From Lorentzian to Galilean (2+1) gravity: Drinfel'd doubles, quantisation and noncommutative spacetimes

preprint2014arXivOpen access

Abstract

It is shown that the canonical classical rr-matrix arising from the Drinfel'd double structure underlying the two-fold centrally extended (2+1) Galilean and Newton-Hooke Lie algebras (with either zero or non-zero cosmological constant ΛΛ, respectively) originates as a well-defined non-relativistic contraction of a specific class of canonical rr-matrices associated with the Drinfel'd double structure of the (2+1) (anti)-de Sitter Lie algebra. The full quantum group structure associated with such (2+1) Galilean and Newton-Hooke Drinfel'd doubles is presented, and the corresponding noncommutative spacetimes are shown to contain a commuting 'absolute time' coordinate x^0{\hat x}_0 together with two noncommutative space coordinates (x^1,x^2)({\hat x}_1,{\hat x}_2), whose commutator is a function of the cosmological constant ΛΛ and of the (central) 'quantum time' coordinate x^0{\hat x}_0. Thus, the Chern-Simons approach to Galilean (2+1) gravity can be consistently understood as the appropriate non-relativistic limit of the Lorentzian theory, and their associated quantum group symmetries (which do not fall into the family of so-called kappa-deformations) can also be derived from the (anti)-de Sitter quantum doubles through a well-defined quantum group contraction procedure.

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