In the Gravity from Entropy framework, spherically symmetric black holes acquire r^{-4} corrections to Schwarzschild geometry, with large-mass evaporation at constant rate -β/24 and intermediate-mass loss following the classical Hawking M^{-2} scaling.
In- flation from entropy.arXiv preprint arXiv:2509.23987, 2025
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GfE theory receives a thermodynamic treatment for FRW spacetimes, yielding emergent dynamical dark energy, k-temperatures and k-pressures obeying a first law, and non-decreasing entropy that recovers standard Friedmann cosmology at low energy.
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Spherically symmetric black holes in Gravity from Entropy and spontaneous emission
In the Gravity from Entropy framework, spherically symmetric black holes acquire r^{-4} corrections to Schwarzschild geometry, with large-mass evaporation at constant rate -β/24 and intermediate-mass loss following the classical Hawking M^{-2} scaling.
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The Thermodynamics of the Gravity from Entropy Theory
GfE theory receives a thermodynamic treatment for FRW spacetimes, yielding emergent dynamical dark energy, k-temperatures and k-pressures obeying a first law, and non-decreasing entropy that recovers standard Friedmann cosmology at low energy.