  As a charged black hole reaches its extremal state via Hawking radiation,
quantum effects become important for its thermodynamic properties when its
temperature is below a mass gap scale. Using AdS$_2$/CFT$_1$ correspondence and
solutions for the corresponding Schwarzian action, we calculate the black hole
greybody factors including the quantum effects. In the low temperature limit,
the greybody factors scale as $T^{2s + 3/2}$ with $s$ the radiated field spin.
Hence, the Hawking radiation of a near-extremal charged black hole (NEBH) is
dominated by emitting scalar particles including the Higgs boson. Time
evolution of an NEBH is also calculated and shows a stochastic feature. For an
NEBH lighter than around $10^8$ times the Planck mass, its temperature at the
current universe is below the mass gap scale and is universally tens of GeV,
which is important if one searches for primordial (hidden) charged black holes.
