Thermodynamic Geometry of Regular Black Hole Surrounded by Quintessence

dc.contributor.authorAhmed Rizwan, C.L.
dc.contributor.authorNaveena Kumara, A.
dc.contributor.authorVaid, D.
dc.date.accessioned2026-02-06T06:36:17Z
dc.date.issued2021
dc.description.abstractWe investigate thermodynamics of regular Bardeen AdS black hole surrounded by quintessence. Pressure-Volume (P-V) and temperature-entropy (T-S) plots are obtained from the first law of black hole thermodynamics, shows a critical behaviour. This is reflected in the divergence of specific heat against entropy plots. Using the thermodynamic geometry, we have tried to affirm this critical property. From the Ruppeiner and Weinhold geometries, we have calculated the thermodynamic curvature scalar R<inf>R</inf> and R<inf>W</inf> in the quintessence dark energy regime. It is found that in our case these thermodynamic scalars can only identify the critical behaviour and fail to show divergence at the phase transition points observed in specific heat study. © 2021, Springer Nature Singapore Pte Ltd.
dc.identifier.citationSpringer Proceedings in Physics, 2021, Vol.261, , p. 937-941
dc.identifier.issn9308989
dc.identifier.urihttps://doi.org/10.1007/978-981-33-4408-2_134
dc.identifier.urihttps://idr.nitk.ac.in/handle/123456789/30369
dc.publisherSpringer Science and Business Media Deutschland GmbH
dc.titleThermodynamic Geometry of Regular Black Hole Surrounded by Quintessence

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