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What is Near-BPS Kerr-Newman Black Holes Analysis about?

The paper investigates the spectrum of near-BPS Kerr-Newman black holes in AdS4 and its relation to the ABJM superconformal theory, proposing that the fluctuations of these black holes can be described by a version of the N = 2 super-Schwarzian theory. It finds a mass gap of order N −3/2 between the 1/16-BPS states and the lightest near BPS state, and predicts the operator dimension spectrum above this gap in the large N, low T limit. The results are consistent with the Bekenstein-Hawking formula and random

Author

Sarthak

Language

EN