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 Ringdowns
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In an unstable Q-ball hairy black hole, the early growth of the weakly responding scalar component is dominated by a second-order QNM rather than its linear response.
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.
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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.