Bubbles in the early universe hide gravitational waves express

Original: "Non-conformal obstructions to bubble expansion"
arXiv:2607.27874v1 · 2026-07-30 · CC BY 4.0 · 1 min
Astrophysicists have found that bubbles of a new state of matter, growing after the Big Bang, encounter unexpected obstacles — and this changes predictions about gravitational waves.

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The universe right after the Big Bang was like a boiling cauldron: bubbles of a new state of matter were bursting and growing everywhere. These were first-order phase transitions — exactly like water boiling, only at temperatures reaching trillions of degrees. According to the Standard Model, one such transition could have spawned the very matter that makes up everything around us.

Calculations based on pure Yang–Mills theory (a simplified version of the strong interaction) have revealed an unpleasant surprise. It turns out that the motion of bubble walls hits hydrodynamic barriers — as if a bubble in boiling water suddenly runs into an invisible wall. Some solutions simply vanish. For physics close to quantum chromodynamics, explosive expansion modes — detonations — are completely forbidden. Instead, 'shocked detonations' can arise: an additional shock wave is born inside a rarefaction wave.

Interestingly, these barriers act as a cosmic breakwater — they quench the most powerful gravitational waves that were hoped to be captured.

All this dramatically changes the energy balance inside the bubbles and, consequently, predictions about the gravitational-wave background. If detonations are forbidden, the most powerful waves simply do not occur. On the other hand, knowing about such invisible barriers helps to better separate extraneous bursts from the sought-after ripples. The code for constructing solutions has been made publicly available — now anyone can check how the bubbles of the early universe conceal their waves.

The walls of such bubbles can accelerate to nearly the speed of light, but sometimes slow down to the speed of sound — like a speedboat suddenly dropping to a gentle current.

Scientists
George GamowLeo EsakiHenri PoincaréFritz ZwickyJoseph WeberStephen Hawking
Concepts
obstacle bubble collision bubble nucleation bottleneck hydrodynamics Yang-Mills equation Navier-Stokes equations confined water transport classical physics unconventional superconductivity hydrodynamic simulation microorganism swimming dynamics patterned fluid dynamics smoothed particle hydrodynamics energy conditions