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? ? Weakly Interacting Neutrino = WIN ? ?<br />
• Prediction: ISM-SNe, wind-SNe and Cen A<br />
account for cosmic rays (quantitative model from<br />
1993 +, applied 2009 - 2013)<br />
• Prediction: At redshift of order < ∼ 80 first<br />
massive star formation, energetic CR particles, GRBs<br />
and first BHs, supermassive BHs (starting near 3 106 M⊙),<br />
high luminosity GWs (observable by PTA ?)<br />
• Prediction: radio background, neutrino background,<br />
BH formation explosion remnant Thomson depth - all<br />
detected, match<br />
27<br />
• Prediction: Radio background structure with residual<br />
Thomson depth; reionization by SMS and explosion<br />
remnant; same structure in γ-ray, X-ray and FIR bg<br />
• Prediction: At redshift of order < ∼ 80 H + 3 , H+ 2 ,<br />
and H2 forest of absorption lines
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