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.
2025 [arXiv:2505.08737] Paczy´nsky B., Wiita P
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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.