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Black Holes: Absolute Rigidity ⚡ экспресс

Original: "No Love for black holes: tightest constraints on tidal Love numbers of black holes from GW250114"
arXiv:2512.01918 · 2025-12-01 · CC BY 4.0 · ⏱ 1 min · General Relativity High Energy
Gravitational waves from the latest merger prove that black holes don't deform one bit.
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Black holes turn out to be perfectly rigid: a new record-breaking gravitational wave signal shows that they resist tidal stretching. This rules out some theories of 'fuzzy' quantum holes and boson stars.

🎯 If a black hole the size of a soccer ball were subjected to tidal forces, the allowable deformation of its horizon would be less than the thickness of a proton.

\tilde{\Lambda} < 34.8
Dimensionless parameter of tidal rigidity: the closer to zero, the harder it is to deform an object.
Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
gravitational waves black hole spacetime curvature
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsequivalence principleno-hair theorem
Original: arXiv:2512.01918 · CC BY 4.0 · bridge42worlds