Spindle black holes and theories of class $\mathcal{F}$
Abstract
We construct solutions in the form of , where denotes a spindle geometry, within a particular 4d gauged supergravity with vector multiplets and a charged hypermultiplet stemming from a consistent truncation of 6d matter coupled gauged supergravity on a Riemann surface. We also compute the Bekenstein-Hawking entropy for the presumed asymptotically black hole solutions, providing a dual prediction for the spindle index of 3d superconformal field theories falling under the class . Notably, the gravitational block description of the solutions accurately replicates the entropy and the values of scalar fields at the two orbifold points of the spindle, validating our findings.
Keywords
Cite
@article{arxiv.2405.17432,
title = {Spindle black holes and theories of class $\mathcal{F}$},
author = {Kiril Hristov and Minwoo Suh},
journal= {arXiv preprint arXiv:2405.17432},
year = {2024}
}
Comments
v2: 33 pages, 1 figure, published version. arXiv admin note: substantial text overlap with arXiv:2307.10378