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Growth rate of matter perturbations as a probe of large-scale magnetism
The growth rate of matter perturbations is computed in a magnetized environment for the LambdaCDM and wCDM paradigms. It is argued that the baryons do not necessarily follow into the dark matter potential wells after they are released from the drag of the photons. The baryonic evolution equations in...
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| Lenguaje: | eng |
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2011
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.84.063010 http://cds.cern.ch/record/1361970 |