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arxiv: astro-ph/0410687 · v1 · submitted 2004-10-28 · 🌌 astro-ph · gr-qc· hep-ph· hep-th

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Large-scale magnetic fields from density perturbations

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classification 🌌 astro-ph gr-qchep-phhep-th
keywords densitymagneticperturbationsamplitudefieldrecombinationarisescomoving
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We derive the minimal seed magnetic field which unavoidably arises in the radiation and matter eras, prior to recombination, by the rotational velocity of ions and electrons, gravitationally induced by the non-linear evolution of primordial density perturbations. The resulting magnetic field power-spectrum is fully determined by the amplitude and spectral index of density perturbations. The rms amplitude of the seed-field at recombination is B ~ 10^{-23} (\lambda/Mpc)^{-2} G, on comoving scales larger than about 1 Mpc.

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  1. Chiral gravitational waves from multi-phase magnetogenesis

    astro-ph.CO 2026-02 unverdicted novelty 6.0

    Multi-phase inflation with chiral vector interactions generates amplified primordial magnetic fields that induce a detectable circularly polarized gravitational-wave background.