How the Jitters of Space Can Stifle the Birth of Black Holes express

Original: "Tensor-Induced Backreaction in Ultra-Slow-Roll Inflation"
arXiv:2608.07264v1 · 2026-08-07 · CC BY 4.0 · 1 min
The invisible ripples of space itself may hold back the formation of tiny black holes in the early universe.

When you blow up a balloon too quickly, its surface starts to quiver. Something similar happened to space in the first moments after the Big Bang: the universe expanded rapidly, and the very fabric of space began to ripple. This ripple, gravitational waves, doesn't just travel through the cosmos; it can also interfere with the birth of tiny black holes.

Normally, such holes could form when an especially dense clump of energy randomly appeared in the expanding universe. But calculations show that the jitters of space act like a headwind. They slow down the expansion right where a clump is trying to become a hole. The process resembles a self-regulating system: the stronger the expansion in a region, the more powerful the counter-wave that reins it in.

Here, gravitational waves act not as an observable signal but as a built-in limiter, like the float in a toilet tank that keeps water from overflowing.

This effect changes the game for theorists. Previously, to get the right number of black holes, you had to fine-tune the expansion parameters very precisely, like tuning a radio, where the slightest turn of the dial takes you off the station. Now, nature itself turns the dial back, smoothing out the peaks. The fine-tuning that seemed suspicious becomes much less critical.

All this happens within the same field that drives the universe's expansion — no extra entities needed. The geometry of space itself, by curving, restrains its own growth.

The tiny black holes in question could be the size of an atom but weigh as much as a mountain. If such a hole passed through Earth, it would leave a tunnel thinner than a human hair.

Scientists
Albert EinsteinBarry BarishKip ThorneRichard FeynmanRussell HulseStephen Hawking
Concepts
black hole memory burden backreaction black hole feedback refined inflationary dynamics Penrose process mass inflation scalar perturbations logarithmic correction quantum corrections quasar feedback negative energy starobinsky inflation barrow entropy dark energy black hole interaction inflation