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

X. Z. Wu1...2,*, Y. R. Shou2, Z. B. Guo1, H. G. Lu1, J. X. Liu1, D. Wu1, Z. Gong3, and X. Q. Yan14 |Show fewer author(s)
Author Affiliations
  • 1State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing 100871, China
  • 2Center for Relativistic Laser Science, Institute for Basic Science, Gwangju 61005, Republic of Korea
  • 3Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, Heidelberg 69117, Germany
  • 4Collaborative Innovation Center of Extreme Optics, Shanxi University, Shanxi 030006, China
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    Figures & Tables(7)
    Dispersion relation for the case g = 0.002c2/λ.
    (a) and (b) Time evolution of spatial proton density ln[ñp(k,t)] in the transverse direction. (c) and (d) Transverse momentum distribution of protons ln[np(y, Py)] at t = 25 T. (e) and (f) Corresponding transverse drift distance of protons ln[np(y, δy)] at t = 25 T. (a), (c), and (e) are for a cold target; (b), (d), and (f) are for a warm target.
    (a) and (b) Comparison of growth rates at low and high electron temperature for the LWM k = 1.9k0 and the SWM k = 3.8k0, respectively. (c) Temporal evolution of averaged proton longitudinal momentum P̄x (blue, left axis) within the whole simulation box, electron temperature (black, right black axis), and proton beam energy spread Δɛ/ɛ0 (red, rightmost axis). Solid and dashed lines represent the LET and HET cases, respectively.
    (a) Proton density profile at t = 22 T. (b) Proton phase space (y, Py) distribution at t = 22 T. (c) and (d) Electron energy distributions at t = 15 and 22 T. (e) Time evolution of electron energy spectrum. In this simulation, the target thickness l0 = 0.5λ and the electron density ne = 40nc. Other simulation parameters are the same as in Fig. 2. The initial electron temperature is set as 10 eV.
    (a) Proton density profile at t = 25 T (ne0 = 20nc). The inset shows the transverse electron (green line) and proton (black line) density profiles. (b) Growth of the dominant mode (k = 1.9k0) for electron and protons. The inset shows the Fourier analysis of electron mode growth. (c) Time evolution of transverse electron density fluctuation (ne − ne0). (d) and (e) The same as (a) and (b) but for the case ne0 = 80nc. (f) Ratio of the growth rate from simulations and that predicted by RTI theory (red line) and LS termination time (blue line) vs electron density. The dominant mode wavenumbers are 1.9k0, 1.4k0, 1.1k0, and 1.4k0, respectively.
    (a) Temporal evolution of proton average longitudinal momentum P̄x within the whole simulation box for the cases ne0 = 20nc, 40nc, 60nc, and 80nc. The dashed lines show the accelerations in the LS phase, which are 0.012c2/λ, 0.006c2/λ, 0.004c2/λ, and 0.003c2/λ. (b) Proton energy spectra at t = 50 T from 2D simulations with ne = 80nc (blue), 60nc (green), 40nc (orange), and 20nc (red). The inset shows the time evolution of the proton cutoff energy for the case ne = 20nc.
    (a) Dominant frequency of electron density modulation ωm and (b) LS acceleration termination time τLS obtained from a series of 2D PIC simulations. The laser intensity a0 and the areal density σ = ne0l0 are varied. For each laser intensity case, the areal density is increased from σop to 4σop.
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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

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    Paper Information

    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)

    DOI:10.1063/5.0130513

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