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The impact of the cosmic variance on $H_0$ on cosmological analyses · Around

2018

The impact of the cosmic variance on $H_0$ on cosmological analyses

Camarena, David, Marra, Valerio

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The current $3.8 \sigma$ tension between local (arXiv:1804.10655) and global (arXiv:1605.02985) measurements of $H_0$ cannot be fully explained by the concordance $\Lambda$CDM model.

It could be produced by unknown systematics or by physics beyond the standard model.
On the other hand, it is well known that linear perturbation theory predicts a cosmic variance on the Hubble parameter $H_0$, which leads to systematic errors on its local determination.
Here, we study how including in the likelihood the cosmic variance on $H_0$ affects statistical inference.

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