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Cited by 436

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Primordial Magnetic Fields, Right Electrons, and the Abelian Anomaly

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Joyce, M., Shaposhnikov, M.·1997·Physical Review Letters

Abstract

In the standard model there are charges with Abelian anomaly only (e.g., right-handed electron number) which are effectively conserved in the early Universe until some time shortly before the electroweak scale. A state at finite chemical potential of such a charge, possibly arising due to asymmetries produced at the grand unified theory scale, is unstable to the generation of hypercharge magnetic field. Quite large magnetic fields ( $\ensuremath{\sim}{10}^{22}$ G at $T\ensuremath{\sim}100$ GeV with typical inhomogeneity scale $\ensuremath{\sim}\frac{{10}^{6}}{T}$) can be generated. These fields may be of cosmological interest, potentially acting as seeds for amplification to larger scale magnetic fields through nonlinear mechanisms. Previously derived bounds on exotic $B\ensuremath{-}L$ violating operators may also be evaded.

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Metadata

Authors
Joyce, M., & Shaposhnikov, M.
Venue
Physical Review Letters
Published
1997-08-18
Volume
79
Issue
7
Pages
1193-1196
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2132062610
Cited by
436
References
1
FWCI
10.45
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Primordial Magnetic Fields, Right Electrons, and the Abelian Anomaly. https://app.cochat.ai/papers/10.1103/physrevlett.79.1193
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Joyce, M., & Shaposhnikov, M. (1997). Primordial Magnetic Fields, Right Electrons, and the Abelian Anomaly. Physical Review Letters. https://doi.org/10.1103/physrevlett.79.1193

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