A residue-based approach in f(Q) gravity claims that thermodynamic Hessian degeneracy in the extended state space produces corresponding shifts in quasinormal-mode frequencies, Lyapunov exponents, damping times, and near-horizon monodromy.
Riemannian geometry in thermodynamic fluctuation theory,
3 Pith papers cite this work. Polarity classification is still indexing.
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An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
Thermodynamic instability and fluctuation analysis of the GMG warped black hole, including exact on-shell angular momentum trajectories and thermodynamic lengths for isentropic/isoenergetic processes.
citing papers explorer
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Thermodynamic-Geometric Phase Transition and Gravitational-Wave Quasinormal Modes of Schwarzschild Black Holes in $f(Q)$ Gravity: An RVB-Residue Approach
A residue-based approach in f(Q) gravity claims that thermodynamic Hessian degeneracy in the extended state space produces corresponding shifts in quasinormal-mode frequencies, Lyapunov exponents, damping times, and near-horizon monodromy.
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Renormalization-group improved Schwarzschild black hole: shadow, ringdown, and strong cosmic censorship
An RG-improved Schwarzschild metric with de Sitter core is studied for shadow radius, scalar/EM/Dirac quasinormal modes via WKB and time-domain methods, SCC compliance at the inner horizon, and a Davies-type thermodynamic phase transition.
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Thermodynamic Stability and Fluctuations of the (2+1)-dimensional GMG Warped Black Hole
Thermodynamic instability and fluctuation analysis of the GMG warped black hole, including exact on-shell angular momentum trajectories and thermodynamic lengths for isentropic/isoenergetic processes.