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Non-relativistic conformal symmetries and Newton–Cartan structures

C Duval1,3 and P A Horváthy2

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This paper provides us with a unifying classification of the conformal infinitesimal symmetries of non-relativistic Newton–Cartan spacetime. The Lie algebras of non-relativistic conformal transformations are introduced via the Galilei structure. They form a family of infinite-dimensional Lie algebras labeled by a rational 'dynamical exponent', z. The Schrödinger–Virasoro algebra of Henkel et al corresponds to z = 2. Viewed as projective Newton–Cartan symmetries, they yield, for timelike geodesics, the usual Schrödinger Lie algebra, for which z = 2. For lightlike geodesics, they yield, in turn, the Conformal Galilean Algebra (CGA) of Lukierski, Stichel and Zakrzewski (alias '\mathfrak {alt} ' of Henkel), with z = 1. Physical systems realizing these symmetries include, e.g. classical systems of massive and massless non-relativistic particles, and also hydrodynamics, as well as Galilean electromagnetism.


PACS

04.20.Gz Spacetime topology, causal structure, spinor structure

02.20.Sv Lie algebras of Lie groups

02.30.Jr Partial differential equations

04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields

MSC

37K30 Relations with infinite-dimensional Lie algebras and other algebraic structures

35Q55 NLS-like (nonlinear Schrödinger) equations (See also 37K10)

37J15 Symmetries, invariants, invariant manifolds, momentum maps, reduction (See also 53D20)

83C75 Space-time singularities, cosmic censorship, etc.

53D25 Geodesic flows

22E60 Lie algebras of Lie groups (For the algebraic theory of Lie algebras, see 17Bxx)

Subjects

Mathematical physics

Gravitation and cosmology

Dates

Issue 46 (20 November 2009)

Received 8 July 2009, in final form 26 September 2009

Published 22 October 2009



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