Large-scale anomalies of the CMB in the curvaton scenario

Understand

We extend the curvaton scenario presented by Erickcek et al.

• (2008, 2009), to explain how the even-odd multipole asymmetry of the Cosmic Microwave Background (CMB) (also called parity asymmetry, (Kim & Naselsky 2010)) and power anisotropies can be generated by the curvaton field, which acts as an extra component to the spectrum of adiabatic perturbations in the inflationary epoch.
• Our work provides a possible cosmic explanation to the CMB large-scale asymmetry problems besides systematics and unknown residuals.