This paper derives quantitative correction factors for traditional SSA minimum energy estimates to account for inhomogeneity and non-spherical geometry in emitting regions.
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3D hydro simulations show that TDE outflow interactions with a broken power-law CNM can reproduce the range of observed radio light curves via early flares inside the Bondi radius and possible late rebrightenings outside it.
Faint radio emission in TDE2025aarm implies a collimated outflow from unbound debris with solid angle ≲0.1 sr, while X-rays can arise from the same shock via synchrotron or inverse-Compton scattering.
Late-time radio rebrightening in SN 2012ap is consistent with either progenitor mass-loss variation producing a density enhancement or an off-axis energetic jet viewed at large angle, potentially reclassifying it as GRB-like rather than weakly engine-driven.
The paper provides observing strategies, detection forecasts, and predictions for using SKA and VLBI to study radio emission from tidal disruption events around supermassive black holes.
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On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm
Faint radio emission in TDE2025aarm implies a collimated outflow from unbound debris with solid angle ≲0.1 sr, while X-rays can arise from the same shock via synchrotron or inverse-Compton scattering.