In blazars, the location where magnetic reconnection dissipates jet energy determines the observed spectrum and neutrino output, bridging BL Lacs and FSRQs in a single model.
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The role of dissipation distance on reconnection-driven multi-messenger signals from blazar jets
In blazars, the location where magnetic reconnection dissipates jet energy determines the observed spectrum and neutrino output, bridging BL Lacs and FSRQs in a single model.