Magnetogenesis in Higgs-Starobinsky inflation

In the framework of mixed Higgs-Starobinsky inflation, we consider the generation of Abelian gauge fields due to their nonminimal coupling to gravity (in two different formulations of gravity-metric and Palatini). We couple the gauge-field invariants F mu nu F mu nu and F mu nu F similar to mu nu to an integer power of the scalar curvature Rn in Jordan frame and, treating these interactions perturbatively, switch to the Einstein frame where they lead to effective kinetic and axial couplings between gauge fields and inflaton. We determine the power spectra, energy densities, correlation length, and helicality of the generated gauge fields for different values of the nonminimal coupling constants and parameter n. We analytically estimate the spectral index nB of the magnetic power spectrum and show that for n > 1 it is possible to get the scale -invariant or even red-tilted spectrum for a wide range of modes that implies larger correlation length of the generated fields. On the other hand, the magnitude of these fields typically decreases in time becoming very small in the end of inflation. Thus, it is difficult to obtain both large magnitude and correlation length of the gauge field in the frame of this model.

Automated summary

In this study, we investigate the generation of Abelian gauge fields in the framework of mixed Higgs-Starobinsky inflation. By coupling the gauge fields to gravity with nonminimal couplings, we derive the power spectra, energy densities, correlation length, and helicality of the generated gauge fields. Our results show that it is possible to obtain scale-invariant or red-tilted spectra for the gauge fields under certain conditions.