We investigate static and dynamical spherically symmetric black hole solutions within the gravity from entropy (GfE) framework. We derive and solve the modified vacuum field equations for a static, spherically symmetric spacetime, revealing that the classical Schwarzschild geometry receives perturbative corrections scaling as $r^{-4}$. We establish that the GfE framework is consistent with current strong-field astrophysical observations. Higher-order geometric stresses inherent to the GfE vacuum drive a consistent mass-evolution profile. In the limit of large black hole mass, the theory predicts a constant background evaporation rate $-\beta /24$, suggesting an inherent “entropic leakage” of the vacuum. At intermediate scales, the framework replicates the standard Hawking radiation mass-loss law as $\dot{M}\propto M^{-2}$ through a purely classical response of the modified background.

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• Alternative gravity theories
• Quantum aspects of black holes
• Quantum gravity