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Hawking's Area Law: How Black Holes Test Quantum Gravity ⚡ экспресс

Original: "Hawking area law in quantum gravity"
· Gianluca Calcagni
arXiv:2604.18669 · 2026-04-20 · CC BY · ⏱ 1 min · General Relativity HEP Theory
Black hole collisions detected by LIGO are weeding out many quantum gravity theories.
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Black hole collisions not only produce gravitational waves but also serve as a rigorous test for the very fabric of the cosmos. Fresh LIGO data is forcing quantum gravity theories to play by a simple rule: the total event horizon area cannot decrease – and this cuts out many complex constructs.

🎯 If the horizon area could shrink, you could endlessly extract energy from a black hole – but the universe's design forbids it.

S = \frac{A}{4}
S is the black hole's entropy, A is the area of its event horizon
Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole gravitational waves entropy spacetime curvature
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2604.18669 · CC BY · bridge42worlds