In modified gravity, dynamical Schwarzschild black holes under scalar waves exhibit non-thermal particle creation while preserving the generalized second law and forming stable zero-temperature remnants at the extremal bound.
Roshan, Test of Birkhoff’s theorem in Scalar-Tensor- Vector Gravity, Phys
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Dynamical Black Hole Thermodynamics in Modified Gravity
In modified gravity, dynamical Schwarzschild black holes under scalar waves exhibit non-thermal particle creation while preserving the generalized second law and forming stable zero-temperature remnants at the extremal bound.