Dolan, Brian P.
(2014)
Vacuum energy and the latent heat of AdS-Kerr black holes.
Physical Review D, 90 (084002).
pp. 1-8.
ISSN 1550-7998
Abstract
Phase transitions for rotating asymptotically anti–de Sitter black holes in four dimensions are described
in the P − T plane, in terms of the Hawking temperature and the pressure provided by the cosmological
constant. The difference between constant angular momentum and constant angular velocity is highlighted;
the former has a second order phase transition while the latter does not. If the angular momentum is fixed
there a line of first order phase transitions terminating at a critical point with a second order phase transition
and vanishing latent heat, while if the angular velocity is fixed there is a line of first order phase transitions
terminating at a critical point with infinite latent heat. For constant angular velocity the analytic form of the
phase boundary is determined, latent heats derived and the Clapeyron equation verified.
Item Type: |
Article
|
Additional Information: |
This article was originally published at DOI: 10.1103/PhysRevD.90.084002 |
Keywords: |
Vacuum energy; latent heat; AdS-Kerr black holes; |
Academic Unit: |
Faculty of Science and Engineering > Mathematical Physics |
Item ID: |
5821 |
Identification Number: |
https://doi.org/10.1103/PhysRevD.90.084002 |
Depositing User: |
Dr. Brian Dolan
|
Date Deposited: |
11 Feb 2015 15:02 |
Journal or Publication Title: |
Physical Review D |
Publisher: |
American Physical Society |
Refereed: |
Yes |
URI: |
|
Use Licence: |
This item is available under a Creative Commons Attribution Non Commercial Share Alike Licence (CC BY-NC-SA). Details of this licence are available
here |
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