THERMODYNAMIC GEOMETRY OF BTZ BLACK HOLE

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BEHZADIMEHR A.R.; KHAKSARI Z.; MIRZA B.

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Journal: Iranian Journal of Physics Research Year:2012 | Volume:12 | Issue:2 Page(s): 147-155

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Information Journal Paper

Title

THERMODYNAMIC GEOMETRY OF BTZ BLACK HOLE

Author(s)

BEHZADIMEHR A.R. | KHAKSARI Z. | MIRZA B. | Issue Writer Certificate

Keywords

PHASE TRANSITIONQ2

THERMODYNAMIC GEOMETRYQ2

STABILITYQ2

BLACK HOLEQ2

Abstract

In this paper, we considered cosmological constant as a variable and studied properties and the thermodynamics STABILITY of BTZ BLACK HOLE from a geometric perspective. Also, we examined the correspondence between thermodynamic curvature singularities and PHASE TRANSITIONpoints with different thermodynamic metrics. We found that theQuevedo metric cannot predict the PHASE TRANSITION points in two ensembles. This result is also valid for the kerr-de sitter spacetime.

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APA: Copy

BEHZADIMEHR, A.R., KHAKSARI, Z., & MIRZA, B.. (2012). THERMODYNAMIC GEOMETRY OF BTZ BLACK HOLE. IRANIAN JOURNAL OF PHYSICS RESEARCH, 12(2), 147-155. SID. https://sid.ir/paper/1825/en

Vancouver: Copy

BEHZADIMEHR A.R., KHAKSARI Z., MIRZA B.. THERMODYNAMIC GEOMETRY OF BTZ BLACK HOLE. IRANIAN JOURNAL OF PHYSICS RESEARCH[Internet]. 2012;12(2):147-155. Available from: https://sid.ir/paper/1825/en

IEEE: Copy

A.R. BEHZADIMEHR, Z. KHAKSARI, and B. MIRZA, “THERMODYNAMIC GEOMETRY OF BTZ BLACK HOLE,” IRANIAN JOURNAL OF PHYSICS RESEARCH, vol. 12, no. 2, pp. 147–155, 2012, [Online]. Available: https://sid.ir/paper/1825/en

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