The relativistic flying parabolic mirror can provide a higher laser intensity than the intensity a current laser system can reach via the optical-focusing scheme. A weakly relativistic laser intensity (1.8 × × 10 ¹⁷ 17 W/cm ² 2 , η = 0.29 η = 0.29 ) can be intensified up to a super-strong intensity of >1× > 1 × 10 ²⁷ 27 W/cm ² 2 ( η ≈ 2.2 × 10⁴ η ≈ 2.2 × 10 4 ) by the relativistic flying mirror. Such a super-strong field can be applied to study the strong-field quantum electrodynamics in perturbative and non-perturbative regimes. In this review, the analytic derivations on the field strength and distribution obtained by the ideal relativistic flying parabolic mirror have been shown under the 4 π π -spherical-focusing approach. The quantum non-linearity parameter is calculated when such a super-strong field collides with the high-energy γ γ -photons. The peak quantum non-linearity parameter reaches above 1600 when the 1-GeV γ γ -photon collides with a super-strong laser field reflected and focused by the relativistic flying mirror driven by a 10 PW laser pulse.
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Jeong et al. (2024) studied this question.
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