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arxiv: 2509.06230 · v3 · submitted 2025-09-07 · ⚛️ physics.plasm-ph · astro-ph.HE

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Complete reflection of nonlinear electromagnetic waves in underdense pair plasmas enabled by dynamically formed Bragg-like structures

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classification ⚛️ physics.plasm-ph astro-ph.HE
keywords plasmasreflectionpairwavesbragg-likecompleteelectromagneticinitially
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In contrast to relativistically induced transparency in electron--ion plasmas, where nonlinear electromagnetic waves render initially opaque plasmas transparent, we show using kinetic simulations that such waves can instead make initially transparent pair plasmas fully reflective. The difference is mass symmetry, which eliminates charge-separation electric fields. As the wave compresses the pair plasma, weak reflection seeds density spikes that form a moving Bragg-like grating. Enhanced reflection enables a transition to a regime where the plasma--vacuum interface sustains complete reflection.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Interaction of Strong Electromagnetic Waves with Unmagnetized Pair Plasmas

    physics.plasm-ph 2026-04 unverdicted novelty 7.0

    Strong EM waves in pair plasmas are governed by nonlinearity parameter ε_p, producing attenuation over ε_p^{-2/3} wavelengths when small and shock formation when large.

  2. Powerful parametric instability of Alfven waves in astrophysical pair plasma

    astro-ph.HE 2026-05 unverdicted novelty 6.0

    Nonlinear Alfven waves with k near k0 in highly magnetized pair plasmas experience strong modulational instability that drives density fluctuations and generates high-frequency modes.