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arXiv · 1604.01024

A framework for testing isotropy with the cosmic microwave background

Daniela Saadeh·Stephen M. Feeney·Andrew Pontzen·Hiranya V. Peiris·Jason D. McEwen
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Abstract

We present a new framework for testing the isotropy of the Universe using cosmic microwave background data, building on the nested-sampling ANICOSMO code. Uniquely, we are able to constrain the scalar, vector and tensor degrees of freedom alike; previous studies only considered the vector mode (linked to vorticity). We employ Bianchi type VII$_h$ cosmologies to model the anisotropic Universe, from which other types may be obtained by taking suitable limits. In a separate development, we improve the statistical analysis by including the effect of Bianchi power in the high-$\ell$, as well as the low-$\ell$, likelihood. To understand the effect of all these changes, we apply our new techniques to WMAP data. We find no evidence for anisotropy, constraining shear in the vector mode to $(σ_V/H)_0 < 1.7 \times 10^{-10}$ (95% CL). For the first time, we place limits on the tensor mode; unlike other modes, the tensor shear can grow from a near-isotropic early Universe. The limit on this type of shear is $(σ_{T,\rm reg}/H)_0 < 2.4 \times 10^{-7}$ (95% CL).

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Daniela Saadeh, Stephen M. Feeney, Andrew Pontzen, Hiranya V. Peiris, Jason D. McEwen. 2016-09-07. A framework for testing isotropy with the cosmic microwave background. https://doi.org/10.1093/mnras%2Fstw1731

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