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- W1520286699 abstract "We show that the ${ensuremath{Omega}}_{b}ensuremath{-}{ensuremath{Omega}}_{mathrm{DM}}$ coincidence can naturally be explained in a framework where axino is cold dark matter which is predominantly produced in nonthermal processes involving decays of $Q$-balls formed in Affleck-Dine baryogenesis. In this approach, the similarity of ${ensuremath{Omega}}_{b}$ and ${ensuremath{Omega}}_{mathrm{DM}}$ is a direct consequence of the (sub-)GeV scale of the mass of the axino, while the reheating temperature ${T}_{R}$ must be low, some ${10}^{2}text{ }text{ }mathrm{GeV}$, or less." @default.
- W1520286699 created "2016-06-24" @default.
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- W1520286699 date "2007-04-19" @default.
- W1520286699 modified "2023-10-16" @default.
- W1520286699 title "Axino Dark Matter from<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>Q</mml:mi></mml:math>-Balls in Affleck-Dine Baryogenesis and the<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:msub><mml:mi>Ω</mml:mi><mml:mi>b</mml:mi></mml:msub><mml:mo>−</mml:mo><mml:msub><mml:mi>Ω</mml:mi><mml:mi>DM</mml:mi></mml:msub></mml:math>Coincidence Problem" @default.
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- W1520286699 doi "https://doi.org/10.1103/physrevlett.98.161304" @default.
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