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ThermodynamicsofLovelockblackholeswithanonminimal scalar field

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We source the Lovelock gravity theories indexed by an integer k and fixed by requiring a unique anti-de Sitter vacuum with a self-interacting nonminimal scalar field in arbitrary dimension d. For each inequivalent Lovelock gravity theory indexed by the integer k, we establish the existence of a two-parametric self-interacting potential that permits to derive a class of black hole solutions with planar horizon for any arbitrary value of the nonminimal coupling parameter. In the thermodynamical analysis of the solution, we show that, once regularized the Euclidean action, the mass contribution coming form the gravity side exactly cancels, order by order, the one arising from the matter part yielding to a vanishing mass. This result is in accordance with the fact that the entropy of the solution, being proportional to the lapse function evaluated at the horizon, also vanishes. Consequently, the integration constant appearing in the solution is interpreted as a sort of hair which turns out to vanish at high temperature.

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fields

gr-qc 1 hep-th 1

years

2026 1 2019 1

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UNVERDICTED 2

roles

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background 1

representative citing papers

Relativistic strange quark stars in Lovelock gravity

gr-qc · 2019-07-05 · unverdicted · novelty 5.0

Numerical computation of mass-radius profiles, compactness, and gravitational redshift for strange quark stars in 5D Gauss-Bonnet gravity across several values of the Gauss-Bonnet parameter.

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