A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
Nonlinearities in Black Hole Ring- downs.Phys
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The early growth of the weakly responding scalar component in an unstable Q-ball hairy black hole is dominated by a second-order QNM sourced by the linear unstable mode, even while evolution remains perturbative.
The r^{-3} curvature decay is a universal threshold that makes zero part of the essential spectrum of the linearized coupled Einstein-Maxwell operator via delocalized modes, unifying the infrared behavior of spin-1, spin-2, and mixed fields and linking it to memory effects.
citing papers explorer
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GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
A new gravitational wave event reveals a binary black hole merger with total mass 190-265 solar masses, indicating black holes can form via gravitational-wave driven mergers beyond standard stellar channels.
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Early-Time Nonlinear Growth in an Unstable Q-Ball Hairy Black Hole
The early growth of the weakly responding scalar component in an unstable Q-ball hairy black hole is dominated by a second-order QNM sourced by the linear unstable mode, even while evolution remains perturbative.
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Infrared Universality: The $r^{-3}$ Spectral Threshold for Coupled Gravitational and Electromagnetic Fields
The r^{-3} curvature decay is a universal threshold that makes zero part of the essential spectrum of the linearized coupled Einstein-Maxwell operator via delocalized modes, unifying the infrared behavior of spin-1, spin-2, and mixed fields and linking it to memory effects.