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How Chaos Governs the Chemistry of Giants ⚡ экспресс

Original: "Chaos Gated Tunneling Drives Molecular Reactivity in Astrophysical Environments"
Quantum tunnels accelerate reactions, but molecular chaos destroys them — except for the moment when it suddenly vanishes.
Abstract

The chemistry of giant planet ionospheres is defined by proton transfer reactions, whose rates at ultra-low temperatures are controlled by quantum tunneling and vibrations. Researchers combined random matrix theory and adiabatic gauge potentials to assess quantum chaos in the transition state. Using H₃⁺ and H₅⁺ as examples, it is shown that at the critical moment, chaos subsides, boosting tunneling. A fragility index is introduced, demonstrating how vibrations bring back chaos and suppress the reaction. This approach will refine models of chemical evolution in planetary and interstellar environments.

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A chemical reaction resembles passing through a turnstile: a crowd creates chaos and gets stuck, while an orderly line moves. In the quantum world, however, when the jostling subsides, the barrier can become ghostly — a particle passes through it as if the turnstile has vanished. This tunneling governs the chemistry of giant planets.

Research has shown: in the transition state, when molecules are about to transform, chaos quiets down. It is then that hydrogen ions seep through barriers, forming molecules critical for Jupiter's atmosphere.

Quantum tunneling is passage through a barrier forbidden by classical physics. Without it, the chemistry of space would freeze.

Scientists introduced a "fragility index": it predicts which molecular vibrations return chaos and break the tunnel. The most surprising part: without this brief lull, even the strongest collisions would not trigger the reaction. Thus, in the cold depths of Jupiter, it is the suppression of chaos, not heat, that ignites the auroras.

🎯 The H3+ ion is not just abundant in Jupiter's atmosphere — it ignites its auroras.

Scientists
Jacob BekensteinStephen HawkingCharles-Augustin de CoulombJames Clerk MaxwellLudwig BoltzmannJohannes Rydberg
Tags
hydrogen entropy
Laws
second law of thermodynamicsBekenstein-Hawking entropyCoulomb's lawBoltzmann distributionRydberg formulafirst law of thermodynamics
Original: arXiv:2604.21005 · CC BY 4.0 · bridge42worlds