Gravitational lensing effect on cosmic microwave background polarization

Phys. Rev. D 58, 023003 – Published 22 June 1998
Matias Zaldarriaga and Uroš Seljak

Abstract

We investigate the effect of gravitational lensing by matter distribution in the universe on the cosmic microwave background polarization power spectra and temperature-polarization cross-correlation spectrum. As in the case of the temperature spectrum, gravitational lensing leads to a smoothing of narrow features and the enhancement of power on the damping tail of the power spectrum. Because the acoustic peaks in polarization spectra are narrower than in the temperature spectrum the smoothing effect is significantly larger and can reach up to 10% for l<1000 and even more above that. A qualitatively new feature is the generation of B type polarization even when only E is intrinsically present, such as in the case of pure scalar perturbations. This may be directly observed with Planck and other future small scale polarization experiments. The gravitational lensing effect is incorporated in the new version (2.4) of the CMBFAST code.

DOI: http://dx.doi.org/10.1103/PhysRevD.58.023003

  • Received 16 March 1998
  • Published 22 June 1998

© 1998 The American Physical Society

Authors & Affiliations

Matias Zaldarriaga

  • Department of Physics, MIT, Cambridge, Massachusetts 02139

Uroš Seljak

  • Harvard Smithsonian Center For Astrophysics, Cambridge, Massachusetts 02138

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