B polarization of cosmic background radiation from second-order scattering sources

M. Beneke, C. Fidler, K. Klingmüller

Publikation: Beitrag in FachzeitschriftArtikelBegutachtung

12 Zitate (Scopus)

Abstract

B-mode polarization of the cosmic background radiation is induced from purely scalar primordial sources at second order in perturbations of the homogeneous, isotropic universe. We calculate the B-mode angular power spectrum ClBB sourced by the second-order scattering term in the full second-order Boltzmann equations for the polarized radiation phase-space density, which have recently become available. We find that at l ≈ 200 the second-order effect is comparable to the first-order effect for a tensor-to-scalar ratio of r = 10-6, and to about 2·10 -4 at l ≈ 1000. It is always negligible relative to the weak-lensing induced contribution.

OriginalspracheEnglisch
Aufsatznummer008
FachzeitschriftJournal of Cosmology and Astroparticle Physics
Jahrgang2011
Ausgabenummer4
DOIs
PublikationsstatusVeröffentlicht - Apr. 2011
Extern publiziertJa

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