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In order to describe magnetogenesis during inflation in the kinetic coupling model, we utilize a gradient expansion which is based on the fact that only long-wavelength (superhorizon) modes undergo amplification.
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T. Fujita and R. Namba, Pre-reheating magnetogenesis in the kinetic coupling model, Phys. Rev. D 94
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A. Notari and K. Tywoniuk, Dissipative axial inflation
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