Volume 99, Number 2, July 2012
|Number of page(s)||5|
|Published online||19 July 2012|
Thermodynamic geometry of black hole in the deformed Hořava-Lifshitz gravity
Institute of Theoretical Physics, Lanzhou University - Lanzhou 730000, PRC
Received: 12 April 2012
Accepted: 22 June 2012
We investigate the thermodynamic geometry and phase transition of Kehagias-Sfetsos black hole in the deformed Hořava-Lifshitz gravity with coupling constant λ = 1. The phase transition in black-hole thermodynamics is thought to be associated with the divergence of the capacities. And the structures of these divergent points are studied. We also find that the thermodynamic curvature produced by the Ruppeiner metric is positive definite for all r+ > r− and is divergent at η2 = 0 corresponding to the divergent points of CΦ and CT . These results suggest that the microstructure of the black hole has an effective repulsive interaction, which is very similar to the ideal gas of fermions. These may shed some light on the microstructure of the black hole.
PACS: 04.70.Dy – Quantum aspects of black holes, evaporation, thermodynamics / 04.90.+e – Other topics in general relativity and gravitation (restricted to new topics in section 04)
© EPLA, 2012
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.