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20132026
most citedPhase transition, Quasinormal modes and Hawking radiation of Schwarzschild black hole in Quintessence field

61 citations · 222 across the 9 of their papers we have counts for

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gr-qc2026

Exact Analytical Phase Transitions, Horizon Bistability, and Thermodynamic State-Space Representation of Regular Hayward Black Holes

Jyothipriya M Shaji, Jiswin Varghese, R. Tharanath +1

We establish exact analytical thresholds and present a unified thermodynamic state-space representation for the regular Hayward black hole, resolving the full phase structure witho…

gr-qc2025

Thermodynamics of Reissner-Nordstörm black bounce black hole

Feba C Joy, R Tharanath

Black bounce black holes are modification of classical black hole solutions that regularize the singularity by using a bouncing parameter. In our work, we explored the thermodynami…

gr-qc2014★ 14 cited

A unified thermodynamic picture of Hořava-Lifshitz black hole in arbitrary space time

Jishnu Suresh, Tharanath R, V C Kuriakose

In this paper, we analyze the complete thermodynamic and phase transition phenomena of a black hole solution in Hořava-Lifshitz gravity in arbitrary space time. Nature of phase tra…

gr-qc2014★ 45 cited

Phase transitions and Geometrothermodynamics of Regular black holes

R. Tharanath, Jishnu Suresh, V. C. Kuriakose

In this paper we study the thermodynamics and state space geometry of regular black hole solutions such as Bardeen black hole, Ayón-Beato and García black hole, Hayward black hole…

gr-qc2014★ 12 cited

Thermodynamic Geometry of Reissener-Nordström-de Sitter black hole and its extremal case

R. Tharanath, Jishnu Suresh, Nijo Varghese +1

We study the thermodynamics and the different thermodynamic geometric methods of Reissener-Nordström-de Sitter black hole and its extremal case, which is similar to the de Sitter b…

gr-qc2014★ 61 cited

Phase transition, Quasinormal modes and Hawking radiation of Schwarzschild black hole in Quintessence field

R. Tharanath, Nijo Varghese, V C Kuriakose

Black hole thermodynamic stability can be determined by studying the nature of heat capacity of the system. For Schwarzschild black hole the heat capacity is negative, but in the q…