The secondary cosmic microwave background (CMB) B-modes stem from the
post-decoupling distortion of the polarization E-modes due to the
gravitational lensing effect of large-scale structures. These lensing-induced
B-modes constitute both a valuable probe of the dark matter distribution and
an important contaminant for the extraction of the primary CMB B-modes from
inflation. Planck provides accurate nearly all-sky measurements of both the
polarization E-modes and the integrated mass distribution via the
reconstruction of the CMB lensing potential. By combining these two data
products, we have produced an all-sky template map of the lensing-induced
B-modes using a real-space algorithm that minimizes the impact of sky masks.
The cross-correlation of this template with an observed (primordial and
secondary) B-mode map can be used to measure the lensing B-mode power
spectrum at multipoles up to 2000. In particular, when cross-correlating with
the B-mode contribution directly derived from the Planck polarization maps,
we obtain lensing-induced B-mode power spectrum measurement at a significance
level of 12σ, which agrees with the theoretical expectation derived
from the Planck best-fit ΛCDM model. This unique nearly all-sky
secondary B-mode template, which includes the lensing-induced information
from intermediate to small (10≲ℓ≲1000) angular scales, is
delivered as part of the Planck 2015 public data release. It will be
particularly useful for experiments searching for primordial B-modes, such as
BICEP2/Keck Array or LiteBIRD, since it will enable an estimate to be made of
the lensing-induced contribution to the measured total CMB B-modes.Comment: 20 pages, 12 figures; Accepted for publication in A&A; The B-mode map
is part of the PR2-2015 Cosmology Products; available as Lensing Products in
the Planck Legacy Archive http://pla.esac.esa.int/pla/#cosmology; and
described in the 'Explanatory Supplement'
https://wiki.cosmos.esa.int/planckpla2015/index.php/Specially_processed_maps#2015_Lensing-induced_B-mode_ma