Geometry of \( \mathcal{I} \)-extremization and black holes microstates

From MaRDI portal
Revision as of 14:38, 2 February 2024 by Import240129110113 (talk | contribs) (Created automatically from import240129110113)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)

Publication:2317825

DOI10.1007/JHEP07(2019)174zbMATH Open1418.83026arXiv1904.04269MaRDI QIDQ2317825

Author name not available (Why is that?)

Publication date: 12 August 2019

Published in: (Search for Journal in Brave)

Abstract: The entropy of a class of asymptotically AdS4 magnetically charged BPS black holes can be obtained by extremizing the topologically twisted index of the dual three-dimensional field theory. This principle is known as mathcalI-extremization. A gravitational dual of mathcalI-extremization for a class of theories obtained by twisted compactifications of M2-branes living at a Calabi-Yau four-fold has been recently proposed. In this paper we investigate the relation between the two extremization principles. We show that the two extremization procedures are equivalent for theories without baryonic symmetries, which include ABJM and the theory dual to the non-toric Sasaki-Einstein manifold V5,2. We then consider a class of quivers dual to M2-branes at toric Calabi-Yau four-folds for which the mathcalI-functional can be computed in the large N limit, and depends on three mesonic fluxes. We propose a gravitational dual for this construction, that we call mesonic twist, and we show that the gravitational extremization problem and mathcalI-extremization are equivalent. We comment on more general cases.


Full work available at URL: https://arxiv.org/abs/1904.04269



No records found.


No records found.








This page was built for publication: Geometry of \( \mathcal{I} \)-extremization and black holes microstates

Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q2317825)