetric with the laser-cavity detuning. In contrast, the enhancement of the Raman peak from VB phonon is asymmetric: it vanishes slowly at blue (heating) and quickly at red (cooling) detunings. The heating and cooling arise from cavity mechanical modes, indicating that the cavity mechanical modes participate in the coupling between cavity photons and VB lattice phonons.

Close modal

The steady state population of cavity photons is obviously enhanced around the resonance. Cavity photons then couple to the lattice phonons in Si3N4 or VB center, thereby enhancing the Raman signals.46 For the Si3N4 phonon presented in the upper panel in Fig. 2(b), this enhancement is weak (10%) and nearly symmetric with respect to the detuning. The line shape reflects the real peak wavelength of the cavity mode, 731.007 nm, and the real linewidth, 3.5 ± 0.1 pm, corresponding to a Q-factor >2×105 in the ultrahigh regime.47 The symmetry confirms that cavity photons directly couple to Si3N4 phonons, and the enhancement simply arises from a resonance in the optical density in the sample. In complete contrast, from the intensity of the VB phonon presented in the bottom panel of Fig. 2(b), we observe a much stronger enhancement (>10×) around the resonance that exhibits a pronounced asymmetry with respect to the detuning. Notably, the intensity reduces rapidly at red detunings while being much slower for blue detunings. This observation reveals that the cavity mechanical modes induce coupling between cavity photons and VB phonons because the population of cavity mechanical phonons is reduced at red detunings (cooling) while enhanced at blue detunings (heating).9 As such, the correlation between VB lattice phonons and cavity mechanical phonons in the local phonon modes is demonstrated in the coupling to cavity photons.

Finally, we explore the coupling of local phonon modes to the electronic transition of VB. For this experiment, we fabricate a sample as depicted in Fig. 3(a). The sample is homogeneously irradiated by 30 keV N+ ions with an ion fluence (dose) of 1014 ions/cm2 to create VB centers in the hBN flake.37,38 Such a sample does not support cavity phononic mode but hosts cavity mechanical modes such as the one shown in the top panel in Fig. 3(a). The local amplitude of the mechanical mode generally increases for positions away from the clamping point (orange dashed line). This enables us to probe the impact of the mechanical mode by performing position dependent spectroscopy of the VB centers.34 

FIG. 3.

Probing local phonon modes in the electron–phonon coupling. (a) Schematic of the sample and typical mechanical mode. The amplitude of the mechanical mode is position dependent, generally increasing with the distance to the clamping point (orange dashed line). The right panel is the SEM image of the sample. (b) Map of normalized VB emission spectra extracted from a loop trace 0abc, denoted in the SEM image. VB emission is dominated by the phonon sideband arising from the coupling between electronic transition and local phonon modes. Anticrossings are clearly observed in the position dependence, indicating that the cavity mechanical modes participate in the coupling of local phonon modes to the electronic transition of VB.

FIG. 3.

Probing local phonon modes in the electron–phonon coupling. (a) Schematic of the sample and typical mechanical mode. The amplitude of the mechanical mode is position dependent, generally increasing with the distance to the clamping point (orange dashed line). The right panel is the SEM image of the sample. (b) Map of normalized VB emission spectra extracted from a loop trace 0abc, denoted in the SEM image. VB emission is dominated by the phonon sideband arising from the coupling between electronic transition and local phonon modes. Anticrossings are clearly observed in the position dependence, indicating that the cavity mechanical modes participate in the coupling of local phonon modes to the electronic transition of VB.

Close modal

VB emission is dominated by phonon sideband, i.e., the electronic transition couples to local phonon modes as a polaron and then emits a photon,30–33 and the photon wavelength is determined by the energy of local phonon modes. In Fig. 3(b), we present the broad phonon sideband emission of VB recorded from positions along the loop trace denoted in Fig. 3(a). The position dependence of VB emission, along with two anticrossings, is clearly observed as depicted by the dashed lines in Fig. 3(b). This is combined with the identity of spectra at the beginning and end of the loop. Similar anticrossings are also observed from the spatially resolved Raman spectra of VB (Sec. II C of the supplementary material), further supporting the generality of this conclusion. The anticrossings demonstrate the coherent correlation between VB lattice phonons and cavity mechanical modes with spatial dependence. This electron–phonon coupling in Fig. 3, combined with the photon–phonon coupling in Fig. 2, further strengthens the phononic coupling between the cavity mechanical modes and VB lattice phonons shown in the right part in Fig. 1(b), and thereby, greatly supports the non-Lorentzian cavity emission arising from the phonon-induced emitter–optomechanical interaction.

In summary, we report on the interaction between VB centers and optomechanical modes in a hBN nanocavity. Experimental results reveal that in both the phonon couplings to electrons and photons, the local phonon modes are not isolated but arise from the coupling between VB lattice phonons and cavity mechanical modes that are strongly correlated. This phonon-induced interaction between the electronic transition in VB and the cavity photonic mode results in the spectral anomaly in the emission from the hBN nanocavity. Such a multi-modal system provides exciting opportunities to interface fixed quantum degrees of freedom to photonic and phononic modes using 2D materials and opens up interesting perspectives for quantum sensing and quantum transduction.

The supplementary material includes the detailed methods and results of control experiments to support the conclusions.

All authors gratefully acknowledge the German Science Foundation (DFG) for the financial support via Grant Nos. FI 947/8-1, DI 2013/5-1, AS 310/9-1, and SPP-2244, as well as the clusters of excellence MCQST (EXS-2111) and e-conversion (EXS-2089). J. J. F. gratefully acknowledges the state of Bavaria via the One Munich Strategy and Munich Quantum Valley. C. Q. gratefully acknowledges the support from the Chinese Academy of Sciences Project for Young Scientists in Basic Research (Grant No. YSBR-112) and the National Natural Science Foundation of China (Grants Nos. 12474426, 12494601). C. Q. and V. V. gratefully acknowledge the Alexander v. Humboldt Foundation for the financial support in the framework of their fellowship program. The support from the Ion Beam Center (IBC) at HZDR is gratefully acknowledged.

The authors have no conflicts to disclose.

Chenjiang Qian: Conceptualization (lead); Data curation (lead); Formal analysis (lead); Funding acquisition (lead); Investigation (lead); Writing – original draft (lead); Writing – review & editing (equal). Viviana Villafañe: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Martin Schalk: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Georgy V. Astakhov: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Ulrich Kentsch: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Manfred Helm: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Pedro Soubelet: Data curation (equal); Investigation (equal); Writing – review & editing (equal). Andreas V. Stier: Conceptualization (equal); Data curation (equal); Formal analysis (equal); Investigation (equal); Writing – review & editing (equal). Jonathan J. Finley: Conceptualization (lead); Data curation (lead); Formal analysis (lead); Funding acquisition (lead); Investigation (lead); Writing – review & editing (equal).

The datasets generated and analyzed during the current study are available from the corresponding author upon reasonable request.

The hBN/Si3N4 hybrid nanobeam cavity is fabricated through e-beam lithography (EBL), inductively coupled plasma reactive ion etching (ICPRIE), the viscoelastic dry transfer method, and wet underetching. First, we prepare a Si substrate with 200 nm Si3N4 grown by low pressure chemical vapor deposition (LPCVD) on top. Then, we use EBL and ICPRIE to etch periodic nanotrenches in Si3N4. After removing the residual resist, we transfer the hBN flake with a thickness of 100nm on top of the nanotrenches. Finally, we use EBL and ICPRIE to etch the nanobeams, followed by a wet underetching to remove the bottom Si. Detailed fabrication procedures are presented in Sec. I A of the supplementary material.

The sample is excited using a 532 nm cw-laser for the spatially resolved spectroscopy or a tunable cw-laser for the resonant spectroscopy of the cavity photonic mode. The laser has a spot size 1μm and the excitation power 120μW. PL and Raman signals are recorded by a confocal micro-PL setup. The objective has a magnification of 100 and a NA of 0.75. The PL and Raman spectra of VB centers are collected by a matrix array Si CCD detector in a spectrometer, with a focal length of 0.55 m and a grating of 300 grooves per mm. The PL spectra of cavity photons are collected by the same detector and spectrometer but with a grating of 1200 grooves per mm.

The theoretical emission spectral form of the cavity photonic mode is calculated by solving the steady state of the master equation,
where ρ is the density matrix of the system, H is the Hamiltonian, and the Liouvillian superoperator L(cn) describes the Markovian processes corresponding to the pump and decay in the system. Detailed processes can be found in Sec. I D of the supplementary material.
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