Tiny black holes as dark matter express

Original: "Asteroid-mass Primordial Black Holes as Dark Matter from Supersymmetry"
· Andrea Boccia, Marco Chianese
arXiv:2604.26005 · 2026-04-28 · CC BY 4.0 · 1 min
Hypothetical heavy particles in the early Universe helped give birth to asteroid-mass black holes.

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After the Big Bang, the Universe resembled a tightly inflated balloon: pressure prevented matter from clumping together. But hypothetical superheavy particles — sort of ‘heavyweights’ of the microcosm — momentarily made the balloon less stiff. Matter easily clumped, giving birth to black holes with masses from a billion to a billion billion tons. The size of an atomic nucleus, they emit no light, yet their collective gravity governs the motion of stars and galaxies. Calculations show: if such holes make up all dark matter, everything matches observations. The usual model gives too few holes and has been rejected. An unexpected twist: these same tiny ones could have become the seeds of supermassive black holes at the centers of galaxies.

An asteroid-mass black hole is microscopic: passing through Earth, it would leave only a thin tunnel and cause weak tremors. The chance of such an event is extremely small.

Scientists
Stephen HawkingJacob BekensteinVera RubinFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
early universe black holes supermassive black hole asymmetric dark matter dark star beyond standard model particle searches quasistar nuclear reaction mass gap no-hair theorem supersymmetry neutron star mass limit matter antimatter asymmetry schwarzschild metric cosmic string gravastar planetesimal formation gravitational atom event horizon stability hawking radiation mechanism particle creation critical collapse