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The Holography Hypothesis and Pre-Big Bang Cosmology

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arxiv hep-th/9811051 v1 pith:ZKKEFAMY submitted 1998-11-05 hep-th

A. K. Biswas , J. Maharana , R. K. Pradhan This is my paper · ORCID
classification hep-th
keywords boundedholographyhypothesisstringactionareabangcase
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abstract

The consequences of holography hypothesis are investigated for the Pre-big-bang string cosmological models. The evolution equations are obtained from the tree level string effective action. It is shown that $S/A$ is bounded by a constant in each case, $S$ being the entropy within the volume bounded by the horizon of area $A$.

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Cited by 1 Pith paper

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  1. Testing the Generalized Second Law in $(2+1)$-Dimensional Cosmology: Holographic Entropy Bounds and Observational Constraints

    gr-qc 2025-08 reject novelty 3.0 of 10

    In (2+1)-dimensional cosmology with a negative cosmological constant, the Fischler-Susskind entropy bound is incompatible with the generalized second law in contracting phases, while the Hubble entropy bound can be re...

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