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arxiv: 1708.07194 · v3 · pith:WX62M44Bnew · submitted 2017-08-23 · ✦ hep-th · gr-qc

Axionic black branes in the k-essence sector of the Horndeski model

classification ✦ hep-th gr-qc
keywords k-essencesolutionsblackfieldshorndeskisectortermanalytic
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We construct new black brane solutions in the context of Horndeski gravity, in particular in its K-essence sector. These models are supported by axion scalar fields that depend only on the horizon coordinates. The dynamics of these fields is determined by a K-essence term that includes the standard kinetic term $X$ and a correction of the form $X^{k}$. We find both neutral and charged exact and analytic solutions in $D$-dimensions, which are asymptotically anti de Sitter. Then, we describe in detail the thermodynamical properties of the four-dimensional solutions and we compute the dual holographic DC conductivity.

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  1. A new rotating axionic AdS$_4$ black hole dressed with a scalar field

    hep-th 2025-04 unverdicted novelty 4.0

    A new axionically charged rotating AdS4 black hole solution with scalar field is presented, defined by a structural function and parameters, with thermodynamics derived via Euclidean method satisfying the first law.