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- W2031466919 abstract "We use a simple analytic model for the evolution of currents in superconducting strings to estimate the strength of the `seed' magnetic fields generated by these strings. This model is an extension of the evolution model of Martins and Shellard depending on a parameter $f$ which characterizes the importance of equilibration process in the evolution of the currents. For GUT-scale strings, we find that a viable seed magnetic field for the galactic dynamo can be generated if equilibration is weak. On the other hand, electroweak-scale strings originate magnetic fields that are smaller than required." @default.
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- W2031466919 date "1998-04-15" @default.
- W2031466919 modified "2023-09-25" @default.
- W2031466919 title "Galactic magnetic fields from superconducting strings" @default.
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- W2031466919 doi "https://doi.org/10.1103/physrevd.57.5276" @default.
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