Compact Metasurface Terahertz Spectrometer
W. Ji (TU Delft - ImPhys/Adam group)
Jin Chang (TU Delft - QN/Groeblacher Lab)
Behnam Mirzaei (TU Delft - ImPhys/Optics)
M.L. Ridder (SRON–Netherlands Institute for Space Research)
W. Jellema (SRON–Netherlands Institute for Space Research)
T. Y. Kao (LongWave Photonics LLC)
Alan Lee (LongWave Photonics LLC)
JR Gao (TU Delft - ImPhys/Adam group, SRON–Netherlands Institute for Space Research)
Paul Urbach (TU Delft - ImPhys/Adam group)
Aurèle L.C. Adam (TU Delft - ImPhys/Adam group)
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Abstract
The terahertz frequency region of the electromagnetic spectrum is crucial for understanding the formation and evolution of galaxies and stars throughout the universe's history, as well as the process of planet formation. Detecting the unique spectral signatures of molecules and atoms requires terahertz spectrometers, which must be operated in space observatories due to water vapor absorption in the Earth's atmosphere. However, current terahertz spectrometers face challenges such as low resolution, limited bandwidth, large volume, and complexity. In this paper, the issues of size and weight are addressed by demonstrating a concept for a centimeter-sized, low-weight terahertz spectrometer using a metasurface. The design of the metasurface spectrometer is first discussed for the 1.85 to 2.4 THz range, followed by its fabrication. Next, an array of quantum cascade lasers operating at slightly different frequencies around 2.1 THz is utilized to characterize the spectrometer. Finally, a spectrum inversion method is applied to analyze the measured data, confirming a resolution R (λ/Δλ) of at least 273. This concept can be extended to other application areas, such as planetary observations and various wavelengths in the far-infrared (FIR) and near-infrared (NIR) ranges.