Abstract
Abstract
We consider rotating, electrically charged, supersymmetric AdS black holes in four, five, six and seven dimensions, and provide a derivation of the respective extremization principles stating that the Bekenstein-Hawking entropy is the Legendre transform of a homogeneous function of chemical potentials, subject to a complex constraint. Extending a recently proposed BPS limit, we start from finite temperature and reach extremality following a supersymmetric trajectory in the space of complexified solutions. We show that the entropy function is the supergravity on-shell action in this limit. Chemical potentials satisfying the extremization equations also emerge from the complexified solution.
Publisher
Springer Science and Business Media LLC
Subject
Nuclear and High Energy Physics
Reference68 articles.
1. A. Strominger and C. Vafa, Microscopic origin of the Bekenstein-Hawking entropy, Phys. Lett.B 379 (1996) 99 [hep-th/9601029] [INSPIRE].
2. F. Benini, K. Hristov and A. Zaffaroni, Black hole microstates in AdS
4from supersymmetric localization, JHEP05 (2016) 054 [arXiv:1511.04085] [INSPIRE].
3. F. Benini, K. Hristov and A. Zaffaroni, Exact microstate counting for dyonic black holes in AdS
4, Phys. Lett.B 771 (2017) 462 [arXiv:1608.07294] [INSPIRE].
4. A. Zaffaroni, Lectures on AdS black holes, holography and localization, arXiv:1902.07176 [INSPIRE].
5. A. Cabo-Bizet, D. Cassani, D. Martelli and S. Murthy, Microscopic origin of the Bekenstein-Hawking entropy of supersymmetric AdS
5black holes, arXiv:1810.11442 [INSPIRE].
Cited by
59 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献