4.6 Article

Tunable single-mode laser on thin film lithium niobate

期刊

OPTICS LETTERS
卷 46, 期 21, 页码 5505-5508

出版社

Optica Publishing Group
DOI: 10.1364/OL.441167

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资金

  1. National Key Research and Development Program of China [2017YFA0303701, 2019YFB2203501]
  2. National Natural Science Foundation of China [11734011, 12134009, 91950107]
  3. ShanghaiMunicipal Science and Technology Major Project [2019SHZDZX01-ZX06]
  4. Shanghai Jiao Tong University [21X010200828]

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The erbium-doped lithium niobate on insulator (LNOI) laser is crucial for complete photonic integrated circuits (PICs). In this study, an integrated tunable whispering gallery single-mode laser (WGSML) was achieved by utilizing a coupled microdisk and microring on LNOI. The output power of the WGSML can be increased by adjusting the temperature, and the central wavelength can be altered within a certain range. Additionally, different wavelengths of WGSMLs were obtained by changing the coupling gap width between the microdisk and microring, showing promise for future research in obtaining more precise adjustable WGSMLs using the electro-optic effect of LNOI.
The erbium-doped lithium niobate on insulator (LNOI) laser plays an important role in the complete photonic integrated circuits (PICs). Here, we demonstrate an integrated tunable whispering gallery single-mode laser (WGSML) by making use of a coupled microdisk and microring on LNOI. A 974 nm single-mode pump light can have an excellent resonance in the designed microdisk, which is beneficial to the whispering gallery mode (WGM) laser generation. The WGSML at 1560.40 nm with a maximum 31.4 dB side mode suppression ratio (SMSR) has been achieved. By regulating the temperature, the output power of the WGSML increases, and the central wavelength can be changed from 1560.30 to 1560.40 nm. Furthermore, 1560.60 and 1565.00 nm WGSMLs have been achieved by changing the coupling gap width between the microdisk and microring. We can also use the electro-optic effect of LNOI to obtain more accurate adjustable WGSMLs in further research. (C) 2021 Optical Society of America

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