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Towards a holographic theory of cosmology -- threads in a tapestry

In this Essay we address several fundamental issues in cosmology: What is the nature of dark energy and dark matter? Why is the dark sector so different from ordinary matter? Why is the effective cosmological constant non-zero but so incredibly small? What is the reason behind the emergence of a critical acceleration parameter of magnitude $10^{-8} cm/sec^2$ in galactic dynamics? We suggest that the holographic principle is the linchpin in a unified scheme to understand these various issues.

preprint2013arXivOpen access
Y. Jack Ng
astro-ph.COgr-qchep-th
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Y. Jack Ng

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