Probing small-scale cosmological fluctuations with the 21 cm forest: Effects of neutrino mass, running spectral index, and warm dark matter

被引:37
|
作者
Shimabukuro, Hayato [1 ]
Ichiki, Kiyotomo [2 ]
Inoue, Susumu [3 ,4 ]
Yokoyama, Shuichiro [4 ]
机构
[1] Nagoya Univ, Grad Sch Sci, Dept Phys, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univers, Aichi 4648602, Japan
[3] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany
[4] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
关键词
GAMMA-RAY BURSTS; BARYON ACOUSTIC-OSCILLATIONS; HIGH-REDSHIFT; STAR-FORMATION; ALPHA FOREST; RADIO; REIONIZATION; ABSORPTION; GALAXIES; CONSTRAINTS;
D O I
10.1103/PhysRevD.90.083003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
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页数:13
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