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  4. Modeling the radio background from the first black holes at cosmic dawn: Implications for the 21 cm absorption amplitude
 
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Modeling the radio background from the first black holes at cosmic dawn: Implications for the 21 cm absorption amplitude
Ewall-Wice, A.
Chang, T.-C.
Lazio, J.
Doré, O.
Seiffert, M.
Monsalve, Raúl
Facultad de Ingeniería 
10.3847/1538-4357/aae51d
The American Astronomical Society (AAS)
2018
We estimate the 21 cm radio background from accretion onto the first intermediate-mass black holes between z ≈ 30 and z ≈ 16. Combining potentially optimistic, but plausible, scenarios for black hole formation and growth with empirical correlations between luminosity and radio emission observed in low-redshift active galactic nuclei, we find that a model of black holes forming in molecular cooling halos is able to produce a 21 cm background that exceeds the cosmic microwave background (CMB) at z ≈ 17, though models involving larger halo masses are not entirely excluded. Such a background could explain the surprisingly large amplitude of the 21 cm absorption feature recently reported by the EDGES collaboration. Such black holes would also produce significant X-ray emission and contribute to the 0.5–2 keV soft X-ray background at the level of ≈10−13–10−12 erg s−1 cm−2 deg−2, consistent with existing constraints. In order to avoid heating the intergalactic medium (IGM) over the EDGES trough, these black holes would need to be obscured by hydrogen column depths of N H ~ 5 × 1023 cm−2. Such black holes would avoid violating constraints on the CMB optical depth from Planck if their UV photon escape fractions were below f esc 0.1, which would be a natural result of N H ~ 5 × 1023 cm−2 being imposed by an unheated IGM.
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Checksum
Dark ages
Reionization
First stars
Ciencias físicas
Historial de mejoras
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