2026-06-08T02:38:19Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/60332023-08-27T12:13:06Zcom_20.500.14352_14col_20.500.14352_15

00925njm 22002777a 4500 dc Cabral, Francisco author Lobo, Francisco S. N. author Rubiera García, Diego author 2019-12 Einstein-Cartan theory is an extension of the standard formulation of General Relativity where torsion (the antisymmetric part of the affine connection) is non-vanishing. Just as the space-time metric is sourced by the stress-energy tensor of the matter fields, torsion is sourced via the spin density tensor, whose physical effects become relevant at very high spin densities. In this work we introduce an extension of the Einstein-Cartan-Dirac theory with an electromagnetic (Maxwell) contribution minimally coupled to torsion. This contribution breaks the U(1) gauge symmetry, which is suggested by the possibility of a torsion-induced phase transition in the early Universe, yielding new physics in extreme (spin) density regimes. We obtain the generalized gravitational, electromagnetic and fermionic field equations for this theory, estimate the strength of the corrections, and discuss the corresponding phenomenology. In particular, we briefly address some astrophysical considerations regarding the relevance of the effects which might take place inside ultra-dense neutron stars with strong magnetic fields (magnetars). 1434-6044 10.1140/epjc/s10052-019-7536-3 https://hdl.handle.net/20.500.14352/6033 http://dx.doi.org/10.1140/epjc/s10052-019-7536-3 https://link.springer.com/ Einstein-Cartan-Dirac gravity with U(1) symmetry breaking