  Black brane solutions with scalar hair and with non-AdS asymptotics have
several features that make them very interesting for holographic applications:
(1) They allow to circumvent usual no-hair theorems; (2) They may have a non
singular extremal limit in the form of a scalar soliton that interpolates
between AdS and non-AdS vacua; (3) They allow for phase transitions between the
Schwarzschild-AdS (SADS) and scalar dressed black branes; (4) They give an
holographic realization of hyperscaling violation in critical systems. In this
note I illustrate these features using an exact integrable Einstein-scalar
gravity model.
