Do We Really Understand the Cosmos?
arXiv:1611.03505 · doi:10.1016/j.crhy.2017.02.001
Abstract
Our knowledge about the universe has increased tremendously in the last three decades or so --- thanks to the progress in observations --- but our understanding has improved very little. There are several fundamental questions about our universe for which we have no answers within the current, operationally very successful, approach to cosmology. Worse still, we do not even know how to address some of these issues within the conventional approach to cosmology. This fact suggests that we are missing some important theoretical ingredients in the overall description of the cosmos. I will argue that these issues --- some of which are not fully appreciated or emphasized in the literature --- demand a paradigm shift: We should not think of the universe as described by a specific solution to the gravitational field equations; instead, it should be treated as a special physical system governed by a different mathematical description, rooted in the quantum description of spacetime. I will outline how this can possibly be done.
Invited Review; 28 pages; 1 figure
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- The atoms of spacetime and the cosmological constant
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- First Law of Thermodynamics and Emergence of Cosmic Space in a Non-Flat Universe
- Configuration entropy in the CDM and the dynamical dark energy models: Can we distinguish one from the other?
- Varying fundamental constants: a full covariant approach and cosmological applications
- Horizon thermodynamics and cosmological equations: A holographic-like connection between thermostatistical quantities on a cosmological horizon and in the bulk
- A study of holographic dark energy models using configuration entropy
- Cosmological model based on both holographic-like connection and Padmanabhan's holographic equipartition law
- Can we constrain the dark energy equation of state parameters using configuration entropy?
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- On cosmological expansion and local physics
- Cosmological scenario based on the first and second laws of thermodynamics: Thermodynamic constraints on a generalized cosmological model