Non-Riemannian generalizations of the Born–Infeld model and the meaning of the cosmological term

DOI10.1142/S0219887817501080zbMath1377.83081WikidataQ115245359 ScholiaQ115245359MaRDI QIDQ5370973

Diego Julio Cirilo-Lombardo

Publication date: 20 October 2017

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

non-Riemannian geometrycosmological termsigma modelBorn-Infeldfundamental constantsmagnetogenesisdynamo effectanomalous MHDdynamical torsion field

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Magnetohydrodynamics and electrohydrodynamics (76W05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Electromagnetic fields in general relativity and gravitational theory (83C50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)

Related Items (3)

Dynamical symmetries, coherent states and nonlinear realizations: Towards noncommutative gravity ⋮ Non-Riemmanian geometry, force-free magnetospheres and the generalized Grad-Shafranov equation ⋮ Beyond general relativity models, magnetosphere structure and dark matter stars

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