Non-Lorentzian Chaos and Cosmological Holography
arXiv:2106.07649 · doi:10.1103/PhysRevD.104.L101901
Abstract
We study chaos in non-Lorentzian field theories, specifically Galilean and Carrollian conformal field theories in two dimensions. In a large central charge limit, we find that the Lyapunov exponent saturates the bound on chaos, conjectured originally for relativistic field theories. We recover the same Lyapunov exponent holographically by a shock-wave calculation in three-dimensional flat space cosmologies, providing further evidence for flat space holography.
5 pages, 1 figure
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Cited by in corpus (11)
- Carroll contractions of Lorentz-invariant theories
- Scattering Amplitudes: Celestial and Carrollian
- Fractons, dipole symmetries and curved spacetime
- Carrollian hydrodynamics from symmetries
- Islands in Flat-Space Cosmology
- From CFTs to theories with Bondi-Metzner-Sachs symmetries: Complexity and out-of-time-ordered correlators
- Bound on Lyapunov exponent in Einstein-Maxwell-Dilaton-Axion black holes
- Fast Scrambling due to Rotating Shockwaves in BTZ
- Einstein's equations and the pseudo-entropy of pseudo-Riemannian information manifolds
- Asymptotic symmetries in Carrollian theories of gravity
- Asymptotic symmetries in Carrollian theories of gravity with a negative cosmological constant