Abstract
We study the AdS/CFT thermodynamics of the spatially isotropic counterpart of the Bjorken similarity flow in -dimensional Minkowski space with , and of its generalization to linearly expanding -dimensional Friedmann-Robertson-Walker cosmologies with arbitrary values of the spatial curvature parameter . The bulk solution is a nonstatic foliation of the generalized Schwarzschild-AdS black hole with a horizon of constant curvature . The boundary matter is an expanding perfect fluid that satisfies the first law of thermodynamics for all values of the temperature and the spatial curvature, but it admits a description as a scale-invariant fluid in local thermal equilibrium only when the inverse Hawking temperature is negligible compared with the spatial curvature length scale. A Casimir-type term in the holographic energy-momentum tensor is identified from the threshold of black hole formation and is shown to take different forms for and .
- Received 14 October 2008
DOI:https://doi.org/10.1103/PhysRevD.78.126011
©2008 American Physical Society