Near Infrared to Visible Upconversion Polarization Imaging Enabled by Cs2NaScCl6: Er3+ Composite Film

Authors

  • Henan Yang School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China. Author
  • Ye Wang School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China. Author
  • Cheng Ding School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China. Author
  • Jie Cao School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China. Author
  • Bingkun Chen School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China. Author
  • Siyang Chen 2School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China. Author
  • Qun Hao School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China. Author
  • Kun Zheng Yangtze Delta Region Academy of Beijing Institute of Technology, Jiaxing 314019, Zhejiang, China. Author

DOI:

https://doi.org/10.47363/JJCMR/2026(6)206

Keywords:

Lead-free Double Perovskite, Cs2NaScCl6: Er3+, Upconversion Emission, Composite Film, Near Infrared Polarization Imaging

Abstract

Herein, TLCP and TRCP denote the transmitted light intensities of
the UCPL film under illumination with LCP and RCP, respectively.
CD refers to the differential absorption between LCP and RCP. A
positive value of ΔT indicates that the film induces a left-handed
effect, whereas a negative value signifies a right-handed effect.
The same principle applies to the CD value. Typically, the CD
signal of strongly chiral materials reaches a magnitude of 1000
mdeg. As shown in Figure S9(B), the test results of the UCPL film
in this study exhibit almost no spectral fluctuations at this scale.
When the scale is magnified to that presented in Figure S9(C),
as evidenced by the curves, a sharp increase in the left-handed
effect emerges at approximately 390 nm and 540 nm; however,
the magnitude of this effect is extremely small, remaining below
4 mdeg in all cases. This can be identified as baseline noise,
confirming that the UCPL film exhibits no chiral characteristics.

Author Biographies

  • Henan Yang, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China.

    Henan Yang, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China

  • Ye Wang, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China.

    Ye Wang, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China

  • Cheng Ding, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China.

    Cheng Ding, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China

  • Jie Cao, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China.

    Jie Cao, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China

  • Bingkun Chen, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China.

    Bingkun Chen, School of Optics and Photonics, Beijing Institute of Technology, Beijing 100081, China

  • Siyang Chen, 2School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China.

    Siyang Chen, School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China

  • Qun Hao, School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China.

    Qun Hao, School of Electro - Optical Engineering, Changchun University of Science and Technology, Changchun 130022, China

  • Kun Zheng, Yangtze Delta Region Academy of Beijing Institute of Technology, Jiaxing 314019, Zhejiang, China.

    Kun Zheng, Yangtze Delta Region Academy of Beijing Institute of Technology, Jiaxing 314019, Zhejiang, China

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Published

2022-06-09