Euclid preparation - LVI. Sensitivity to non-standard particle dark matter models

Open Access

Fig. 13.

Degeneracies between the 1b-DDM parameter $Γ_{ddm} f_{ddm}^{ini}$ $\Gamma_{\mathrm{ddm}} \, f_{\mathrm{ddm}}^{\mathrm{ini}}$ and four other cosmological parameters for different data sets. Top: Optimistic case. Bottom: Pessimistic case. The addition of 3 × 2pt to WL and of Planck to 3 × 2pt leads to a better determination of all cosmological parameters and lifts degeneracies.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.