Smarr Integral Formula of D-dimensional Stationary Spacetimes in Einstein-\AE ther-Maxwell Theroy
General Relativity and Quantum Cosmology
2018-06-29 v5 Astrophysics of Galaxies
High Energy Physics - Phenomenology
High Energy Physics - Theory
Abstract
Using the Wald formalism, we investigate the thermodynamics of charged black holes in D-dimensional stationary spacetimes with or without rotations in Einstein-\ae ther-Maxwell theory. In particular, assuming the existence of a scaling symmetry of the action, we obtain the Smarr integral formula, which can be applied to both Killing and universal horizons. When restricted to 4-dimensional spherically symmetric spacetimes, previous results obtained by a different method are re-derived.
Keywords
Cite
@article{arxiv.1712.09399,
title = {Smarr Integral Formula of D-dimensional Stationary Spacetimes in Einstein-\AE ther-Maxwell Theroy},
author = {Fei-hung Ho and Shao-Jun Zhang and Hai-Shan Liu and Anzhong Wang},
journal= {arXiv preprint arXiv:1712.09399},
year = {2018}
}
Comments
No figures and tables. Phys. Let. B782 (2018) 723-727