Supersymmetric black holes and deformation
arXiv:2207.01462 · doi:10.1103/PhysRevD.107.L121903
Abstract
The entropy of supersymmetric black holes in string theory compactifications can be related to that of a D- or M-brane system, which in many cases can be further reduced to a two-dimensional conformal field theory (CFT). For black holes in M-theory, this relation involves a decoupling limit where the black hole mass diverges. We suggest that moving away from this limit corresponds to a specific irrelevant perturbation of the CFT, namely the supersymmetric completion of the deformation. We demonstrate that the black hole mass matches precisely with the deformed energy levels, upon identifying the deformation parameter with the inverse of the leading term of the black hole mass. We discuss various implications for black holes and deformed CFT's, including a Hagedorn temperature for wrapped M5-branes, and potential change of degeneracies in the deformed theory.
arXiv commentv2: improved discussion
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