• Matter and Radiation at Extremes
  • Vol. 8, Issue 6, 064002 (2023)
Feng Wan1, Chong Lv2, Kun Xue1, Zhen-Ke Dou1, Qian Zhao1, Mamutjan Ababekri1, Wen-Qing Wei1, Zhong-Peng Li1, Yong-Tao Zhao1, and Jian-Xing Li1、a)
Author Affiliations
  • 1Ministry of Education Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Shaanxi Province Key Laboratory of Quantum Information and Quantum Optoelectronic Devices, School of Physics, Xi’an Jiaotong University, Xi’an 710049, China
  • 2Department of Nuclear Physics, China Institute of Atomic Energy, P.O. Box 275(7), Beijing 102413, China
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    DOI: 10.1063/5.0163929 Cite this Article
    Feng Wan, Chong Lv, Kun Xue, Zhen-Ke Dou, Qian Zhao, Mamutjan Ababekri, Wen-Qing Wei, Zhong-Peng Li, Yong-Tao Zhao, Jian-Xing Li. Simulations of spin/polarization-resolved laser–plasma interactions in the nonlinear QED regime[J]. Matter and Radiation at Extremes, 2023, 8(6): 064002 Copy Citation Text show less
    Standard particle-in-cell (PIC) loop with four kernel parts.
    Fig. 1. Standard particle-in-cell (PIC) loop with four kernel parts.
    (a) and (b) Yee grid and position of each field component in 3D and 2D cases, respectively. In (b), the z direction is squeezed.
    Fig. 2. (a) and (b) Yee grid and position of each field component in 3D and 2D cases, respectively. In (b), the z direction is squeezed.
    Leapfrog algorithm for particle pushing and field advancing.
    Fig. 3. Leapfrog algorithm for particle pushing and field advancing.
    q(χ) vs χ.
    Fig. 4. q(χ) vs χ.
    Dynamics of an electron [p0 = (4000, 0, 0)] scattering with an ultraintense linearly polarized laser pulse of Ey=100exp−ϕ−10010π2cosϕ, with ϕ ≡ t + x. Here, Lo., LL., and MLL. denote results calculated from the Lorentz, LL, and modified LL equations, respectively.
    Fig. 5. Dynamics of an electron [p0 = (4000, 0, 0)] scattering with an ultraintense linearly polarized laser pulse of Ey=100expϕ10010π2cosϕ, with ϕt + x. Here, Lo., LL., and MLL. denote results calculated from the Lorentz, LL, and modified LL equations, respectively.
    Spin dynamics of an electron [p0 = (4000, 0, 0), s0 = (1, 0, 0)] scattering with an ultraintense linearly polarized laser pulse of Ey=100exp−ϕ−10010π2cosϕ, with ϕ ≡ t + x. Here, A, B, C, and D denote results calculated using the Lorentz + T-BMT, Lorentz + radiative T-BMT, LL + radiative T-BMT, and MLL + radiative T-BMT equations, respectively.
    Fig. 6. Spin dynamics of an electron [p0 = (4000, 0, 0), s0 = (1, 0, 0)] scattering with an ultraintense linearly polarized laser pulse of Ey=100expϕ10010π2cosϕ, with ϕt + x. Here, A, B, C, and D denote results calculated using the Lorentz + T-BMT, Lorentz + radiative T-BMT, LL + radiative T-BMT, and MLL + radiative T-BMT equations, respectively.
    Flowchart of spin- and polarization-resolved NCS.
    Fig. 7. Flowchart of spin- and polarization-resolved NCS.
    Dynamics of 1000 electrons via stochastic NCS, with the simulation parameters the same as those in Fig. 6. Blue lines are for ten sampled electrons, and black ones are the average value over 1000 sample particles.
    Fig. 8. Dynamics of 1000 electrons via stochastic NCS, with the simulation parameters the same as those in Fig. 6. Blue lines are for ten sampled electrons, and black ones are the average value over 1000 sample particles.
    Dynamics of an electron beam (particle number Ne = 104), with colors denoting the number density in arbitrary units and a logarithmic scale (a.u.); other parameters are the same as those in Fig. 6.
    Fig. 9. Dynamics of an electron beam (particle number Ne = 104), with colors denoting the number density in arbitrary units and a logarithmic scale (a.u.); other parameters are the same as those in Fig. 6.
    (a) Energy spectra of scattered electrons (black curve) and generated photons (red curve). (b) Energy-dependent Stokes parameters ξ̄2 and ξ3̄, i.e., circular and linear polarization with respect to the y and z axes. The simulation parameters are the same as those in Fig. 6.
    Fig. 10. (a) Energy spectra of scattered electrons (black curve) and generated photons (red curve). (b) Energy-dependent Stokes parameters ξ̄2 and ξ3̄, i.e., circular and linear polarization with respect to the y and z axes. The simulation parameters are the same as those in Fig. 6.
    Flowchart of the spin- and polarization-resolved nonlinear Breit–Wheeler (NBW) pair production process.
    Fig. 11. Flowchart of the spin- and polarization-resolved nonlinear Breit–Wheeler (NBW) pair production process.
    (a) Normalized energy spectrum (black solid curve) and energy-resolved longitudinal spin polarization (red solid curve) of positrons. (b) Statistics of the longitudinal spin components of generated positrons. The laser and electron beam parameters are consistent with those in Fig. 9.
    Fig. 12. (a) Normalized energy spectrum (black solid curve) and energy-resolved longitudinal spin polarization (red solid curve) of positrons. (b) Statistics of the longitudinal spin components of generated positrons. The laser and electron beam parameters are consistent with those in Fig. 9.
    Bremsstrahlung of 100 MeV electrons: (a) scattered electron spectra; (b) yield photon spectra. Solid curves represent PIC results and dashed curves Geant4 results. Reproduced with permission from F. Wan et al., Eur. Phys. J. D 71, 236 (2017). Copyright 2017, EDP Sciences, SIF, Springer-Verlag GmbH Germany.
    Fig. 13. Bremsstrahlung of 100 MeV electrons: (a) scattered electron spectra; (b) yield photon spectra. Solid curves represent PIC results and dashed curves Geant4 results. Reproduced with permission from F. Wan et al., Eur. Phys. J. D 71, 236 (2017). Copyright 2017, EDP Sciences, SIF, Springer-Verlag GmbH Germany.
    Bremsstrahlung of 1 GeV electrons: (a) scattered electron spectra; (b) yield photon spectra. Solid curves represent PIC results and dashed curves Geant4 results. Reproduced with permission from F. Wan et al., Eur. Phys. J. D 71, 236 (2017). Copyright 2017, EDP Sciences, SIF, Springer-Verlag GmbH Germany.
    Fig. 14. Bremsstrahlung of 1 GeV electrons: (a) scattered electron spectra; (b) yield photon spectra. Solid curves represent PIC results and dashed curves Geant4 results. Reproduced with permission from F. Wan et al., Eur. Phys. J. D 71, 236 (2017). Copyright 2017, EDP Sciences, SIF, Springer-Verlag GmbH Germany.
    (a) M(χγ) (red and blue solid curves) and the corresponding low-energy-limit constants, with red and blue dash-dotted lines equal to 4 and 7, respectively. (b) Relative error between M(χγ) and the low-energy-limit constant.
    Fig. 15. (a) M(χγ) (red and blue solid curves) and the corresponding low-energy-limit constants, with red and blue dash-dotted lines equal to 4 and 7, respectively. (b) Relative error between M(χγ) and the low-energy-limit constant.
    VB effect of a γ-photon [ɛγ = 1 GeV, ξ = (1, 0, 0)] propagating through (a) static crossed fields with Ey = −Bz = 100 and (b) a laser field (the same as in Fig. 6).
    Fig. 16. VB effect of a γ-photon [ɛγ = 1 GeV, ξ = (1, 0, 0)] propagating through (a) static crossed fields with Ey = −Bz = 100 and (b) a laser field (the same as in Fig. 6).
    Data structure of SLIPs.
    Fig. 17. Data structure of SLIPs.
    Framework of SLIPs.
    Fig. 18. Framework of SLIPs.
    Generation of polarized electrons: (a) number density log_{10}(d2N/dθxdθy) (a.u.); (b) spin polarization Sx.
    Fig. 19. Generation of polarized electrons: (a) number density log_{10}(d2N/xy) (a.u.); (b) spin polarization Sx.
    Generation of LP γ-photons: (a) number density log10(d2N/dθxdθy) (a.u.); (b) linear polarization ξ3.
    Fig. 20. Generation of LP γ-photons: (a) number density log10(d2N/xy) (a.u.); (b) linear polarization ξ3.
    Generation of CP γ-photons with longitudinally polarized electrons: (a) number density log10(d2N/dθxdθy) (a.u.); (b) circular polarization |ξ2|.
    Fig. 21. Generation of CP γ-photons with longitudinally polarized electrons: (a) number density log10(d2N/xy) (a.u.); (b) circular polarization |ξ2|.
    Laser–plasma interaction via 2D simulation: (a)–(c) spatial distributions of Ex, Ey, and Bz, respectively; (d)–(f) number densities (in logrithm) of target electrons, generated NBW positrons, and NCS γ-photons, respectively.
    Fig. 22. Laser–plasma interaction via 2D simulation: (a)–(c) spatial distributions of Ex, Ey, and Bz, respectively; (d)–(f) number densities (in logrithm) of target electrons, generated NBW positrons, and NCS γ-photons, respectively.
    Photons generated by laser–plasma interaction: (a) number density with respect to energy and angle, i.e., log10(dN2/dγγdθ) (a.u.) with γγ≡Eγ/mec2 and θ ≡ py/px; (b) energy- and angle-resolved linear polarization degree ξ̄3; (c) energy-resolved number and polarization distributions; (d) angle-resolved number and polarization distributions.
    Fig. 23. Photons generated by laser–plasma interaction: (a) number density with respect to energy and angle, i.e., log10(dN2/γ) (a.u.) with γγEγ/mec2 and θpy/px; (b) energy- and angle-resolved linear polarization degree ξ̄3; (c) energy-resolved number and polarization distributions; (d) angle-resolved number and polarization distributions.
    Positrons generated by laser–plasma interaction: (a) number density with respect to energy and angle, i.e., dN2/dγ+dθ (a.u.), with γ+ ≡ ɛ+/mec2 and θ ≡ arctan(py/px); (b) energy- and angle-resolved spin component S̄z; (c) normalized angular distribution n(θ) ≡ dN/dθ (a.u.); (d) angular distribution of S̄z (i.e., energy-averaged); (e) normalized energy distribution n(ɛ+) ≡ dN/dɛ+ (a.u.).
    Fig. 24. Positrons generated by laser–plasma interaction: (a) number density with respect to energy and angle, i.e., dN2/+ (a.u.), with γ+ɛ+/mec2 and θ ≡ arctan(py/px); (b) energy- and angle-resolved spin component S̄z; (c) normalized angular distribution n(θ) ≡ dN/(a.u.); (d) angular distribution of S̄z (i.e., energy-averaged); (e) normalized energy distribution n(ɛ+) ≡ dN/+ (a.u.).
    Table 1. VB effect in SLIPs.
    Feng Wan, Chong Lv, Kun Xue, Zhen-Ke Dou, Qian Zhao, Mamutjan Ababekri, Wen-Qing Wei, Zhong-Peng Li, Yong-Tao Zhao, Jian-Xing Li. Simulations of spin/polarization-resolved laser–plasma interactions in the nonlinear QED regime[J]. Matter and Radiation at Extremes, 2023, 8(6): 064002
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