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gr-qc2026

Thermodynamic-Geometric Phase Transition and Gravitational-Wave Quasinormal Modes of Schwarzschild Black Holes in Gravity: An RVB-Residue Approach

Wen-Xiang Chen

We construct a residue-based framework connecting the thermodynamic geometry of a Schwarzschild-type black hole in gravity with its gravitational-wave quasinormal-mode spect…