Emergent physics: Fermi point scenario
arXiv:0801.0724 · doi:10.1098/rsta.2008.0070
Abstract
The Fermi-point scenario of emergent gravity has the following consequences: gravity emerges together with fermionic and bosonic matter; emergent fermionic matter consists of massless Weyl fermions; emergent bosonic matter consists of gauge fields; Lorentz symmetry persists well above the Planck energy; space-time is naturally 4-dimensional; Universe is naturally flat; cosmological constant is naturally small or zero; underlying physics is based on discrete symmetries; `quantum gravity' cannot be obtained by quantization of Einstein equations; there is no contradiction between quantum mechanics and gravity; etc.
16 pages, 8 figures, submitted to proceedings of Royal Society scientific discussion meeting "Cosmology meets condensed matter" held on 28 January 2008 in London, references added
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- Breaking Diffeomorphism Invariance and Tests for the Emergence of Gravity
- Emergent Gravity requires (kinematic) non-locality
- Mass Varying Neutrinos, Quintessence, and the Accelerating Expansion of the Universe
- Emergent gauge symmetries -- making symmetry as well as breaking it
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- Disorder effects on thermal transport on the surface of topological superconductors by the self-consistent Born approximation
- Emergent gravity: the BEC paradigm
- Challenges for Emergent Gravity
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- The cosmological constant and scale hierarchies with emergent gauge symmetries
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- Divergences in spinfoam quantum gravity
- Fundamental Principles of Theoretical Physics and Concepts of Quasiaverages, Quantum Protectorate and Emergence
- Quantum Gravity: Has Spacetime Quantum Properties?
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- String Theory - Nomological Unification and the Epicycles of the Quantum Field Theory Paradigm
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- Diffeomorphism Invariance Breaking in Gravity and Cosmological Evolution
- Fundamental Principles of Theoretical Physics and Concepts of Quantum Protectorate and Emergence