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Tiny black holes explain galaxy flows and the expansion of the Universe ⚡ экспресс

Original: "More power on large scales"
· Jeremy Mould
arXiv:2601.07106 · 2026-01-12 · CC BY 4.0 · ⏱ 1 min · Cosmology
Tiny black holes born at the Universe's dawn could explain why galaxies move faster and smooth out disagreements in expansion measurements.
Abstract

Perhaps dark matter is not made of elementary particles but of primordial black holes (PBHs). Unlike standard cold dark matter, PBHs were already dense clumps in the radiation era, triggering early gravitational collapse. Simulations show this produces more powerful galactic flows. Moreover, the lightest PBHs (with masses of 10^-20–10^-17 solar masses) gradually evaporate via Hawking radiation, transforming into energy. This dynamically lowers the matter density in the early universe, reducing the sound horizon and helping to resolve the Hubble tension. The universe's dark 'building blocks' do more than just attract—they change over time.

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Dark matter may not be particles but black holes from the Big Bang era. In the early Universe, which was like a swirling batter, they were like heavy lumps—barely moving, they gathered surrounding matter and spun it into the swift galaxy flows astronomers observe today. But there's a twist: the lightest holes, according to Hawking's theory, evaporate, emitting energy. This evaporation gently warms the cosmic 'batter' in its early stages, thereby changing the calculated rate of the Universe's expansion and smoothing out the notorious tension between different measurement methods.

Astonishingly: a hole with the mass of an asteroid compressed to a point smaller than an atomic nucleus. Its slow evaporation could produce a mysterious glow in space.
Simulations showed: accounting for such holes removes the need to tweak other cosmological parameters—an elegant strike on two mysteries at once.

🎯 One such hole weighs as much as an asteroid but is compressed to a point smaller than an atomic nucleus. Its evaporation is so unhurried that over the entire history of the Universe, it would lose only a minuscule fraction of its mass.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
dark matter black hole expansion of the universe big bang
Laws
Friedmann equationsHubble's lawHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equations
Original: arXiv:2601.07106 · CC BY 4.0 · bridge42worlds