How Tiny Black Holes Gain Weight ✛ ✦

Original: "Primordial Black Hole mass growth from neutrinos during radiation era"
· Maël Gonin
arXiv:2607.09285 · 2026-07-10 · CC BY 4.0 · 1 min
Primordial black holes fatten up on ghostly neutrinos and grow rapidly.

Right after the Big Bang, tiny primordial black holes could have been born. Stephen Hawking believed they didn’t grow: the hot plasma around them moved too fast to fall into such a small capture region (the Schwarzschild radius). New research turns this idea on its head. It turns out these holes can satisfy their hunger with neutrinos — ghostly particles that ordinarily pass through matter as if through a void.

Thanks to inflation (an idea from Alan Guth) and the expansion of the universe, at a certain point neutrinos start behaving like prey, falling into the black hole. This allows primordial holes to gain a mass of anywhere from a thousand to a million solar masses. The surprising conclusion: these grown-up holes could turn out to be the very dark matter that holds galaxies together.

Black holes are fishermen, neutrinos are the prey. In the early universe, the ‘pond’ was teeming with food, and the hungriest holes grew fast.

Now the James Webb Space Telescope can glimpse the traces of these feasts in distant galaxies, and gravitational wave detectors (LIGO) can catch the ripples from their mergers. Dark matter may not be so dark after all.

Neutrinos can pierce a light-year of lead without noticing it, but in the searing-hot ‘kitchen’ of the early universe, they become the main course for voracious black holes.

In Carl Sagan’s novel ‘Contact,’ black holes are gateways for travel. Here, they grow by feeding on ghostly particles — and this isn’t science fiction, but the cutting edge of science.

r_s = \frac{2GM}{c^2}
Characteristic size of the event horizon, depending on mass M
\lambda_\nu = \frac{1}{n_\nu \langle\sigma_{\text{weak}}\rangle}
Average distance a neutrino travels without interaction; n_ν is concentration, σ_weak ∝ G_F^2 T^2 is the weak interaction cross-section
Scientists
Stephen HawkingJacob BekensteinAdam RiessSaul PerlmutterBrian Schmidt
Concepts
early universe black holes primordial black hole nuclear reaction mass gap mass inflation primordial nucleosynthesis wave amplification population iii stars hawking radiation mechanism early universe star formation dark ages radiation dominated era stellar evolution first stars nucleosynthesis Penrose process dark star barrow entropy no-hair theorem reheating particle creation accretion disk wind