A Collision That Heats the Vacuum ✎ express

Original: "Separating Equation-of-State Dynamics from Hadronic Rescattering in Low-Mass Dileptons"
arXiv:2608.04598v1 · 2026-08-05 · arXiv non-exclusive · independent analysis · 1 min
The glow of electron pairs reveals how matter changes its properties under extreme impacts.

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When two atomic nuclei smash together, a tiny fireball is born. It lives for an instant, but inside, entire epochs pass: compression, heating, expansion. Physicists have learned to eavesdrop on this process, and their "microphone" is the pairs of electrons and positrons that fly out of the ball at different stages.

In the new work, two scenarios were compared. In the first, the matter inside the ball rearranges smoothly, like butter softening in a pan. In the second, it changes abruptly, as if ice turns into water. The sharp transition adds an early burst of radiation, while the smooth one enhances the low-energy part later: the ball lives longer and heats itself.

The collision energy of 2.2 gigaelectronvolts per nucleon is about twice the rest mass of a proton packed into each participant of the impact.

The difference is clearly visible after averaging over the entire evolution. At low beam energies, the two scenarios diverge like branches of a tree. So by measuring the flow of such pairs at accelerators, one can precisely tell what happened to the matter in the first moments after the impact.

A positron is the twin of an electron, but with a positive charge. When it meets an ordinary electron, both vanish, turning into pure energy.

Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
Phase transition first order phase transition Navier-Stokes equations delay differential equation differential equations electric dipole moment Gross–Pitaevskii equation