Impact of Propagation Effects on the Spectro-temporal Properties of Fast Radio Bursts

Abstract We present a mathematical analysis of propagation-induced distortions in the spectro-temporal properties of fast radio bursts (FRBs). Within the triggered relativistic dynamical model, we derive a centroid-based formulation of the sub-burst slope law, which describes an inverse relation between the sub-burst frequency drift rate and the intrinsic temporal width t w . We extend this framework to include two frequency-dependent propagation effects: (i) multipath scattering, characterized by a pulse-broadening timescale τ sc ∝ ν −4 , and (ii) residual dispersion, parameterized by ΔDM ∝ ν −2 . Our analysis shows that scattered bursts exhibit the same qualitative inverse slope–duration relation but differ quantitatively through a larger scaling coefficient when τ sc &gt; t w . Residual DM errors act asymmetrically: under-dedispersion flattens the sub-burst slope, whereas over-dedispersion produces a nonlinear increase and eventual sign change. When both effects are present, scattering counterbalances the steepening induced by over-dedispersion and augments the flattening from under-dedispersion, yielding characteristically distorted curves. We repeat analysis for ultrashort duration bursts (ultra-FRBs) with t w = 50 μ s at 1 GHz and find them to be far more sensitive to propagation errors. Deviations become measurable for <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mfenced close="∣" open="∣"> <mml:mrow> <mml:mi mathvariant="normal">Δ</mml:mi> <mml:mi mathvariant="normal">DM</mml:mi> </mml:mrow> </mml:mfenced> <mml:mo>∼</mml:mo> <mml:mn>0.05</mml:mn> </mml:math> pc cm −3 and for τ sc ∼ 0.1 ms at 1 GHz, levels that have negligible impact on the standard-width sub-bursts. Our analysis provides practical diagnostics to disentangle propagation effects from observed spectro-temporal properties, thereby recovering intrinsic correlations among FRB parameters.