Non-Lorentzian chaos and cosmological holography

dc.contributor.author	Bagchi, A.
dc.contributor.author	Chakrabortty, S.
dc.contributor.author	Grumiller, D.
dc.contributor.author	Radhakrishnan, B.
dc.contributor.author	Riegler, M.
dc.contributor.author	Sinha, A.
dc.date.accessioned	2022-08-18T10:12:44Z
dc.date.available	2022-08-18T10:12:44Z
dc.date.issued	2022-08-18
dc.identifier.uri	http://localhost:8080/xmlui/handle/123456789/3826
dc.description.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.	en_US
dc.language.iso	en_US	en_US
dc.title	Non-Lorentzian chaos and cosmological holography	en_US
dc.type	Article	en_US