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New Boundary Conditions for AdS3

Published 11 Mar 2013 in hep-th and gr-qc | (1303.2662v1)

Abstract: New chiral boundary conditions are found for quantum gravity with matter on AdS3. The associated asymptotic symmetry group is generated by a single right-moving U(1) Kac-Moody-Virasoro algebra with c_R = 3l/2G. The Kac-Moody zero mode generates global left-moving translations and equals, for a BTZ black hole, the sum of the total mass and spin. The level is positive about the global vacuum and negative in the black hole sector, corresponding to ergosphere formation. Realizations arising in Chern-Simons gravity and string theory are analyzed. The new boundary conditions are shown to naturally arise for warped AdS3 in the limit that the warp parameter is taken to zero.

Citations (175)

Summary

New Boundary Conditions for AdS

The paper "New Boundary Conditions for AdS," authored by Geoffrey Compère, Wei Song, and Andrew Strominger, presents an advanced exploration of asymptotic geometry in AdS3 spaces. It introduces novel chiral boundary conditions for quantum gravity with matter within AdS3 environments. The research builds upon the foundational work of Brown and Henneaux, altering their seminal boundary conditions to uncover a self-consistent framework that accommodates BTZ black holes and yields a single right-moving U(1) Kac-Moody-Virasoro algebra.

Key Findings

  1. Asymptotic Symmetry Group: The authors establish a new asymptotic symmetry group characterized by a noncompact U(1) Kac-Moody-Virasoro algebra. This differs from the traditional Brown-Henneaux setup, where left and right Virasoro algebras manifest symmetrically. Moreover, the novel symmetry regime reveals asymmetric dynamics, with notable implications on mass and spin representations.
  2. Kac-Moody Level: The paper delineates the computation of the Kac-Moody level, which transitions from positive around the global vacuum to negative in black hole scenarios. Such behavior suggests ergosphere formation linked to superradiant instabilities, akin to phenomena observed in complex systems such as AdS fragmentation and Kerr superradiance.
  3. Realizations in Theoretical Frameworks: The implications of these chiral boundary conditions are further explored within the contexts of Chern-Simons gravity and string theory. Specifically, these conditions emerge naturally as the warp parameter in warped AdS3 is reduced to zero, reverting to traditional AdS3 models.
  4. Semiclassical Compatibility: While the study emphasizes the semiclassical consistency of the discovered boundary conditions, it acknowledges the absence of a fully developed quantum theory adhering to these constraints. The paper suggests potential avenues in warped CFTs and string compactifications to bridge this gap.

Implications

This work provides a robust platform for examining chiral symmetries in AdS3 spaces, positing significant advancements for both theoretical and applied aspects of gravitational physics. The asymmetric boundary approach introduces innovative methodologies for understanding superradiant instabilities, enriching the discourse surrounding complex gravitational systems.

Future Directions

The exploration of these new boundary conditions in regards to string compactifications and warped CFTs may yield further insights. As the quantum mechanical landscape of gravity continues to evolve, leveraging this framework could facilitate advancements in higher-dimensional models or holographic dualities. Moreover, the analysis of instabilities attributed to ergospheres could lead to enhanced comprehension of gravitational wave phenomena within astrophysical settings.

The research encapsulated in this paper harnesses deep mathematical rigor and theoretical speculation, paving the way for seminal discussions in the study of quantum gravity on AdS3 manifolds. It offers a compelling vantage point from which future explorations of asymptotic symmetries and chiral dynamics can be undertaken.

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