The CMB asymmetry from inflation
  Erickcek, Kamionkowski and Carroll proposed in 2008 that the dipole
modulation of the CMB could be due to a very large scale perturbation of the
field $\phi$ causing the primordial curvature perturbation. We repeat their
calculation using weaker assumptions and the current data. If $\phi$ is the
inflaton of {\em any} single-field inflation with the attractor behaviour, the
asymmetry is almosy certainly too small. If instead $\phi$ is {\em any}
curvaton-type field (ie.\ one with the canonical kinetic term and a negligible
effect during inflation) the asymmetry can agree with observation if $|\fnl|$
in the equilateral configuration is $\simeq 10$ for $k\mone=1\Gpc$ and $\lsim
3$ for $k\mone=1\Mpc$. An $\fnl$ with these properties can apparently be
obtained from the curvaton with an axionic potential. Within any specific
curvaton-type model, the function $\fnl(k_1,k_2,k_3)$ required to generate the
asymmetry would be determined, and could perhaps already be confirmed or ruled
out using existing Planck or WMAP data.
