Abstract

We demonstrate that the near horizon symmetries of black holes in Einstein-Yang-Mills (EYM) theory are generated by an infinite-dimensional algebra that contains, in addition to supertranslations and superrotations, a non-Abelian loop algebra. This means that the Virasoro-Kac-Moody structure of EYM in asymptotically flat spacetimes has an exact analog in the near horizon region.

Highlights

  • In 2015, Hawking conjectured that, in their near horizon limit, black holes might exhibit an infinite-dimensional symmetry [1] similar to the supertranslations that appear near null infinity in asymptotically flat spacetimes [2–4]

  • The study of infinite-dimensional symmetries in the near horizon region has antecedents [13–15], and more recently it led to interesting developments and generalizations; see for instance [16–25]

  • We will consider the case of Einstein gravity coupled to Yang-Mills theory for an arbitrary gauge group G, and we will show that, in addition to supertranslations and superrotations, the black holes of the theory exhibit an infinite-dimensional symmetry that is generated by a nonAbelian loop algebra. This means that, as it happens in Einstein-Yang-Mills theory in asymptotically flat spacetimes [26], a Virasoro-Kac-Moody structure emerges in the near horizon region of colored black holes

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Summary

INTRODUCTION

In 2015, Hawking conjectured that, in their near horizon limit, black holes might exhibit an infinite-dimensional symmetry [1] similar to the supertranslations that appear near null infinity in asymptotically flat spacetimes [2–4]. We will consider the case of Einstein gravity coupled to Yang-Mills theory for an arbitrary gauge group G, and we will show that, in addition to supertranslations and superrotations, the black holes of the theory exhibit an infinite-dimensional symmetry that is generated by a nonAbelian loop algebra. This means that, as it happens in Einstein-Yang-Mills theory in asymptotically flat spacetimes [26], a Virasoro-Kac-Moody structure emerges in the near horizon region of colored black holes.

NON-ABELIAN HORIZONS
Z pffiffiffiffiffi 1 Z pffiffiffiffiffi
SYMMETRY ALGEBRA
DISCUSSION

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