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Preprint | PUBDB-2025-01264 |
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2025
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Please use a persistent id in citations: doi:10.3204/PUBDB-2025-01264
Report No.: arXiv:2411.07925
Abstract: We investigate the external reverse shock (RS) region of relativistic jets as the origin of X-ray afterglows of jetted tidal disruption events (TDEs) that exhibit luminous jets accompanied by fast-declining nonthermal X-ray emissions. We model the dynamics of jet propagating within an external density medium, accounting for continuous energy injection driven by accretion activities. We compute the time-dependent synchrotron and inverse Compton emissions from the RS region. Our analysis demonstrates that the RS scenario can potentially explain the X-ray light curves and spectra of four jetted TDEs, namely, AT 2022cmc, Swift J1644, Swift J2058, and Swift J1112. Notably, the rapid steepening of the late-stage X-ray light curves can be attributed jointly to the jet break and cessation of the central engine as the accretion rate drops below the Eddington limit. Using parameters obtained from X-ray data fitting, we also discuss the prospects for γ-ray and neutrino detection.
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Journal Article
Revisiting X-ray Afterglows of Jetted Tidal Disruption Events with the External Reverse Shock
The astrophysical journal / Part 1 982(2), 196 (2025) [10.3847/1538-4357/adbbde]
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