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This work investigates the interconnections between mass, energy, and structural properties within black hole thermodynamics.

May 26, 2026Open Access

Black Hole Thermodynamics. Energy, Time and Structural Closure.

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The article analyzes structural aspects of black hole thermodynamics, highlighting causal links between mass and entropy.

This work investigates the interconnections between mass, energy, and structural properties within black hole thermodynamics.
Analyzes relations among mass, energy, horizon radius, area, temperature, and entropy in black holes.
Examines the implications of the limit M → 0 in terms of Hawking evaporation.
Proposes minimum premises for future microscopic theories of black holes.
Shows that a finite black hole configuration has limited physical distinguishability as M approaches zero.
Demonstrates that Hawking temperature diverges as energy, horizon radius, and entropic capacity tend to zero.
Argues for the necessity of a last admissible horizon state during complete evaporation.

Julián Sánchez Navarro (2026) studied this question.

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