Description

We explore some particle physics implications of the growing evidence for a helical primordial magnetic field (PMF). From the interactions of magnetic monopoles and the PMF, we derive an upper bound on the monopole number density, nðt0Þ < 1 ×

We explore some particle physics implications of the growing evidence for a helical primordial magnetic field (PMF). From the interactions of magnetic monopoles and the PMF, we derive an upper bound on the monopole number density, nðt0Þ < 1 × 10−20 cm−3, which is a “primordial” analog of the Parker bound for the survival of galactic magnetic fields. Our bound is weaker than existing constraints, but it is derived under independent assumptions. We also show how improved measurements of the PMF at different redshifts can lead to further constraints on magnetic monopoles. Axions interact with the PMF due to the gaγφE · B=4π interaction. Including the effects of the cosmological plasma, we find that the helicity of the PMF is a source for the axion field. Although the magnitude of the source is small for the PMF, it could potentially be of interest in astrophysical environments. Earlier derived constraints from the resonant conversion of cosmic microwave background photons into axions lead to gaγ ≲ 10−9 GeV−1 for the suggested PMF strength ∼10−14 G and coherence length ∼10 Mpc. Finally, we apply constraints on the neutrino magnetic dipole moment that arise from requiring successful big bang nucleosynthesis in the presence of a PMF, and we find μν ≲ 10−16 μB.

Downloads
PDF (356.4 KB)

Details

Title
  • Implications of a Primordial Magnetic Field for Magnetic Monopoles, Axions, and Dirac Neutrinos
Contributors
Date Created
2015-05-20
Resource Type
  • Text
  • Collections this item is in
    Identifier
    • Digital object identifier: 10.1103/PhysRevD.91.103522
    • Identifier Type
      International standard serial number
      Identifier Value
      2470-0029
    • Identifier Type
      International standard serial number
      Identifier Value
      2470-0010
    Note
    • Copyright 2015 by the American Physical Society. View the article as published at http://dx.doi.org/10.1103/PhysRevD.91.103522

    Citation and reuse

    Cite this item

    This is a suggested citation. Consult the appropriate style guide for specific citation guidelines.

    Long, Andrew J., & Vachaspati, Tanmay (2015). Implications of a primordial magnetic field for magnetic monopoles, axions, and Dirac neutrinos. PHYSICAL REVIEW D, 91(10), 0-0. http://dx.doi.org/10.1103/PhysRevD.91.103522

    Machine-readable links