Probing small-scale cosmological fluctuations with the 21 cm forest:
  effects of neutrino mass, running spectral index and warm dark matter
  Although the cosmological paradigm based on cold dark matter and adiabatic,
nearly scale-invariant primordial fluctuations is consistent with a wide
variety of existing observations, it has yet to be sufficiently tested on
scales smaller than those of massive galaxies, and various alternatives have
been proposed that differ significantly in the consequent small-scale power
spectrum (SSPS) of large-scale structure. Here we show that a powerful probe of
the SSPS at $k\gtrsim 10$ Mpc$^{-1}$ can be provided by the 21 cm forest, that
is, systems of narrow absorption lines due to intervening, cold neutral
hydrogen in the spectra of high-redshift background radio sources in the cosmic
reionization epoch. Such features are expected to be caused predominantly by
collapsed gas in starless minihalos, whose mass function can be very sensitive
to the SSPS. As specific examples, we consider the effects of neutrino mass,
running spectral index (RSI) and warm dark matter (WDM) on the SSPS, and
evaluate the expected distribution in optical depth of 21 cm absorbers out to
different redshifts. Within the current constraints on quantities such as the
sum of neutrino masses $\sum m_\nu$, running of the primordial spectral index
$d n_s/d \ln k$ and WDM particle mass $m_{\rm WDM}$, the statistics of the 21
cm forest manifest observationally significant differences that become larger
at higher redshifts. In particular, it may be possible to probe the range of
$m_{\rm WDM} \gtrsim 10$ keV that may otherwise be inaccessible. Future
observations of the 21 cm forest by the Square Kilometer Array may offer a
unique and valuable probe of the SSPS, as long as radio sources such as quasars
or Population III gamma-ray bursts with sufficient brightness and number exist
at redshifts of $z \gtrsim$ 10 - 20, and the astrophysical effects of
reionization and heating can be discriminated.
