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Semi-analytical approach to magnetized temperature autocorrelations
The cosmic microwave background (CMB) temperature autocorrelations, induced by a magnetized adiabatic mode of curvature inhomogeneities, are computed with semi-analytical methods. As suggested by the latest CMB data, a nearly scale-invariant spectrum for the adiabatic mode is consistently assumed. I...
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Lenguaje: | eng |
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2007
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Acceso en línea: | https://dx.doi.org/10.1186/1754-0410-1-5 http://cds.cern.ch/record/1044291 |