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.
Geometrothermodynamics of 3d regular black holes,
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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.