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Magnetized initial conditions for CMB anisotropies
This paper introduces a systematic treatment of the linear theory of scalar gravitational perturbations in the presence of a fully inhomogeneous magnetic field. The analysis is conducted both in the synchronous and in the conformally Newtonian gauges. The cosmological plasma is assumed to be compose...
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| Lenguaje: | eng |
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2004
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| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.70.123507 http://cds.cern.ch/record/796147 |