Figure 2.
The 21-cm distortion as a function of redshift for various values of fPBH. The fiducial parameters are fBH, X = λ = 0.1 and fduty = 0.01. We have ignored any modification to thermal history of Universe such as changes in electron fraction and matter temperature. We also show the case where we fix fPBH to 10−4 but tune fBH, X, λ, and fduty such that radio luminosity is boosted by a factor of 20. With a further boost of a factor 2–3, the parameters could help explain the ARCADE excess.

The 21-cm distortion as a function of redshift for various values of fPBH. The fiducial parameters are fBH, X = λ = 0.1 and fduty = 0.01. We have ignored any modification to thermal history of Universe such as changes in electron fraction and matter temperature. We also show the case where we fix fPBH to 10−4 but tune fBH, X, λ, and fduty such that radio luminosity is boosted by a factor of 20. With a further boost of a factor 2–3, the parameters could help explain the ARCADE excess.

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