A high-flux and high-efficiency setup for magneto-infrared spectroscopy

  • Zeping Shi
  • , Wenbin Wu
  • , Zhiwei Zhang
  • , Yuhan Du*
  • , Chenyao Xu
  • , Guangyi Wang
  • , Mingsen Zhou
  • , Congming Hao
  • , Xianghao Meng
  • , Xiangyu Jiang
  • , Chunhui Pan
  • , Wei Lu
  • , Hao Shen
  • , Haifeng Pan
  • , Zhenrong Sun
  • , Junhao Chu
  • , Xiang Yuan*
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We report the design and implementation of a high-flux, high-efficiency magneto-infrared spectroscopy system optimized for broadband measurements in high magnetic fields, which requires a high signal-to-noise ratio. The setup integrates a Fourier transform infrared spectrometer, a 12 T cryogen-free superconducting magnet, precision-polished and gold-plated light tubes, custom-designed reflective focusing modules for Faraday and Voigt geometries, and an external multi-detector chamber with motorized selection. Optical throughput is maximized by reducing light tube loss from 65.5% to 22.0% m−1 via abrasive flow and mechanical polishing followed by gold electroplating and by adopting a single-on-axis parabolic-mirror Faraday module that increases the effective numerical aperture from 0.14 to 0.36, enhancing collection efficiency by nearly an order of magnitude. An eight-position motorized sample stage and fully automated control over magnetic field, temperature, optical path, and detector choice enable high-throughput measurements without repeated warm-ups. The optimized configuration achieves a root-mean-square noise level of 0.0061% in a 2-min integration for a 40% reflectivity sample, corresponding to a signal-to-noise ratio exceeding 1.6 × 104. System capabilities are demonstrated by resolving weak replica bands in EuCd2As2 and high-index Landau level transitions in LaAlSi with amplitudes as low as 0.06%.

Original languageEnglish
Article number113902
JournalReview of Scientific Instruments
Volume96
Issue number11
DOIs
StatePublished - 1 Nov 2025

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