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Magnetic field contribution to the last electron-photon scattering
When the cosmic microwave photons scatter electrons just prior to the decoupling of matter and radiation, magnetic fields do contribute to the Stokes matrix as well as to the scalar, vector and tensor components of the transport equations for the brightness perturbations. The magnetized electron-pho...
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Lenguaje: | eng |
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2010
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Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/27/22/225016 http://cds.cern.ch/record/1276504 |