The Birth of Black Holes from Cosmic Ripples ✛ ✎ ✦

Original: "Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls"

· Utkarsh Kumar, Anish Ghoshal

arXiv:2605.15197v1 · 2026-05-14 · arXiv non-exclusive · independent analysis · 1 min

Cosmology General Relativity HEP Phenomenology HEP Theory

In the early Universe, tiny black holes could have formed from gravitational ripples, like whirlpools from waves.

Immediately after the Big Bang, the Universe resembled a seething ocean. As it cooled, it changed phase: like a liquid turning into vapor, but on a cosmic scale. Giant bubbles of the new phase collided, shaking the fabric of spacetime — generating gravitational waves. Overlapping, these waves compressed matter to the point of birthing black holes — like whirlpools from converging waves.

Such holes turn out tiny: with the mass of a mountain squeezed into the size of an atomic nucleus. According to Stephen Hawking, they evaporate, but many have survived to this day. Modern calculations suggest they could make up all the dark matter, whose existence was suspected by Vera Rubin. The irony is that invisible points, each smaller than an atom, together weigh five times more than all visible matter. The waves themselves didn’t vanish: due to the expansion of the Universe, they have been stretched into a low hum. Future detectors, inspired by the work of Rainer Weiss, are tuned to catch this ancient whisper.

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A primordial black hole with the mass of an asteroid is comparable in size to an atomic nucleus, yet weighs as much as an entire mountain.

Tiny black holes as gateways to other worlds — a recurring image in Lovecraft, for instance in 'The Shadow Out of Time'.

M_{\rm PBH} \approx 10^{-6} M_{\rm eq} \left(\frac{T_{\rm eq}}{T_\star}\right)^2

Here M_eq ≈ 3×10¹⁷ M⊙ is the horizon mass at matter-radiation equality, T_eq ≈ 0.8 eV is the temperature at that epoch, and T_⋆ is the phase transition temperature. The formula shows how the hole's mass decreases as the transition temperature rises.

f_{\rm PBH} \propto T_\star

Numerical simulations confirm a direct proportionality between the abundance of primordial black holes and the phase transition temperature, simplifying the connection to observable parameters and making the model's predictions robust.

Scientists

Stephen Hawking Jacob Bekenstein Vera Rubin Henri Poincaré Fritz Zwicky Karl Schwarzschild

Concepts

primordial black hole early universe black holes primordial gravitational waves quantum cosmological inhomogeneities bubble collision gravitational wave background domain walls particle creation first stars nucleosynthesis cosmic string early dark energy tidal disruption event first stars gap fundamental tone Hawking radiation perturbation spectrum inner horizon density fluctuation overtones

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The Birth of Black Holes from Cosmic Ripples ✛ ✎ ✦