Primordial Magnetogenesis in a Bouncing Universe
  We investigate primordial magnetogenesis and the evolution of the
electromagnetic field through a quantum bounce, in a model that starts in the
far past from a contracting phase where only dust is present and the
electromagnetic field is in the adiabatic quantum vacuum state. By including a
coupling between curvature and electromagnetism of the form $RF_{\mu \nu}F^{\mu
\nu}$, we find acceptable magnetic field seeds within the current observational
constraints at 1 mega-parsec (Mpc), and that the magnetic power spectrum
evolves as a power-law with spectral index $n_B=6$. It is also shown that the
electromagnetic backreaction is not an issue in the model under scrutiny.
