Relativistic Maxwell-Bloch equations are derived showing that radiating system response and coherence between emitters are preserved across reference frames, with timescales and intensity transforming as expected relativistically.
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Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.
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Relativistic Maxwell-Bloch Equations with Applications to Astrophysics
Relativistic Maxwell-Bloch equations are derived showing that radiating system response and coherence between emitters are preserved across reference frames, with timescales and intensity transforming as expected relativistically.