Journal
PHYSICAL REVIEW D
Volume 90, Issue 8, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.90.083003
Keywords
-
Funding
- Ministry of Education, Sports, Science and Technology (MEXT) of Japan [25-3015, 24340048, 24-2775]
- Grants-in-Aid for Scientific Research [13J03015] Funding Source: KAKEN
Ask authors/readers for more resources
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 greater than or similar to 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 Sigma m(nu), running of the primordial spectral index dn(s)/d ln k and WDM particle mass m(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(WDM) greater than or similar to 10 keV that may otherwise be difficult to access. 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 gammaray bursts with sufficient brightness and number exist at redshifts of z greater than or similar to 10 - 20, and the astrophysical effects of reionization and heating can be discriminated.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available