Luminosity distance for Born-Infeld electromagnetic waves propagating in a cosmological magnetic background

Details Luminosity distance for Born-Infeld electromagnetic waves propagating in a cosmological magnetic background Luminosity distance for Born-Infeld electromagnetic waves propagating in a cosmological magnetic background

2006-01-10

arxiv.org/abs/astro-ph/0601208v3

JCAP 0806:006,2008

Astronomy and Astrophysics

Astrophysics

7 Pages, 4 figures. Extended introduction and some clarifications in sections 2 and 3. Version to be published in JCAP

Scientific paper

10.1088/1475-7516/2008/06/006

Born-Infeld electromagnetic waves interacting with a static magnetic background are studied in an expanding universe. The non-linear character of Born-Infeld electrodynamics modifies the relation between the energy flux and the distance to the source, which gains a new dependence on the redshift that is governed by the background field. We compute the luminosity distance as a function of the redshift and compare with Maxwellian curves for supernovae type Ia.

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