Sunday, May 19, 2013

1305.3261 (Thomas Tram et al.)

Optimal polarisation equations in FLRW universes    [PDF]

Thomas Tram, Julien Lesgourgues
This paper presents the linearised Boltzmann equation for photons for scalar, vector and tensor perturbations in flat, open and closed FLRW cosmologies. We show that E- and B-mode polarisation for all types can be computed using only a single hierarchy. This was previously shown explicitly for tensor modes in flat cosmologies but not for vectors, and not for non-flat cosmologies.
View original: http://arxiv.org/abs/1305.3261

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