English

Snapping swallowtails in accelerating black hole thermodynamics

General Relativity and Quantum Cosmology 2019-05-22 v2 High Energy Physics - Theory

Abstract

The thermodynamic behaviour of a charged and accelerating AdS black hole is studied in the context of extended phase space with variable cosmological constant. When compared to the charged AdS black hole without acceleration, a remarkable new feature of `snapping swallowtails' appears. Namely, for any black hole with charge QQ and any string tension μ\mu causing the acceleration of the black hole, there exists a transition pressure Pt=3μ2/(8πQ2)P_t=3\mu^2/(8\pi Q^2) at which the standard swallowtail `snaps', causing the branch of low temperature black holes to completely disappear, leading to a pressure induced zeroth order phase transition between small and large black holes. For intermediate values of the string tension, we also observe a reentrant phase transition, as the small black hole changes to a large one and then back to small, as the pressure decreases, crossing the coexistence line of the two phases several times. We also find a new class of `mini-entropic' black holes, whose isoperimetric ratio becomes unbounded in a certain region of parameter space.

Keywords

Cite

@article{arxiv.1812.00384,
  title  = {Snapping swallowtails in accelerating black hole thermodynamics},
  author = {Niloofar Abbasvandi and Wan Cong and David Kubiznak and Robert B. Mann},
  journal= {arXiv preprint arXiv:1812.00384},
  year   = {2019}
}

Comments

18 pages, 8 figures. Accepted for publication in Classical and Quantum Gravity

R2 v1 2026-06-23T06:28:20.441Z