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66 × 1011pc ) γDvD aRH a0  ln ( 2 T∗ Teq ) − ln  1 + √ ( γDvD aRH a0 ) 2( T∗ T0 ) 2 + 1     , (27) where we have used the fact that g∗ remains constant after T∗ = 2 × 10−5

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Constraining Nonthermal Dark Matter's Impact on the Matter Power Spectrum

astro-ph.CO · 2019-08-27 · conditional · novelty 6.0

Nonthermal dark matter produced relativistically in an early matter-dominated era remains mostly relativistic at reheating, so free streaming suppresses small-scale structure and Lyman-alpha plus Milky Way satellite data bound its production velocity.

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  • Constraining Nonthermal Dark Matter's Impact on the Matter Power Spectrum astro-ph.CO · 2019-08-27 · conditional · none · ref 4

    Nonthermal dark matter produced relativistically in an early matter-dominated era remains mostly relativistic at reheating, so free streaming suppresses small-scale structure and Lyman-alpha plus Milky Way satellite data bound its production velocity.