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

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

2008-09-18

arxiv.org/abs/0809.3245v2

Gen.Rel.Grav.41:2587-2595,2009

Astronomy and Astrophysics

Astrophysics

4 pages, no figure; replaced to match published version

Scientific paper

10.1007/s10714-009-0782-1

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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