Last scattering, relic gravitons and the circular polarization of the CMB
Massimo Giovannini

TL;DR
This paper investigates the origins of circular polarization in the CMB, concluding that relic gravitons and magnetized plasma do not produce V-mode polarization, with large-scale curvature fluctuations being the main source.
Contribution
It demonstrates that tensor modes and magnetized plasma do not generate V-mode polarization, highlighting the role of large-scale curvature fluctuations in the CMB.
Findings
Tensor contribution to V-mode polarization vanishes at last scattering.
Relic gravitons cannot generate V-mode polarization.
Large-scale curvature fluctuations dominate circular dichroism.
Abstract
The tensor contribution to the -mode polarization induced by a magnetized plasma at last scattering vanishes exactly. Conversely a polarized background of relic gravitons cannot generate a -mode polarization. The reported results suggest that, in the magnetized CDM paradigm, the dominant source of circular dichroism stems from the large-scale fluctuations of the spatial curvature.
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