The small scale power asymmetry in the cosmic microwave background

TL;DR

This paper investigates small-scale power asymmetry in the cosmic microwave background, finds an initial high significance anomaly, but after corrections, concludes no intrinsic asymmetry exists at these scales, setting constraints for future models.

Contribution

The study demonstrates that the observed small-scale asymmetry is a statistical coincidence and provides new constraints on dipolar modulation amplitudes.

Findings

Initial anomaly significance of 6.5 sigma reduced to ~1 sigma after corrections.

No intrinsic asymmetry detected at small scales after accounting for effects.

Derived upper limit on dipolar modulation amplitude, A(k)<0.0045 at 95% C.L.

Abstract

We investigate the hemispherical power asymmetry in the cosmic microwave background on small angular scales. We find an anomalously high asymmetry in the multipole range l=601-2048, with a naive statistical significance of 6.5 sigma. However, we show that this extreme anomaly is simply a coincidence of three other effects, relativistic power modulation, edge effects from the mask applied, and inter-scale correlations. After correcting for all of these effects, the significance level drops to ~1 sigma, i.e., there is no anomalous intrinsic asymmetry in the small angular scales. Using this null result, we derive a constraint on a potential dipolar modulation amplitude, A(k)<0.0045 on the ~10 Mpc-scale, at 95% C.L. This new constraint must be satisfied by any theoretical model attempting to explain the hemispherical asymmetry at large angular scales.