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Holographic Fluids from 5D Dilaton Gravity

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arxiv 2311.14233 v2 pith:GPVS5RZM submitted 2023-11-24 hep-th hep-ph

Holographic Fluids from 5D Dilaton Gravity

classification hep-th hep-ph
keywords dilatonholographicbranefluidblackbrane-dilatonbulkcontinuous
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study a solvable class of five-dimensional dilaton gravity models that continuously interpolate between anti-de Sitter (AdS$_5$), linear dilaton (LD$_5$) and positively curved spacetimes as a function of a continuous parameter $\nu$. The dilaton vacuum expectation value is set by a potential localized on a flat brane. We chart the elementary properties of these backgrounds for any admissible $\nu$, and determine stability conditions of the brane-dilaton system. We find that the spectrum of metric fluctuations can be either continuous or discrete. It features a massless graviton mode confined between the brane and the curvature singularity, and a massive radion mode tied to brane-dilaton stability. We show that, in the presence of a bulk black hole, the holographic theory living on the brane features a perfect fluid. The equation of state of the holographic fluid interpolates between radiation, pressureless matter and vacuum energy as a function of $\nu$. This extends earlier findings on holographic fluids. Our results suggest that the thermodynamics of the fluid mirrors precisely the thermodynamics of the bulk black hole.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Massive Graviton Dark Matter from a Gapped Continuum

    hep-th 2026-07 conditional novelty 6.0

    Radiative corrections in a 5D linear dilaton brane-world produce a long-lived massive graviton resonance and a holographic fluid, either or both of which can account for dark matter.

  2. Uncool soft-wall transitions and gravitational waves

    hep-ph 2026-04 unverdicted novelty 5.0

    Soft-wall warped geometries yield rapid, mildly supercooled phase transitions whose TeV-scale gravitational wave signals are accessible to space-based interferometers.