There is a physical limit to how fast a black hole can grow
Astrophysical limits, such as the Eddington limit and associated radiative feedback, impose constraints on the maximum rate at which black holes can continuously accrete and grow.
The claim that there is a physical limit to how fast a black hole can grow is supported by standard astrophysical concepts like the Eddington luminosity limit, which governs radiation pressure and accretion dynamics. Retrieved papers such as [3] and [9] discuss super-Eddington limits, accretion rates, and how feedback mechanisms restrict further growth, providing adequate support without significant contradictory evidence.
Stratified wind from a super-Eddington X-ray binary is slower than expected.. 2025. https://doi.org/10.1038/s41586-025-09495-w
Paper [3] discusses Eddington limits and radiation pressure on black hole accretion, establishing physical boundaries on accretion rates.
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Warren Massonneau. Massive black holes beyond the Eddington limit. https://doi.org/10.70675/c064e5f3z341az4b8bzb8d5z85ad3e5920b9
Paper [9] examines super-Eddington accretion and explains that rapid feedback mechanisms eventually restrict further black hole growth.
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