Quantum Bounce: A Universe Without Singularity ✎ express

Original: "Quantum Big Bounce in Wheeler-DeWitt scattering theory: Ekpyrotic and LQC-like transitions"
· S. Lo Franco, G. Montani
arXiv:2603.06481 · 2026-03-06 · arXiv non-exclusive · independent analysis · 1 min
Scientists have shown how quantum mechanics can replace the Big Bang with a Big Bounce.

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A spring compressed to the limit breaks. Likewise, classical gravity theory leads to a singularity — a point where all laws break down. Quantum mechanics turns this end into an elastic bounce. Wheeler and DeWitt described the universe as a wave of probabilities. A new model applies this to space closed like a ball. Energy, like a built-in spring, makes it contract and expand.

Physicists discovered two scenarios. The first resembles the usual flow of time — expansion after contraction, as in some approaches. But at high energies, the spring 'jams': calculations require corrections.

At extreme compression, the spring's coils press against each other, just as the equation needs refining.

The second scenario is elegant: the Big Bang becomes a Big Bounce, and time reverses. Past and future swap places. The bounce works on its own, without crutches.

The quantum world smooths out spacetime curvature in the infant universe. The idea can be tested via the cosmic microwave background — perhaps it hides ring-like patterns of gravitational waves.

If a bounce occurred, concentric circles remain in the sky.

According to one scenario, the universe arose from the collision of two three-dimensional membranes in a space with more dimensions.

\hat{H} \Psi = 0
Wheeler-DeWitt equation: $\hat{H}$ is the energy operator, $\Psi$ is the wave function of the universe.
Scientists
Bryce DeWittCarlo RovelliJohn Archibald WheelerGeorges LemaîtreRalph AlpherStephen Hawking
Concepts
Wheeler-DeWitt equation quantum classical boundary quantum classical transition cosmological bounce droplet cosmological phase transition non singular cosmology time evolution geodesic equation cosmic bubble nucleation planck time contraction false vacuum domain walls Walker circulation bottleneck de sitter space virtual particle semiclassical gravity Fock space