Skip to main content
Article
Cosmological Constant as Confining U(1) Charge in Two-Dimensional Dilaton Gravity
Physical Review D
  • Daniel Grumiller, Vienna University of Technology
  • Robert A McNees, IV, Loyola University Chicago
  • Jakob Salzer, Vienna University of Technology
Document Type
Article
Publication Date
8-14-2014
Disciplines
Abstract

The cosmological constant is treated as a thermodynamical parameter in the framework of two-dimensional dilaton gravity. We find that the cosmological constant behaves as a U(1) charge with a confining potential, and that such potentials require a novel Born-Infeld boundary term in the action. The free energy and other thermodynamical quantities of interest are derived, from first principles, in a way that is essentially model independent. We discover that there is always a Schottky anomaly in the specific heat and explain its physical origin. Finally, we apply these results to specific examples, like anti-de Sitter–Schwarzschild–Tangherlini black holes, Bañados-Teitelboim-Zanelli black holes and the Jackiw-Teitelboim model.

Comments

Author Posting. © American Physical Society, 2014. This article is posted here by permission of the American Physical Society for personal use, not for redistribution. The article was published in Physical Review D, Vol. 90, August 2014, http://dx.doi.org/10.1103/PhysRevD.90.044032

Creative Commons License
Creative Commons Attribution-Noncommercial-No Derivative Works 3.0
Citation Information
Grumiller, D., McNees, R.A., Salzer, J. (2014). Cosmological constant as confining U(1) charge in two-dimensional dilaton gravity. Physical Review D., Vol. 90.