Holography in \((2+1)\)-dimensional cosmological models
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Publication:5934671
DOI10.1016/S0370-2693(99)01122-3zbMath0993.83026arXivhep-th/9910185OpenAlexW3102202661MaRDI QIDQ5934671
Publication date: 7 May 2001
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/9910185
Related Items (6)
Two Fluids Cosmological Model in (2+1)-Dimensional Saez-Ballester Scalar-Tensor Theory of Gravitation ⋮ FRIEDMANN EQUATION AND CARDY FORMULA CORRESPONDENCE IN BRANE UNIVERSES ⋮ Relationship between \((2+1)\) and \((3+ 1)\)-Friedmann-Robertson-Walker cosmologies; linear, non-linear, and polytropic state equations ⋮ Closed universes can satisfy the holographic principle in three dimensions ⋮ The holographic principle ⋮ Holography in \((2+1)\)-dimensional cosmological model with generalized equation of state
Cites Work
- Boundary dynamics and the statistical mechanics of the \((2+1)\)-dimensional black hole
- Holography, Cosmology, and the Second Law of Thermodynamics
- Black Hole Entropy from Conformal Field Theory in Any Dimension
- What we don't know about BTZ black hole entropy
- The world as a hologram
- Near-horizon Virasoro symmetry and the entropy of de Sitter space in any dimension
- Conformal description of horizon's states
- Holographic principle in the closed universe: a resolution with negative pressure matter
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