We demonstrate a single-shot terahertz spectrometer consisting of a modified Mach–Zehnder interferometer and a microbolometer focal plane array. The spectrometer is simple to use and can measure terahertz field autocorrelations and spectral power with no moving parts and no ultrashort-pulsed laser. It can effectively detect radiation at 10–40 THz when tested with a thermal source. It can also be used to measure the complex refractive index of a sample material. In principle, it can characterize both laser-based and non-laser-based terahertz sources and potentially cover 1–10 THz with specially designed terahertz microbolometers.
Terahertz (THz) spectroscopy is essential for many applications including material and biomedical science, defense and security, and imaging and communication.1–5 Currently, THz time-domain spectroscopy (THz-TDS) is widely used for accurate THz field characterization with an electro-optic (EO) sampling3,6 or a fast photoconductive switching3,7 technique. This method requires a multi-shot scan that takes from seconds to hours, depending on the THz source power, repetition rate, desired scan step, and field of view. Generally, this method is not well-suited for applications involving irreversible processes such as material damage and structural phase transitions or requiring real-time THz field characterization. Such applications greatly benefit from a single-shot technique.
So far, various EO-based single-shot THz diagnostics have been developed8–14 and successfully applied, for example, to measure electron bunch lengths in real time15,16 and electrical conductivities of laser-ablated materials.17 However, all EO-based techniques have fundamental limitations due to the dispersive and absorptive properties of OE materials, which can distort THz fields and restrict broadband detection.18–20 In the case of ZnTe, an OE crystal commonly used with 800 nm light sources, the detection bandwidth is typically limited to below 3 THz.18 More importantly, all EO-based methods require ultrashort laser pulses for detection, limiting its applications to non-laser-based THz sources and systems.
As a stand-alone diagnostic, Fourier transform infrared (FTIR) spectroscopy21 is popularly used for THz or infrared characterization. Traditionally, FTIR spectroscopy uses a scanning scheme, although there exist stationary (or single-shot capable) FTIR variants using detector arrays.22 A recent advent of focal plane array (FPA) sensors23 that are sensitive to THz radiation has enabled rapid and vibration-free THz characterization.24 In particular, microbolometer FPAs, typically used for thermal imaging in the long wavelength infrared (LWIR) region at 8–15 μm (or 20–37 THz), have been also applied for THz beam profiling and imaging at 1–20 THz. Recently, more advanced THz microbolometers have been developed by NEC,25 INO,26 and CEA Leti27 for applications at 1–10 THz.
In this Letter, we introduce a simple single-shot THz spectrometer using a microbolometer FPA. Like the EO-based single-shot techniques,8–14 our proposed scheme can characterize THz pulses in single shots. Also, as a FTIR spectrometer, it can provide additional advantages such as broadband THz detection and no necessity of an extra laser source.
Figure 1(a) shows a schematic diagram of our experimental setup to demonstrate a single-shot FTIR spectrometer. It consists of a modified Mach–Zehnder interferometer and uses a commercial vanadium oxide (VOx) uncooled microbolometer camera (FLIR, Tau 2 336). The camera provides images of 336 × 256 pixels with one pixel size of 17 μm and can stream 14 bit images at a rate of 60 frames/s with a camera link expansion board (FLIR) and a frame grabber (NI, PCIe-1433).28–30 To examine the THz spectrometer, a silicon carbide (SiC) blackbody radiator is used as a broadband THz source. The blackbody radiator has an active area of 3 mm × 4.4 mm with an emissivity of 0.8, capable of reaching 1700 K with 24 W electric power. Previously, this type of source was used to characterize the spectral response of the microbolometer over a broad range of THz frequencies.30
The radiation from the SiC emitter is collimated by an off-axis parabolic (OAP) mirror with the focal length of 4″, and its power and beam size are controlled by an iris diaphragm. The collimated THz beam is divided into two replica beams by a 1-mm-thick high-resistivity (>10 k cm) silicon (HR-Si) beam splitter (BS) with the diameter of 2″. After reflection by gold mirrors, the two beams are focused by separate OAP mirrors with the focal length of 7.5″ and recombined by the second HR-Si beam splitter. Finally, the two beams cross at an angle θ on the microbolometer camera, producing interference fringes. Here, the parabolic mirrors (OAP2 and OAP3) are used to fit the beams into the microbolometer sensor size (5.7 mm × 4.4 mm). Also, to eliminate background thermal noise to the microbolometer, the beam from the SiC radiator is optically chopped at 5 Hz, and the image obtained with the beam blocked is subtracted from the one with the beam unblocked. Also, the difference image is averaged over 30 frames to enhance the signal-to-noise ratio unless specified otherwise.
In our crossing geometry, the relative time delay, τ, between the two beams is mapped along the horizontal axis, x, [see Fig. 1(a)] on the microbolometer sensor surface as . Here, θ is the crossing angle and c is the speed of light in air. This relationship also determines the maximum possible time window as , where w is the beam width. Also, the minimum temporal resolution, , is determined by the single pixel size, , as .
In the time domain, the interference between two THz fields, and , can be expressed as
where and are constants that do not depend on τ. The last term represents a cross correlation function (or autocorrelation if E1 = E2). The Fourier transform of ,
provides information about the spectrum .
In practice, the crossing angle, θ, does not need to be measured directly. Instead, the mapping ratio can be measured by translating the delay line in Fig. 1(a) and performing a temporal scan. For example, Fig. 1(b) shows sample interferograms taken at three different time delays τ = 0.4, 0.7, and 1 ps. Here, τ = 0 is arbitrarily chosen when the interference fringes appear at the left edge of the beam. Figure 1(c) shows a series of interferogram line-outs (horizontal) patched together with varying time delays τ. From the scan, 7.4 fs/pixel is obtained, which provides .
Figure 2(a) shows THz beam profiles obtained with four different imaging modes. I(x, y) represents the intensity profile obtained with two interfering beams unblocked. and are the ones obtained with one beam unblocked while the other beam blocked. is the difference intensity profile obtained from , which provides a background-free interferogram. Note that the horizontal stripe appearing in nearly all images in Figs. 1(b) and 2(a) is due to an optical damage made on the front silicon window of the microbolometer.
Figure 2(b) shows the THz autocorrelation, , obtained from via space-to-time mapping, also with 100 line averaging along the y-axis. The time window obtained here is around 2.4 ps, which can provide a spectral resolution down to 0.42 THz. From the Fourier transform of the autocorrelation, , the corresponding power spectrum is computed and plotted in Fig. 2(c). For comparison, both 30-shot averaged and single-shot data are presented in Figs. 2(b) and 2(c), which are in good agreement. The measured spectrum, however, is far from blackbody radiation largely due to the microbolometer's strong response at the LWIR (20–37 THz).30 In particular, the spectrum is strongly suppressed at <10 THz because of low beam power emitted from the SiC source and low sensitivity of the microbolometer at such frequencies. The spectrum also drops beyond 40 THz possibly due to a quarter-wave optical cavity adopted inside the microbolometer to limit the detection range.30 The enhanced signal at <1 THz is an artifact arising from our limited time window (2.4 ps).
An alternative method to retrieve the radiation spectrum is to use I(x, y) only, not subtracted by and . This method is applied to the data in Fig. 2(a), and the results are shown in Fig. 3. Notably, the autocorrelation in Fig. 3(a) exhibits a large slowly varying DC offset due to the uncompensated background profiles and . This, however, results in only low-frequency signals (<3 THz) in the spectrum due to the slow oscillation frequency associated with the beam intensity envelope. This near DC signal can be easily distinguished from the real spectrum. The measured spectrum here is well matched to the one in Fig. 2(c) except below 3 THz. Also, there is good agreement between the 30-shot averaged (red lines) and single-shot (blue lines) data in Fig. 3. All these imply that a single-shot acquisition without separate beam profiling is possible if the radiation beam is sufficiently large with little intensity fluctuations, and the interested frequency is not close to DC.
Our single-shot THz spectrometer can also be utilized to characterize sample materials at THz frequencies. This can be done by placing a sample before the interferometer at P1 in Fig. 1(a). For example, Fig. 4 shows our measurements of THz transmission curves with three samples—a 280-μm-thick high-resistivity silicon (HR-Si) wafer, a 26-THz bandpass filter (BPF), and a 28-THz bandpass filter. Figures 4(a), 4(c), and 4(e) show THz autocorrelations taken without (black lines, reference) and with (red lines) the sample. The corresponding spectra are obtained by the Fourier transform and plotted in Figs. 4(b), 4(d), and 4(f). From the ratio of the power spectra, the transmission curves are calculated and plotted (blue lines). Here, the transmission is fairly well determined at 20–40 THz although it is quite noisy outside the range (blue-dotted line).
As the second example, our single-shot spectrometer is used to extract the complex refractive index of of a sample material. In this method, three autocorrelations must be obtained—without the sample, , with the sample placed in P1, , and in P2, [see Fig. 1(a)]. For each case, the interfering THz fields can be expressed as , , and , where and are the transmission amplitude and phase shift that the transmitting field acquires from the sample. From Eq. (2), the Fourier transforms of the autocorrelation functions are given by
From Eq. (3), the power transmission, , and phase shift, , can be retrieved as
Finally, the complex refractive index of the sample with thickness L can be obtained from and as
Figure 5 shows our measurement result obtained with a 390-μm-thick polyethylene (PE) film. Figure 5(a) shows three THz autocorrelations (black line), (red line), and (blue line). The corresponding spectra and transmission curve are obtained from Eqs. (3) and (4) and plotted in Figs. 5(b) and 5(c). According to Fig. 5(c), the sample has ∼50% transmission at 23–40 THz and exhibits a spectral dip at 23 THz. The dip is caused by strong THz absorption by C–H bending vibration, also shown in the expected spectrum (green dotted line). Figure 5(d) shows the phase shift extracted from Eq. (4). Finally, the refractive index, , and absorption coefficient, , are obtained from Eq. (5) and plotted in Fig. 5(e).
In conclusion, we have demonstrated a simple single-shot FTIR spectrometer that combines a modified Mach–Zehnder interferometer with a microbolometer FPA. This can capture a THz field autocorrelation, equivalent to power spectrum, in a single shot. It also allows spectral detection up to 40 THz, more than ten times higher than the typical EO-based single-shot methods.8–14 Also, contrary to conventional FTIR spectrometers utilizing fast scanning, our setup has no moving parts and can characterize ultrafast THz sources as well. Thus, our diagnostic is best suited to characterize ultrafast THz sources that emit high frequency radiation at >10 THz, operate at low repetition rates, or do not provide any synchronous optical light for EO characterization. Even at <10 THz, where our spectrometer has shown a poor response, our interferometric design can be still used with a THz microbolometer that is more sensitive at low THz frequencies.25–27
This work was supported by the Air Force Office of Scientific Research (No. FA9550-16-1-0163) and the Office of Naval Research (No. N00014-17-1-2705). The authors also thank Y. J. Yoo for his initial work on microbolometers.
The data that support the findings of this study are available from the corresponding author upon reasonable request.