We consider the Einstein-scalar-Gauss-Bonnet theory in the presence of a cosmological
constant Λ, either positive or negative, and look for novel, regular black-hole solutions with a …

We consider the Einstein-scalar-Gauss-Bonnet theory, and study the case where a negative
cosmological constant is replaced by a more realistic, negative scalar-field potential. We …

We consider the Einstein-scalar-Gauss-Bonnet theory and assume that, at regimes of large
curvature, the Ricci scalar may be ignored compared to the quadratic Gauss-Bonnet term …

In three dimensions, we consider the Einstein–Maxwell Lagrangian dressed by a
nonminimally coupled scalar field in new massive gravity. For this theory, we provide two …

The aim of this paper is to confirm in new concrete examples that the semiclassical entropy
of a three-dimensional Lifshitz black hole can be recovered through an anisotropic …

Motivated by providing preliminary steps to understand the conception of quantum gravity, in
this paper, we study the phase structure of a semiclassical gravitational system. We …

In arbitrary dimension, we consider a theory described by the most general quadratic
curvature corrections of Einstein gravity together with a self-interacting nonminimally …

Abstract In (2+ 1)(2+ 1)-dimensional AdS spacetime, we obtain new exact black hole
solutions, including two different models (power parameter k= 1 k= 1 and k ≠ 1 k≠ 1), in the …

In five dimensions, we consider a model described by the Einstein gravity with a source
given by a scalar field and various Abelian gauge fields with dilatoniclike couplings. For this …

In this paper we obtain exact asymptotically anti-de Sitter black hole solutions and
asymptotically Lifshitz black hole solutions with dynamical exponents z= 0 and z= 4 of four …