Invisible Black Holes Explain the Expansion of the Universe ✛

Original: "The impact of Hawking radiation from primordial black holes on recombination and the Hubble tension"
· Adam Batten, Jeremy Mould
arXiv:2607.18528v1 · 2026-07-20 · CC BY 4.0 · 2 min
Tiny black holes, evaporating in the early universe, heated the gas and shifted the measurement of cosmic expansion.

The universe cooled like a giant bathtub after a hot start. 400,000 years after the Big Bang, hydrogen was ready to turn neutral — protons were catching electrons. But in this dark water, a tap kept dripping. The drops were primordial black holes — microscopic black holes left over from the universe’s first moments. Their mass is that of a small asteroid, crushed into a point. These holes slowly evaporated through the process discovered by Stephen Hawking (Hawking radiation), adding heat to the gas. Each drop delayed the moment the universe became transparent to the cosmic microwave background — the ancient light reaching us from that era.

This lag helps solve the mystery of the expansion of the universe rate. Two precision methods give different numbers. Adam Riess and colleagues, observing stars in nearby galaxies, get a speed of about 73 km/s per megaparsec. The Planck satellite, studying the cosmic microwave background, infers 67 km/s per megaparsec. The difference is nearly 9%—too much to be an error. But if primordial black holes were heating the gas, then the surface from which the light came shifted. This changes the rate calculation, as if a thermometer in the tub showed the wrong temperature because of the drip heating. The heat from the holes doesn’t push galaxies apart faster: it throws off the calibration of our cosmic ruler.

The heating from an evaporating hole doesn’t depend on its original mass: a massive one heats a larger volume, much like a thick log and a thin splinter, burning completely, give off the same amount of heat per liter of water.

Scientists tested the idea by adding heating into calculations of the universe’s thermal history. Gamma radiation from the holes quickly transferred energy to the surrounding gas, while some energy was carried away by neutrinos — light particles that barely interact with matter. It turned out that if just 0,1% of the invisible dark matter consists of such holes, the discrepancy in the rate vanishes. However, the holes can’t be too light: they would have evaporated before the era of nucleosynthesis. And they can’t be too numerous — otherwise they would cause Reionization of all the hydrogen, and we don’t see that. So these droplets from the universe’s childhood might be the key to a precise map of the cosmos.

The warming from an evaporating black hole doesn’t depend on its mass: a large one heats a larger volume, just as a thick log and a splinter heat water equally.

In science fiction, such as Greg Egan’s novel “The Eternal Flame,” evaporating black holes serve as energy sources. Here, they act as cosmic heaters.

\Delta T_{\text{gas}} \approx 2.6 \times 10^{13} \, f_{\text{C,PBH}} \; \text{K}
independent of the black hole's mass; f_C,PBH is the PBH fraction in dark matter
\frac{\Delta H_0}{H_0} = \frac{3}{2} \frac{\Delta z}{1+z_*}
Δz is the change in the surface-of-last-scattering redshift, z_* is the original value ≈1080
Scientists
Stephen HawkingJacob BekensteinWilliam UnruhChristian DopplerAdam RiessEmmy Noether
Concepts
Hawking radiation black hole memory burden hawking radiation mechanism black hole dark matter interaction early dark energy hubble tension cosmic microwave background obscuration cosmic background nuclear reaction mass gap Bekenstein-Hawking entropy recombination neutron star mass limit reheating quantum cosmological inhomogeneities first stars nucleosynthesis information loss hubble constant iron k alpha reverberation wave amplification primordial nucleosynthesis