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      Cosmology vs. Holography

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          Abstract

          The most radical version of the holographic principle asserts that all information about physical processes in the world can be stored on its surface. This formulation is at odds with inflationary cosmology, which implies that physical processes in our part of the universe do not depend on the boundary conditions. Also, there are some indications that the radical version of the holographic theory in the context of cosmology may have problems with unitarity and causality. Another formulation of the holographic principle, due to Fischler and Susskind, implies that the entropy of matter inside the post-inflationary particle horizon must be smaller than the area of the horizon. Their conjecture was very successful for a wide class of open and flat universes, but it did not apply to closed universes. Bak and Rey proposed a different holographic bound on entropy which was valid for closed universes of a certain type. However, as we will show, neither proposal applies to open, flat and closed universes with matter and a small negative cosmological constant. We will argue, in agreement with Easther, Lowe, and Veneziano, that whenever the holographic constraint on the entropy inside the horizon is valid, it follows from the Bekenstein-Hawking bound on the black hole entropy. These constraints do not allow one to rule out closed universes and other universes which may experience gravitational collapse, and do not impose any constraints on inflationary cosmology.

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          Holography, Cosmology and the Second Law of Thermodynamics

          We propose that in time dependent backgrounds the holographic principle should be replaced by the generalized second law of thermodynamics. For isotropic open and flat universes with a fixed equation of state, the generalized second law agrees with the cosmological holographic principle proposed by Fischler and Susskind. However, in more complicated spacetimes the two proposals disagree. A modified form of the holographic bound that applies to a post-inflationary universe follows from the generalized second law. However, in a spatially closed universe, or inside a black hole event horizon, there is no simple relationship that connects the area of a region to the maximum entropy it can contain.
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            Author and article information

            Journal
            19 April 1999
            1999-07-01
            Article
            10.1103/PhysRevD.60.103509
            hep-th/9904120
            2769b28d-869d-4164-b683-ec87df100a2c
            Custom metadata
            SU-ITP-99-6
            Phys.Rev.D60:103509,1999
            8 pages, we added one reference and comments about possible problems with unitarity and causality of the holographic theory in cosmology
            hep-th astro-ph gr-qc hep-ph

            General relativity & Quantum cosmology,General astrophysics,High energy & Particle physics

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