We demonstrate continuous infrared spectra from 20 nm sample spots, by combining dispersive Fourier-transform infrared spectroscopy (FTIR) with scattering near-field microscopy (s-SNOM). With the “apertureless” tip of a standard AFM cantilever in one arm of a Michelson interferometer the spectra arise simultaneously in amplitude and phase. The effect of near-field phonon resonance of SiC is used to verify background-free s-SNOM operation, and to determine the absolute scattering efficiency, at 6 cm−1 spectral resolution. We further report first evidence of free-induction decay from a scatterer composed of parts coupled by near-fields. This is possible only with broadband illumination. It offers a new, unique tool to discriminate against background scattering artifacts.
© 2009 OSA
Near-field microscopy by Rayleigh scattering from a tip has the proven potential of tip-limited resolution of typically 20 nm. This is independent of the wavelength which can be chosen throughout the visible, infrared, THz and even microwave regions . Disturbing “background” scattering from parts outside the tip's apex region are routinely suppressed by tapping the tip against the sample and demodulating the light signal at the tapping frequency or its harmonics. Numerous applications have been established using monochromatic s-SNOM, for example, the detection of nanosize metallic regions that occur in the insulator-metal phase transition , or the quantitative mapping of free-carrier concentration in semiconductor nanodevices . Yet the future impact of s-SNOM requires a spectroscopic operation exploiting the infrared and far-infrared vibrational fingerprints. These are routinely assessed in research and industry, using FTIR spectrometers for identification and quantifying chemical composition. Monochromatic s-SNOM has already succeeded in mapping vibrational resonances by repeated s-SNOM imaging at varied frequency, and subsequent extraction of spectra [4–8]. This procedure is, however, rather laborious and prone to errors from non-reproducibilities of the scan process. For example, the sample might drift, the tapping conditions might change, and the tip might erode or pick up debris.
2. Design of broadband s-SNOM
Our present experiment uses spectrally broadband illumination of a novel, commercial s-SNOM (NeaSNOM, neaspec.com), for recording a spectrum at each pixel while scanning (Fig. 1 ).
Interferometric operation is achieved by a dispersive Michelson configuration, resembling the earlier homodyne , multi-heterodyne , and pseudo-heterodyne setups . The reference arm's length is continuously varied and an interferogram is recorded for subsequent Fourier-transformation (FT). We use a coherent beam with a broad spectrum resulting from difference-frequency generation in a 200 µm thick GaSe crystal (ATOM, eletot.tsu.ru), of 10-fs Ti:S laser pulses at 125 MHz repetition and 500 mW quasi-c.w. power. The crystal is oriented to generate the band between 9 and 12 µm at 5 µW quasi-c.w. power. The back-scattered infrared beam is partially reflected at the beam splitter, a 2 mm thick uncoated ZnSe plate, and focused on a HgCdTe detector (KLD-0.25-J1, kolmar.com). The signal is amplified by 60 db (HVA-10M-60-B, femto.de) and processed in a lock-in amplifier (EG&G5302, princetonappliedresearch.com). The s-SNOM's focusing mirror has about 20 mm effective focal length and accepts a collimated beam in a 15 mm aperture. The incident beam is at about 30° inclination to the horizontal sample surface and is vertically polarized. The sample is scanned while the commercial cantilevered Pt-coated tip (PPP-NCHPt-20, nanosensors.com) is fixed and oscillates at 310 kHz. An integrated microscope provides a top view of the sample, the cantilever, the AFM laser spot, and the illuminating spot which helps in the alignment of both the AFM and s-SNOM operations.
The recording of interferograms is done with an oscilloscope (Wavesurfer 422, lecroy.com). This also performs on-line FT for previewing spectra at 20 cm−1 resolution, as limited by nonlinearity in the mirror translation stage (P-628, pi.ws). We overcome this constraint by off-line resampling according to frequent calibration interferograms taken with a CO2 laser beam, set at about 100 µW by a step attenuator (102, lasnix.com). With our choice of 1.7 mm long interferograms taken in 2 s the resolution becomes 6 cm−1. The interferometer arm length of about 25 cm is found sufficiently short to keep, in the thermostatted laboratory, thermal drifts small enough that the phase calibration stays valid over hours.
2. SiC near-field phonon resonance
In view of the rather low power from our broadband source the s-SNOM is initially aligned with the CO2 laser beam. The reference mirror position for positive interference of all frequencies (white light position, WLP) is approximately set with the help of a ruler (the optical path length inside the NeaSNOM is 2 x 17 cm). The power efficiency of backscattering from the tip is found to be of the order of 0.25%, which corresponds to a detector signal level of about 5% of the input signal (Fig. 2 ). The latter is experimentally determined by an auxiliary probe arm with a full mirror.
Similar as in earlier reports [9,11,12], the modulated amplitudes of backscattering are found to decrease with n, here roughly by a factor 5 per harmonic order. With the non-resonant Au sample the spectral shapes are similar to that of the input spectrum, except for the direct scattered one, s0; its distortion resembles that found earlier with a different tip shape, and may indicate antenna resonance . The phase spectra are flat and unshifted within 20° which means the locus of backscattering remains within ± 140 nm constant for all spectral elements. Approach curves (not shown) are regularly taken, with the interferometer kept fixed, to ascertain that the n = 2, 3 responses are dominated by near-field interaction.
Figure 2b displays the spectra obtained with a SiC sample which possesses a well-studied near-field phonon resonance in the mid infrared [4,9,13–17]. As expected for this resonance, the amplitude spectra for n = 2, 3 exhibit a ca. 60 cm−1 wide peak (FWHM) at ca. 920 cm−1 exceeding the value of Au. The n = 0, 1 spectra, in contrast, appear flat up to about 980 cm−1 where the amplitude markedly decreases. This is expected for the far-field response due to Fresnel reflection in the Reststrahlen region of SiC, as illustrated in Fig. 2 of ref . The phase spectra exhibit a monotonic increase in the Reststrahlen region. This increase is enhanced in the near-field interaction. Our general conclusion is that spectroscopic s-SNOM generates meaningful amplitude and phase spectra. Specifically, the near-field interaction dominates the spectra from demodulation order n = 2 up, given the tip geometry and tapping paramters as used here.
3. Background-free detection at first harmonic
The results (Fig. 3 ) of a second measurement series with a different tip from the same batch indicate, in the n = 1 spectrum, the presence of substantial background scattering; this could come from a non-perfect alignment of the focus to the tip or may reflect an antenna property of the tip. We present this series because it illustrates a new way to recognize background contamination, by inspecting pulse-type interferograms obtainable only with broadband illumination. In Fig. 3b the centrally plotted interferogram of the input (black, scaled /100) lasts for a time span A. It can be understood as the autocorrelation of a ca. 3-cycle input pulse. Nearly congruent with it are interferograms of the two samples measured at 3 µm retraction from contact (dotted red and green). Since such a retraction must fully suppress the near-field interaction [1,11], the dotted spectra (Fig. 3a) designate pure background scattering. We assume such background spectra should prevail nearly unaltered also at contact. This is confirmed by comparison with the n = 1 interferogram of Au. It starts out congruently in shape with the input, but then continues ringing for a time span B. The difference of both interferograms, on and off contact, is approximately identical in shape with that of the n = 2 interferogram. The latter represents the pure near-field response, as concluded above from approach curves, and as also can be seen by comparing the n = 2 spectrum of Fig. 3a with Fig. 2b and previous reports [9,16].
We thus suggest that the near-field response can be approximately determined even from background-contaminated n = 1 interferograms, during time span B, owing to the fact that the background and the near-field features appear essentially time-separated. Since the signal level for n = 1 is about 5x larger than for n = 2, the choice of using n = 1 interferograms instead of n = 2 interferograms has a decisive advantage for performing the initial s-SNOM setup because it requires a 25x shorter measuring time for the same S/N ratio. Note that, in contrast, the spectral curves (red, full and dotted, in Fig. 3a) would give no hint of the presence of a background. Our observation is corroborated by the interferograms taken with the SiC sample (Fig. 3b). In these, the ringing lasts for a prolonged time span C. Furthermore, it starts with a substantial phase shift compared to the background feature, which leads to a minimum in the s1 envelope. Both features are related to the phonon resonance of SiC. The relatively long ringing marks the high quality factor owing to substantial energy stored in the cavity formed by the tip apex and the sample.
4. Free-induction decay
A prolonged response (ringing) is well known as free-induction decay (FID) in many other fields of coherent spectroscopy mainly of quantum systems such as spin or vibrational/electronic two-level systems. What we observe here is the first evidence of FID in a classical near-field coupled system, namely a scatterer close to a material surface. While implications and analogies with quantum systems are beyond the scope of this letter, we emphasize the FID's interesting practical application for s-SNOM adjustment and operation as already explained. We add another aspect, which may be of high interest in future studies. The interferogram could detect retardation generated by internal delay within a complex scatterer caused, for example, by surface plasmon propagation as considered in refs [18,19]. Intra-scatterer retardation as small as 10° could be detected, which at 1 µm wavelength would correspond to a propagation time as short as 83 as.
5. Influence of tapping amplitude
To probe the influence of the tapping amplitude on both background and near-field signals we performed a systematic variation and display the result in Fig. 4 .
A linear behaviour is found for the pure background signal (dots at n = 1), as to be expected, whereas the other curves show a saturated behaviour obviously due to the near-field parts. In the n = 1 case, for example, at 20 nm the near-field part obtained by subtracting the off-contact from the on-contact interferograms (triangles) equals that of the background (dots), but at 50 nm tapping amplitude it amounts to only 50%. This trend is in accord with earlier estimations [20,21]. These predict a slowed increase of the near-field amplitude once the tapping amplitude exceeds the size of the near field, which is of the order of the tip radius, typically 20 nm in our study.
6. Proximity effect
As a final illustration of broadband s-SNOM spectra we demonstrate the influence of a nearby scattering object, the edge of an Au film, which is situated towards the focusing mirror. From former studies of plasmon-resonant scatterers [22–24] or edge scatterers  we expect to obtain an increased scattering caused by the additional illumination of the tip due to the proximal scatterer. The results show that such an enhancement indeed occurs, amounting to factors between 2 and 4, and that the spectral signatures stay largely unaffected (Fig. 5 ).
The spectra shown in this work were acquired by averaging 10 to 100 interferograms, each lasting 2 s. A boost of the present beam power of 5 µW by at least an order of magnitude would eliminate the need of averaging, and ease the way to spectroscopic near-field images. Altogether, we have shown a robust setup and procedure which uses a broadband light source for illumination and for obtaining local spectra. Our setup requires less installation cost and less computational effort than the former coherent dual frequency-comb system . The present method can readily be used with other types of light sources such as synchrotrons and in other frequency ranges such as, for example, covered by a white light continuum beam.
We acknowledge discussions with M. Brehm, A. Schliesser, N. Ocelic, R. Hillenbrand, and A. Apolonskiy. Supported by Deutsche Forschungsgemeinschaft through Cluster of Excellence Munich-Centre for Advanced Photonics.
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