Erratum: Toroidal magnetic field in closed Robertson-Walker cosmologies

Oliveira, A. L.; Teixeira, A. F. F.

doi:10.1103/physrevd.51.3135.2

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2001

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“…29). Since our study is purely local, we do not worry about the topology of the purely spatial hypersurfaces, so we do not fix limits for the spatial coordinates (for a discussion about these limits in the elliptic geometry see Ref.…”

Section: The Modelmentioning

confidence: 99%

On the Amplification of Cosmological Non-Maxwellian Fields in Curved Background

Oliveira

2001

Mod. Phys. Lett. A

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We study the influence of the gravitational field of Friedmann geometries upon an electromagnetic potential, through the Proca electromagnetic theory in a Dirac aether. The results are compared with those as foreseen by the Maxwellian theory in curved spacetime. Our findings show that strong amplification effects of electromagnetic fields are a distinctive possibility. Thence we discuss some related topics. * E-mail: alexandr@ov.ufrj.br 541 Mod. Phys. Lett. A 2001.16:541-555. Downloaded from www.worldscientific.com by NORTHEASTERN UNIVERSITY on 02/02/15. For personal use only.

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Section: The Modelmentioning

confidence: 99%