Abstract Cavitation luminescence is light emission from gases that are compressed to high temperature and high pressure inside a bubble or group of bubbles. The numerical simulation in this study indicates that if the temperature and pressure inside a bubble are not high enough, then dim and spectral line emission dominates. However, if the temperature and pressure inside the bubble are very high, then the light is bright and a continuum spectrum will be generated. Calculations of the spectrum using modified equations of bubble motion can simulate the spectral profile well. However, pulse width calculations using these equations only partly agree with the experimental results.
Near-zero thermal expansion in β-CuZnV2O7 in a large temperature range Yaguang Hao(郝亚光), Hengli Xie(谢恒立), Gaojie Zeng(曾高杰), Huanli Yuan(袁焕丽), Yangming Hu(胡杨明), Juan Guo(郭娟), Qilong Gao(高其龙), Mingju Chao(晁明举), Xiao Ren(任霄), and Er-Jun Liang(梁二军). Chin. Phys. B, 2022, 31(4): 046502.
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