pith. sign in

arxiv: 1503.01611 · v1 · pith:3FQYOOC5new · submitted 2015-03-05 · 🌌 astro-ph.CO

CMB low multipole alignments in the ΛCDM and Dipolar models

classification 🌌 astro-ph.CO
keywords dipolarlambdamodelalignmentsdataanomalousexplainoctupole
0
0 comments X
read the original 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 $\Lambda$CDM, we confirm that the quadrupole/octupole and the dipole/quadrupole/octupole alignments are anomalous with a significance up to $99.9\%$ 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 $\Lambda$CDM. We conclude that the dipolar model does not provide a better fit to the data than the $\Lambda$CDM.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The angular scale of homogeneity in the Local Universe with the SDSS blue galaxies

    astro-ph.CO 2019-06 unverdicted novelty 3.0

    SDSS blue galaxies yield an angular homogeneity scale of 22.19° ± 1.02° that matches ALFALFA HI sources and ΛCDM expectations at z < 0.06.