The Jelly Universe: Why Black Holes Got Heavier ✛ ✎ ✦

Original: "Primordial black hole formation in bulk-viscous cosmology"
arXiv:2606.26532 · 2026-06-25 · arXiv non-exclusive · independent analysis · 1 min
The viscosity of the early Universe forces clumps to be denser to birth a black hole, and it ends up more massive.

Right after the Big Bang, the cosmos resembled jelly — hot, super-dense, and viscous. Tiny density fluctuations, blown up by inflation, could have collapsed under their own gravity into black holes. Previously, the medium was thought to be ideal, free of friction. New computer simulations factoring in viscosity revealed: the thicker the “jelly,” the denser a clump must be for collapse — even weak viscosity demands 7% more density. The irony is that viscosity usually hinders flow, but here it creates a barrier that gravity must overcome.

This reshapes tests of the hypothesis that dark matter, the invisible scaffolding of galaxies, is made of primordial black holes. With viscosity, holes are born rarer and more massive, which aligns better with light bending from distant stars. This approach helps refine how the expansion of the Universe unfolded.

The idea of primordial black holes was proposed back in the 1970s by Stephen Hawking, but only viscous modeling brings precision.

The viscosity paradox: it usually slows things down, but in the early Universe it became a barrier that gravity had to overcome with greater force, like squeezing jelly into a point.

w_{\text{eff}} = w - \epsilon \sqrt{24\pi}
Viscosity lowers the effective pressure, making the cosmic medium simultaneously softer and 'stickier'.
M_{\text{PBH}} / M_H = k |\mu - \mu_c|^\gamma
Universal mass scaling near the collapse threshold. Viscosity increases the prefactor constant k, barely changing the critical exponent.
Scientists
Stephen HawkingJacob BekensteinJames JeansFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
primordial black hole early universe black holes critical collapse bubble collision Bekenstein-Hawking entropy particle creation barrow entropy mass inflation cosmic bubble nucleation charge to mass ratio cosmic structure formation primordial gravitational waves dark matter core formation quantum cosmological inhomogeneities horizon area quasistar hawking area law Chandrasekhar limit dark matter subhalo structure growth