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20172025
most citedThermodynamically stable asymptotically flat hairy black holes with a dilaton potential

31 citations · 40 across the 3 of their papers we have counts for

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hep-th2025

Thermal superpotential and thermodynamics of neutral hairy black holes in extended SUGRA

Andrès Anabalòn, Dumitru Astefanesei, David Choque +1

We present a family of exact neutral hairy black-hole solutions with spherical horizon topology in extended supergravity with Fayet--Iliopoulos terms. We consider a consistent dila…

hep-th2023

Holographic renormalization and the variational problem for mixed boundary conditions via a solution-dependent superpotential-like function

David Choque, Raúl Rojas

We study holographic renormalization and the variational problem in four-dimensional Einstein gravity coupled to a self-interacting scalar field in asymptotically AdS spacetimes wi…

hep-th20209 cited

Exact holographic RG flows in extended SUGRA

Andrés Anabalón, Dumitru Astefanesei, David Choque +2

We present a family of exact planar hairy neutral black hole solutions in extended supergravity with Fayet-Iliopoulos (FI) terms. We consider a model where the magnetic part of FI…

hep-th2019

Phase transitions of neutral planar hairy AdS black holes

Andres Anabalon, Dumitru Astefanesei, David Choque +1

We investigate the phase diagram of a general class of -dimensional exact regular hairy planar black holes. For some particular values of the parameters in the moduli potential,…

hep-th201931 cited

Thermodynamically stable asymptotically flat hairy black holes with a dilaton potential

Dumitru Astefanesei, David Choque, Francisco Gomez +1

We present a detailed analysis of the thermodynamics of exact asymptotically flat hairy black holes in Einstein-Maxwell-dilaton theory. We compute the regularized action, quasiloca…

hep-th2018

Scalar charges and the first law of black hole thermodynamics

Dumitru Astefanesei, Romina Ballesteros, David Choque +1

We present a variational formulation of Einstein-Maxwell-dilaton theory in flat spacetime, when the asymptotic value of the scalar field is not fixed. We obtain the boundary terms…