Torsional Newton-Cartan Geometry and the Schr\"odinger Algebra
Eric A. Bergshoeff, Jelle Hartong, Jan Rosseel

TL;DR
This paper develops a geometric framework called torsional Newton-Cartan geometry by gauging the Schr"odinger algebra, revealing its significance in holography for Lifshitz space-times and connecting boundary geometry to Schr"odinger symmetry.
Contribution
It extends the gauging of the Schr"odinger algebra to include a St"uckelberg scalar and special conformal symmetry, clarifying the boundary geometry in Lifshitz holography.
Findings
TTNC geometry relates to Lifshitz holography for z=2.
Extra degree of freedom b_0 appears for z≠2 but can be gauged away.
Schr"odinger symmetry dictates the boundary geometry in holographic models.
Abstract
We show that by gauging the Schr\"odinger algebra with critical exponent 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 must be hypersurface orthogonal. For this version of TTNC geometry is very closely related to the one appearing in holographic duals of Lifshitz space-times based on Einstein gravity coupled to massive vector fields in the bulk. For there is however an extra degree of freedom that does not appear in the holographic setup. We show that the result of the gauging procedure can be extended to include a St\"uckelberg scalar that shifts under the particle number generator of…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
