7–12 Jul 2024
Aurum, the ‘Gabriele d’Annunzio’ University and ICRANet
Europe/Rome timezone

Thoughts on Spacetime Models and Cosmological Constant: Gravitation and Electromagnetism

9 Jul 2024, 15:18
18m
Aula 35 (‘Gabriele d’Annunzio’ University)

Aula 35

‘Gabriele d’Annunzio’ University

Viale Pindaro, 42, Pescara
Talk in a parallel session Theories of gravity: alternatives to the cosmological and particle standard models Theories of gravity: alternatives to the cosmological and particle standard models

Speaker

Prof. Lalaonirina Rakotomanana (IRMAR)

Description

Cosmology is mainly based on the Friedmann's equations assuming Isotropy and Homogeneity of the Einstein spacetime, starting from the Friedmann-Lemaître-Robertson Walker metric. Introduction of an ad hoc Cosmological Constant allows to model phenomenologically the so-called Dark Energy for explaining the acceleration of the Universe expansion discovered by Riess et al. and Permutter et al. in 1998.

Considering an Einstein-Cartan vacuum spacetime, this work focus on the influence of electromagnetic background field on this accelerated Universe expansion. In addition to metric and torsion (generated by independent connection), we study the influence of the compatibility of both of them with the volume-form, needed to correctly define any Lagrangian of the vacuum.

The action including Einstein-Palatini (extended version of Hilbert-Einstein Lagrangian) and Yang-Mills Lagrangians is considered all along the study. Application of rigorous Variation Procedure allows us to derive an extended system of fields equations : (1) Maxwell, (2) Einstein-Maxwell and (3) additionally a linking third relation giving what we called « Distortion of the spacetime ». This (third-order) distorsion tensor is expressed explicitly and is generated by a particular component of the background electromagnetic wave : the Chern-Simmons current which is constituted by Magnetic Helicity and Spin Angular Momentum of the wave.

Beyond the classical assumption of Perfect Fluid filling Universe, electromagnetic background clearly induces Anisotropy (and eventually Inhomogeneity) of the Spacetime which precludes any easy derivation of a sufficiently tractable extended Friedmann’s equations in such a case. Nevertheless, assuming that if only the trace torsion-vector is considered, the integral curves of the vector field might be suggested as the tangent field of giant filaments, and confirming that the two major forces remain the gravitation and magnetic forces. By the way, considering a volume-form compatible with metric and connection (with torsion) permits to obtain strikingly action similar to that of Brans-Dicke action.

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