Slowly rotating Einstein–Maxwell-dilaton black hole and some aspects of its thermodynamics View Full Text


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Article Info

DATE

2019-03

AUTHORS

M. M. Stetsko

ABSTRACT

A slowly rotating black hole solution in Einstein–Maxwell-dilaton gravity is considered. Using the obtained solution we investigate thermodynamic functions such as the black hole’s temperature, entropy and heat capacity. In addition, to examine the thermodynamic properties of the black hole an extended technique is applied. The equation of state of Van der Waals type is obtained and investigated. It has been shown that the given system has phase transitions of the first and of the zeroth order below a critical temperature, which is a notable feature of the black hole. A coexistence relation for two phases is also considered and the latent heat is calculated. In the end, critical exponents are calculated. More... »

PAGES

244

References to SciGraph publications

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  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1140/epjc/s10052-019-6738-z

    DOI

    http://dx.doi.org/10.1140/epjc/s10052-019-6738-z

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1112831679


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