Polarization of the CMB in models with secondary ionization

Details Polarization of the CMB in models with secondary ionization Polarization of the CMB in models with secondary ionization

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.580s&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

Recent experiments on CMB anisotropy indicates that the stage of
secondary ionization may take place in post-recombination epoch. The
influence of this ionization at redshifts z < 100 on CMB polarization
generated by scalar perturbations is calculated analytically using
expansion with respect to optical depth.

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