English

CMB low multipole alignments in the $\mathbf{\Lambda}$CDM and Dipolar models

Cosmology and Nongalactic Astrophysics 2015-06-24 v1

Abstract

The dipolar model \cite{Gordon:2005ai} has attracted much interest because it may phenomenologically explain the CMB hemispherical power asymmetry found in the WMAP and Planck data. Since such a model explicitly breaks isotropy at large angular scales it is natural to wonder whether it can also explain other CMB directional anomalies. Focusing on the low \ell alignments and assuming Λ\LambdaCDM, we confirm that the quadrupole/octupole and the dipole/quadrupole/octupole alignments are anomalous with a significance up to 99.9%99.9\% C.L., for both WMAP and Planck data. Moreover, we show for the first time that such features are anomalous also in the dipolar model, roughly at the same level as in Λ\LambdaCDM. We conclude that the dipolar model does not provide a better fit to the data than the Λ\LambdaCDM.

Keywords

Cite

@article{arxiv.1503.01611,
  title  = {CMB low multipole alignments in the $\mathbf{\Lambda}$CDM and Dipolar models},
  author = {L. Polastri and A. Gruppuso and P. Natoli},
  journal= {arXiv preprint arXiv:1503.01611},
  year   = {2015}
}

Comments

13 pages, 2 figures and 4 tables

R2 v1 2026-06-22T08:45:06.547Z