Hawking-Page transition in holographic massive gravity
Allan Adams, Daniel A. Roberts, and Omid Saremi

TL;DR
This paper investigates how momentum dissipation affects the Hawking-Page transition in holographic models, revealing that increased dissipation lowers the deconfinement temperature, leading to a zero-temperature transition at strong dissipation.
Contribution
It introduces a holographic model incorporating momentum dissipation and analyzes its impact on the Hawking-Page transition, showing a novel zero-temperature deconfinement transition.
Findings
Deconfinement temperature decreases with increasing momentum dissipation.
Critical temperature reaches zero at strong dissipation.
Zero-temperature deconfinement transition occurs at high dissipation.
Abstract
We study the Hawking-Page transition in a holographic model of field theories with momentum dissipation. We find that the deconfinement temperature strictly decreases as momentum dissipation is increased. For sufficiently strong momentum dissipation, the critical temperature goes to zero, indicating a zero-temperature deconfinement transition in the dual field theory.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Quantum Electrodynamics and Casimir Effect
