Reconstructing the Thomson optical depth due to patchy reionization with 21 cm fluctuation maps

Gilbert P. Holder, Ilian T. Iliev, Garrelt Mellema

Research output: Contribution to journalArticlepeer-review

Abstract

Large fluctuations in the electron column density can occur during the ionization process. We investigate the possibility of deriving the electron density fluctuations through detailed mapping of the redshifted 21 cm emission from the neutral medium during reionization. We find that the electron-scattering optical depth and 21 cm differential brightness temperature are strongly anticorrelated, allowing optical depth estimates based entirely on redshifted 21 cm measurements. This should help us to isolate the cosmic microwave background (CMB) polarization fluctuations due to reionization, allowing for the removal of the patchy reionization polarization signal from the other polarization signals and for a measurement of the primordial CMB quadrupole at various locations in the universe at the epoch of reionization. This latter application, in principle, allows for three-dimensional mapping of the primordial density field at z ∼ 1100 over a large fraction of the Hubble volume.

Original languageEnglish (US)
Pages (from-to)L1-L4
JournalAstrophysical Journal
Volume663
Issue number1 II
DOIs
StatePublished - Jul 1 2007
Externally publishedYes

Keywords

  • Cosmic microwave background
  • Cosmology: theory -intergalactic medium
  • Large-scale structure of universe
  • Radiative transfer
  • Radio lines: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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