Schr\"odinger symmetry of Schwarzschild-(A)dS black hole mechanics
Jibril Ben Achour, Etera R. Livine, Daniele Oriti

TL;DR
This paper demonstrates that Schwarzschild-(A)dS black hole dynamics exhibit a Schr"odinger symmetry, which could influence quantum gravity corrections and be explored through condensed matter analogues.
Contribution
It reveals a Schr"odinger symmetry in the reduced 2d black hole mechanics, providing a new perspective on black hole dynamics and potential quantum gravity effects.
Findings
Identifies Schr"odinger symmetry in Schwarzschild-(A)dS black holes
Reformulates black hole mechanics as a 2d system with symmetry
Suggests universal quantum corrections via Schr"odinger-preserving deformations
Abstract
We show that the dynamics of Schwarzschild-(A)dS black holes admits a symmetry under the 2d Schr\"odinger group, whatever the sign or value of the cosmological constant. This is achieved by reformulating the spherically-symmetric reduction of general relativity as a 2d mechanical system with a non-trivial potential controlled by the cosmological constant, and explicitly identifying the conserved charges for black hole mechanics. We expect the Schr\"odinger symmetry to drive the dynamics of quantum Schwarzschild-(A)dS black holes. This suggests that Schr\"odinger-preserving non-linear deformations (of the Gross-Piteavskii type) should capture universal quantum gravity corrections to the black hole geometry. Such scenario could be realized in condensed matter analogue models.
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Taxonomy
TopicsGeophysics and Sensor Technology · Noncommutative and Quantum Gravity Theories · Pulsars and Gravitational Waves Research
