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Reynolds numbers in the early Universe
After electron-positron annihilation and prior to photon decoupling the magnetic Reynolds number is approximately twenty orders of magnitude larger than its kinetic counterpart which is, in turn, smaller than one. In this globally neutral system the large-scale inhomogeneities are provided by the sp...
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| Lenguaje: | eng |
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2011
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| Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2012.04.007 http://cds.cern.ch/record/1400110 |