A fixed point for black hole distributions
Jos\'e T. G\'alvez Ghersi, Leo C. Stein

TL;DR
This paper demonstrates that binary black hole mergers lead to a universal fixed point distribution of spin and mass loss, revealing an attractor behavior that is independent of initial conditions and has implications for entropy production in the universe.
Contribution
It introduces a Gedankenexperiment showing that non-linear black hole mergers produce an attractor in distribution space, independent of initial states, with implications for entropy and thermodynamics.
Findings
Distribution converges to a fixed point after few generations
Fixed point features are independent of initial distribution
Entropy production rate per merger converges to a constant
Abstract
Understanding distributions of black holes is crucial to both astrophysics and quantum gravity. Studying astrophysical population statistics has even been suggested as a channel to constrain black hole formation from the quantum vacuum. Here we propose a Gedankenexperiment to show that the non-linear properties of binary mergers (simulated with accurate surrogate models) generate an attractor in the space of distributions. Our results show that the joint distribution of spin magnitude and fractional mass loss evolves to a fixed point, converging in a few generations. The features of this fixed point distribution do not depend on the choice of initial distribution. Since a black hole merger is irreversible it produces entropy - possibly the largest source of entropy in the universe. The fixed-point distributions are neither isothermal nor isentropic, and initially thermodynamic states…
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