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Cosmological electromagnetic fields and dark energy · Around

2008

Cosmological electromagnetic fields and dark energy

Jimenez, Jose Beltran, Maroto, Antonio L.

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We show that the presence of a temporal electromagnetic field on cosmological scales generates an effective cosmological constant which can account for the accelerated expansion of the universe.

Primordial electromagnetic quantum fluctuations produced during electroweak scale inflation could naturally explain the presence of this field and also the measured value of the dark energy density.
The behavior of the electromagnetic field on cosmological scales is found to differ from the well studied short-distance behavior and, in fact, the presence of a non-vanishing cosmological constant could be signalling the breakdown of gauge invariance on cosmological scales.
The theory is compatible with all the local gravity tests, and is free from classical or quantum instabilities.

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