TL;DR
This paper explores scalar black brane solutions with non-AdS asymptotics, highlighting their unique features for holography, including circumventing no-hair theorems, phase transitions, and hyperscaling violation, using an exact Einstein-scalar model.
Contribution
It provides an exact integrable Einstein-scalar gravity model demonstrating scalar black branes with non-AdS asymptotics and their holographic implications.
Findings
Existence of scalar black branes with non-AdS asymptotics.
Ability to interpolate between AdS and non-AdS vacua.
Realization of hyperscaling violation holographically.
Abstract
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.
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