Using logarithmically corrected Barrow entropy on a known EMS black hole, the paper claims remnant formation and phase transitions, but the analysis uses the Schwarzschild area rather than the solution's actual horizon area.
Event horizon telescope imaging of the archetypal blazar 3c 279 at an extreme 20 microarcsecond resolution,
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Einstein Maxwell Scalar Black Hole: Thermodynamic Properties with Logarithmic Barrow Entropy
Using logarithmically corrected Barrow entropy on a known EMS black hole, the paper claims remnant formation and phase transitions, but the analysis uses the Schwarzschild area rather than the solution's actual horizon area.