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Parker Bound and Monopole Pair Production from Primordial Magnetic Fields

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arxiv 2207.08246 v2 pith:M4VFKK4V submitted 2022-07-17 hep-ph astro-ph.COhep-th

Takeshi Kobayashi , Daniele Perri This is my paper · ORCID
classification hep-phastro-ph.COhep-th
keywords fieldsmagneticboundsprimordialboundmonopolesparkersurvival
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We present new bounds on the cosmic abundance of magnetic monopoles based on the survival of primordial magnetic fields during the reheating and radiation-dominated epochs. The new bounds can be stronger than the conventional Parker bound from galactic magnetic fields, as well as bounds from direct searches. We also apply our bounds to monopoles produced by the primordial magnetic fields themselves through the Schwinger effect, and derive additional conditions for the survival of the primordial fields.

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Cited by 1 Pith paper

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

  1. Cosmology-Independent Constraints on Irreducible Magnetic Monopole Background

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Cosmic-ray collisions with interstellar gas create monopoles that would drain galactic magnetic fields, yielding new cosmology-independent Parker-like bounds on light monopoles.

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