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

Hayato Shimabukuro, Kiyotomo Ichiki, Susumu Inoue, and Shuichiro Yokoyama
Phys. Rev. D 90, 083003 – Published 14 October 2014

Abstract

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 k10Mpc1 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 mν, running of the primordial spectral index dns/dlnk and WDM particle mass mWDM, 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 mWDM10  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 gamma-ray bursts with sufficient brightness and number exist at redshifts of z1020, and the astrophysical effects of reionization and heating can be discriminated.

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  • Received 6 March 2014

DOI:https://doi.org/10.1103/PhysRevD.90.083003

© 2014 American Physical Society

Authors & Affiliations

Hayato Shimabukuro1,*, Kiyotomo Ichiki2, Susumu Inoue3,4, and Shuichiro Yokoyama4

  • 1Department of Physics, Graduate School of Science, Nagoya University, Aichi 464-8602, Japan
  • 2Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Aichi 464-8602, Japan
  • 3Max-Planck-Institut für Physik, 80805 München, Germany
  • 4Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan

  • *bukuro@nagoya-u.jp

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Vol. 90, Iss. 8 — 15 October 2014

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