The quantum, the geon, and the crystal
arXiv:1507.07777 · doi:10.1142/S0218271815420134
Abstract
Effective geometries arising from a hypothetical discrete structure of space-time can play an important role in the understanding of the gravitational physics beyond General Relativity. To discuss this question, we make use of lessons from crystalline systems within solid state physics, where the presence of defects in the discrete microstructure of the crystal determine the kind of effective geometry needed to properly describe the system in the macroscopic continuum limit. In this work we study metric-affine theories with non-metricity and torsion, which are the gravitational analog of crystalline structures with point defects and dislocations. We consider a crystal-motivated gravitational action and show the presence of topologically non-trivial structures (wormholes) supported by an electromagnetic field. Their existence has important implications for the quantum foam picture and the effective gravitational geometries. We discuss how the dialogue between solid state physics systems and modified gravitational theories can provide useful insights on both sides.
15 pages, 1 figure, matches published version
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- Observable traces of non-metricity: new constraints on metric-affine gravity
- What is a singular black hole beyond General Relativity?
- Mapping nonlinear gravity into General Relativity with nonlinear electrodynamics
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- Metric-affine bumblebee gravity: classical aspects
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- Black holes in multi-fractional and Lorentz-violating models
- KG-oscillators in Eddington-inspired Born-Infeld gravity: Wu-Yang magnetic monopole and Ricci scalar curvature effects
- Non-metricity signatures on the Higgs boson signal strengths at the LHC