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We compute the three-point cross-correlation function of the primordial curvature perturbation generated during inflation with two powers of a vector field in a model where conformal invariance is broken by a direct coupling of the vector field with the inflaton.
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M. Giovannini and K. E. Kunze, Faraday rotation, stochastic magnetic fields and CMB maps
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2008
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V. Demozzi, V. Mukhanov, and H. Rubinstein, Magnetic fields from inflation?
2009
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S. Kanno, J. Soda, and M.-a. Watanabe, Cosmological Magnetic Fields from Inflation and Backreaction
2009
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M. Giovannini, Estimating relic magnetic fields from CMB temperature correlations
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R. K. Jain and M. S. Sloth, Consistency relation for cosmic magnetic fields
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J. R. Shaw and A. Lewis, Constraining Primordial Magnetism
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D. G. Yamazaki, T. Kajino, G. J. Mathew, and K. Ichiki, The Search for a Primordial Magnetic Field
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