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- W1497258423 abstract "In this presentation we summarize our previous results concerning the evolution of primordial magnetic fields with and without helicity during the expansion of the Universe. We address different magnetogenesis scenarios such as inflation, electroweak and QCD phase transitions magnetoge nesis. A high Reynolds number in the early Universe ensures strong coupling between magnetic field and fluid moti ons. After generation the subsequent dynamics of the magnetic field is governed by decaying hydromagnetic turbul ence. We claim that primordial magnetic fields can be considered as a seeds for observed magnetic fields in galaxie s and clusters. Magnetic field strength bounds obtained in our analysis are consistent with the upper and lower limits of extragalactic magnetic fields." @default.
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- W1497258423 date "2015-07-02" @default.
- W1497258423 modified "2023-09-27" @default.
- W1497258423 title "Evolution of Primordial Magnetic Fields: From Generation Till Today" @default.
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