Matter and Radiation at Extremes, Volume. 8, Issue 3, 036902(2023)
Effects of electron heating and surface rippling on Rayleigh–Taylor instability in radiation pressure acceleration
Fig. 2. (a) and (b) Time evolution of spatial proton density
Fig. 3. (a) and (b) Comparison of growth rates at low and high electron temperature for the LWM
Fig. 4. (a) Proton density profile at
Fig. 5. (a) Proton density profile at
Fig. 6. (a) Temporal evolution of proton average longitudinal momentum
Fig. 7. (a) Dominant frequency of electron density modulation
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X. Z. Wu, Y. R. Shou, Z. B. Guo, H. G. Lu, J. X. Liu, D. Wu, Z. Gong, X. Q. Yan. Effects of electron heating and surface rippling on Rayleigh–Taylor instability in radiation pressure acceleration[J]. Matter and Radiation at Extremes, 2023, 8(3): 036902
Category: Radiation and Hydrodynamics
Received: Oct. 12, 2022
Accepted: Mar. 21, 2023
Published Online: Jun. 30, 2023
The Author Email: Wu X. Z. (xz.wu@pku.edu.cn)