pith. the verified trust layer for science. sign in

arxiv: hep-ph/9209238 · v1 · pith:IYG56LNQnew · submitted 1992-09-15 · ✦ hep-ph · astro-ph

Primordial magnetic fields from pseudo-Goldstone bosons

classification ✦ hep-ph astro-ph
keywords fieldfieldsmagneticprimordialbosonpseudo-goldstoneacceptedaccount
0
0 comments X p. Extension
Add this Pith Number to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{IYG56LNQ}

Prints a linked pith:IYG56LNQ badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

The existence of large-scale magnetic fields in galaxies is well established, but there is no accepted mechanism for generating a primordial field which could grow into what is observed today. We discuss a model which attempts to account for the necessary primordial field by invoking a pseudo-Goldstone boson coupled to electromagnetism. The evolution of this boson during inflation generates a magnetic field; however, it seems difficult on rather general grounds to obtain fields of sufficient strength on astrophysically interesting scales.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation

    astro-ph.CO 2025-08 conditional novelty 7.0

    In pure axion inflation, detectable gravitational wave signals arise only in parameter regions with strong backreaction that violate the upper bound on ΔN_eff.

  2. Schwinger effect in axion inflation on a lattice

    astro-ph.CO 2025-06 unverdicted novelty 7.0

    Lattice simulations show that Schwinger currents saturate gauge-field production in axion inflation, yielding universal conductivity and magnetic-field values at the onset of strong backreaction.

  3. Gravitational waves from axion inflation in the gradient expansion formalism. Part II. Fermionic axion inflation

    astro-ph.CO 2025-09 unverdicted novelty 6.0

    Schwinger fermion production in axion inflation damps gauge fields, enabling observable primordial gravitational waves in LISA/ET bands while satisfying ΔN_eff limits and identifying a new damped-oscillation backreact...

  4. Primordial black hole dark matter from axion inflation

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    PBHs generated by axion inflation with gauge-field coupling can comprise all dark matter in the asteroidal mass range while producing a LISA-measurable stochastic GW background.

  5. Suppressed Magnetogenesis from Ultralight Dark Matter due to Finite Conductivity

    astro-ph.CO 2026-04 unverdicted novelty 5.0

    Finite conductivity of the plasma suppresses parametric resonance amplification of electromagnetic fields from ultralight pseudoscalar dark matter, making it impossible to generate magnetic fields of sufficient streng...

  6. Revisiting constraints on magnetogenesis from baryon asymmetry

    hep-ph 2025-09 unverdicted novelty 5.0

    Maximally helical primordial U(1)_Y magnetic fields can generate both intergalactic magnetic fields and baryon asymmetry; non-helical fields may work if Higgs dynamics compensate helicity loss to ≲10^{-9-10} precision...