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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For isotropic cosmologies in the Gravity from Entropy theory, spacetimes carry k-temperatures and k-pressures satisfying a first law, and Friedmann universes have non-decreasing total entropy.
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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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Thermodynamics of the Gravity from Entropy theory
For isotropic cosmologies in the Gravity from Entropy theory, spacetimes carry k-temperatures and k-pressures satisfying a first law, and Friedmann universes have non-decreasing total entropy.