Solution
= Solution
Today $\rho_X/\rho_B=(m_X/mp)r/\eta\simeq\Omega_{DM}/\Omega_B\simeq5$. Hence
$$
m_X\simeq\frac{5\eta}{r(\alpha)}m_p=\frac{3\times10^{-9}}{r(\alpha)}m_p,
$$
so $\mu=3\times10^{-9}$. For suitable large $\alpha$ this is nonrelativistic and can match the observed abundance.