Higher-derivative holography with a chemical potential

We carry out an extensive study of the holographic aspects of any-dimensional higher-derivative Einstein-Maxwell theories in a fully analytic and non-perturbative fashion. We achieve this by introducing the d-dimensional version of Electromagnetic Quasitopological gravities: higher-derivative theories of gravity and electromagnetism that propagate no additional degrees of freedom and that allow one to study charged black hole solutions analytically. These theories contain non-minimal couplings, that in the holographic context give rise to a modified < JJ > correlator as well as to a general < TJJ > structure whose coefficients we compute. We constrain the couplings of the theory by imposing CFT unitarity and positivity of energy (which we show to be equivalent to causality in the bulk) as well as positive-entropy bounds from the weak gravity conjecture. The thermodynamic properties of the dual plasma at finite chemical potential are studied in detail, and we find that exotic zeroth-order phase transitions may appear, but that many of them are ruled out by the physical constraints. We further compute the shear viscosity to entropy density ratio, and we show that it can be taken to zero while respecting all the constraints, providing that the chemical potential is large enough. We also obtain the charged Renyi entropies and we observe that the chemical potential always increases the amount of entanglement and that the usual properties of Renyi entropies are preserved if the physical constraints are met. Finally, we compute the scaling dimension and magnetic response of twist operators and we provide a holographic derivation of the universal relations between the expansion of these quantities and the coefficients of < JJ > and < TJJ >.

Automated summary

We have conducted an extensive study on the holographic aspects of higher-derivative Einstein-Maxwell theories in any dimension. By introducing electromagnetic quasitopological gravities and imposing various physical constraints, we have analyzed charged black hole solutions, thermodynamic properties at finite chemical potential, shear viscosity to entropy density ratio, and charged Renyi entropies. Our results show the possibility of achieving zero viscosity to entropy density ratio and preserving the usual properties of Renyi entropies while satisfying the physical constraints.