A synchrotron forward-shock model with confined broken-power-law CSM explains FBOT radio diversity via shock transition out of the dense shell, yielding trans-relativistic velocities of 0.1-0.5c and high but brief mass-loss rates of 10^{-4} to 10^{-3} solar masses per year.
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Luminous fast blue optical transients are powered by delayed conversion of massive neutron stars into highly magnetized hybrid stars in the Quark-Nova model, with flares from fragmenting ejecta and self-consistent multi-wavelength emissions.
citing papers explorer
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Radio Emission from Fast Blue Optical Transients Powered by Trans-relativistic Shocks in Confined Circumstellar Material
A synchrotron forward-shock model with confined broken-power-law CSM explains FBOT radio diversity via shock transition out of the dense shell, yielding trans-relativistic velocities of 0.1-0.5c and high but brief mass-loss rates of 10^{-4} to 10^{-3} solar masses per year.
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Optical Flares in the Luminous Fast Blue Optical Transient AT2022tsd ("Tasmanian Devil")
Luminous fast blue optical transients are powered by delayed conversion of massive neutron stars into highly magnetized hybrid stars in the Quark-Nova model, with flares from fragmenting ejecta and self-consistent multi-wavelength emissions.