English

Thermodynamics of Lorentzian Taub-NUT spacetimes

High Energy Physics - Theory 2019-10-02 v2 General Relativity and Quantum Cosmology

Abstract

The thermodynamics of the Taub-NUT solution has been predominantly studied in the Euclidean sector, upon imposing the condition for the absence of Misner strings. Such thermodynamics is quite exceptional: the periodicity of the Euclidean time is restricted and thence the NUT charge cannot be independently varied, the entropy is not equal to a quarter of the area, and the thermodynamic volume can be negative. In this paper we revisit this paradigm and study the thermodynamics of the Lorentzian Taub-NUT solution, maintaining (as recently shown relatively harmless) Misner strings. We argue that in order to formulate a full cohomogeneity first law where the NUT parameter can be independently varied, it is natural to introduce a new charge together with its conjugate quantity. We consider two scenarios: one in which the entropy is given by the Lorentzian version of the Noether charge, the other in which the entropy is given by the standard Bekenstein--Hawking area law. In both cases consistent thermodynamics with positive thermodynamic volume can be formulated.

Keywords

Cite

@article{arxiv.1903.08668,
  title  = {Thermodynamics of Lorentzian Taub-NUT spacetimes},
  author = {Robie A. Hennigar and David Kubiznak and Robert B. Mann},
  journal= {arXiv preprint arXiv:1903.08668},
  year   = {2019}
}

Comments

5 pages, no figures