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The V-mode polarization of the Cosmic Microwave Background
The V-mode polarization of the Cosmic Microwave Background is discussed in a weakly magnetized plasma. The VV and VT angular power spectra are computed for adiabatic initial conditions of the Einstein-Boltzmann hierarchy. Depending upon the frequency channel and upon the magnetic field intensity, th...
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| Lenguaje: | eng |
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2009
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.80.123013 http://cds.cern.ch/record/1207946 |