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Holographic conductivity from Einstein-Maxwell-Dilaton in Gauss-Bonnet gravity and Entropy Function

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arxiv 2212.13673 v1 pith:B4BCIRSU submitted 2022-12-28 gr-qc hep-th

classification gr-qchep-th
keywords conductivityblackgauss-bonnetconductivitieseinstein-maxwell-dilatonentropyfunctiongravity
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In this paper we consider the holographic DC and Hall conductivity in Einstein-Maxwell-Dilaton in Gauss-Bonnet gravity with momentum dissipation. We analytically derived the DC conductivity and Hall conductivity from the black horizon data, and found that the conductivities are independent on the Gauss-Bonnet coupling. We also used the entropy function formalism to get the conductivities in terms of the charge of the black hole, even without knowing the explicit black hole solutions.

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  1. The lack of influence of the scalar hair on the DC conductivity

    hep-th 2024-12 conditional novelty 4.0 of 10

    The DC conductivity of beyond-Horndeski axionic black holes is shown to be independent of the primary scalar hair parameter, depending only on horizon data and axion and charge parameters.

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