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Transfer matrices for magnetized CMB anisotropies
Large-scale magnetic fields can affect scalar cosmological perturbations whose evolution is described in the conformally Newtonian gauge and within the tight coupling approximation. The magnetized curvature perturbations present after matter radiation equality (and prior to decoupling) are computed...
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| Lenguaje: | eng |
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2006
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.73.101302 http://cds.cern.ch/record/939859 |