Optimally scrambling chiral spin-chain with effective black hole geometry

Aiden Daniel1, Andrew Hallam2, Matthew D Horner2,3

  • 1School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, UK. py17ald@leeds.ac.uk.

Scientific Reports
|March 18, 2025
PubMed
Summary

This study uses a chiral spin-chain to model black hole interiors, revealing chaotic dynamics and optimal scrambling behavior. The Lyapunov exponent increases linearly with temperature inside the black hole, unlike the quadratic increase outside.

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