Einstein-Cartan non-supersymmetric spin-polarised nucleons wall dynamos

DOI10.1016/J.AOP.2021.168558zbMath1473.83067OpenAlexW3176746663MaRDI QIDQ821616

L. C. Garcia de Andrade

Publication date: 21 September 2021

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

Full work available at URL: https://doi.org/10.1016/j.aop.2021.168558

zbMATH Keywords

chiral anomaliesmagnetogenesistopological numberstorsional domain walls

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Nuclear physics (81V35) Strong interaction, including quantum chromodynamics (81V05) Spinor and twistor methods applied to problems in quantum theory (81R25) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Yang-Mills and other gauge theories in mechanics of particles and systems (70S15) Simple homotopy type, Whitehead torsion, Reidemeister-Franz torsion, etc. (57Q10)

Related Items (2)

Dynamo chiral plasma instabilities from charges and oscillations driven by torsion fluctuations ⋮ Can magnetogenesis driven by dynamo instabilities in chiral fermion plasmas, favor Einstein-Cartan AdS cosmology?

Cites Work

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• Anisotropic domain walls
• Inflating torsion defects and dilatonic domain walls
• Riemann–Cartan gravitational and axial anomalies in electrodynamics and black holes

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