Can magnetogenesis driven by dynamo instabilities in chiral fermion plasmas, favor Einstein-Cartan AdS cosmology?

DOI10.1016/j.aop.2021.168660zbMath1483.83068OpenAlexW3211131683MaRDI QIDQ2058680

L. C. Garcia de Andrade

Publication date: 9 December 2021

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.aop.2021.168660

zbMATH Keywords

cosmologyAdS gravityEinstein-Cartanchiral anomalieschiral dynamos

Mathematics Subject Classification ID

Electromagnetic fields in general relativity and gravitational theory (83C50) Classical and relativistic thermodynamics (80A10) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60) Exterior differential systems (Cartan theory) (58A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Simple homotopy type, Whitehead torsion, Reidemeister-Franz torsion, etc. (57Q10)

Related Items (2)

Astrophysical chiral dynamos and strain-torsioned Weyl materials ⋮ Dynamo chiral plasma instabilities from charges and oscillations driven by torsion fluctuations

Cites Work

• Einstein-Cartan non-supersymmetric spin-polarised nucleons wall dynamos
• Topological methods in hydrodynamics
• Geometric classification of the torsion tensor in space-time
• Astrophysical and terrestrial probes to test Einstein-Cartan gravity
• Neutrino Cosmology
• Chiral fermions and torsion in the early Universe
• Physical aspects of the space-time torsion

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