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arXiv · 0809.3245

The radiative transfer for polarized radiation at second order in cosmological perturbations

Cyril Pitrou
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Abstract

This article investigates the full Boltzmann equation up to second order in the cosmological perturbations. Describing the distribution of polarized radiation by using a tensor valued distribution function, the second order Boltzmann equation, including polarization, is derived without relying on the Stokes parameters.

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Cyril Pitrou. 2008-09-18. The radiative transfer for polarized radiation at second order in cosmological perturbations. https://doi.org/10.1007/s10714-009-0782-1

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