Torsional Newton-Cartan Geometry and the Schrödinger Algebra

We show that by gauging the Schrödinger algebra with critical exponent z and imposing suitable curvature constraints, that make diffeomorphisms equivalent to time and space translations, one obtains a geometric structure known as (twistless) torsional Newton-Cartan geometry (TTNC). This is a version of torsional Newton-Cartan geometry (TNC) in which the timelike vielbein τ_μ must be hypersurface orthogonal. For z=2 this version of TTNC geometry is very closely related to the one appearing in holographic duals of z=2 Lifshitz space-times based on Einstein gravity coupled to massive vector fields in the bulk. For z 2 there is however an extra degree of freedom b₀ that does not appear in the holographic setup. We show that the result of the gauging procedure can be extended to include a Stückelberg scalar χ that shifts under the particle number generator of the Schrödinger algebra, as well as an extra special conformal symmetry that allows one to gauge away b₀. The resulting version of TTNC geometry is the one that appears in the holographic setup. This shows that Schrödinger symmetries play a crucial role in holography for Lifshitz space-times and that in fact the entire boundary geometry is dictated by local Schrödinger invariance. Finally we show how to extend the formalism to generic torsional Newton-Cartan geometries by relaxing the hypersurface orthogonality condition for the timelike vielbein τ_μ.