Secondary cosmic microwave background anisotropies in a universe reionized in patches

Andrei Gruzinov, H. U. Wayne

    Research output: Contribution to journalArticle

    Abstract

    In a universe reionized in patches, the Doppler effect from Thomson scattering off free electrons generates secondary cosmic microwave background (CMB) anisotropies. For a simple model with small patches and late reionization, we analytically calculate the anisotropy power spectrum. Patchy reionization can, in principle, be the main source of anisotropies on arcminute scales. On larger angular scales, its contribution to the CMB power spectrum is a small fraction of the primary signal and is only barely detectable in the power spectrum with even an ideal, i.e., cosmic variance limited, experiment and an extreme model of reionization. Consequently, patchy reionization is unlikely to affect cosmological parameter estimation from the acoustic peaks in the CMB. Its detection on small angles would help determine the ionization history of the universe, in particular, the typical size of the ionized region and the duration of the reionization process.

    Original languageEnglish (US)
    Pages (from-to)435-439
    Number of pages5
    JournalAstrophysical Journal
    Volume508
    Issue number2 PART II
    DOIs
    StatePublished - 1998

    Keywords

    • Cosmic microwave background
    • Cosmology: theory
    • Intergalactic medium
    • Large-scale structure of universe

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

    Fingerprint Dive into the research topics of 'Secondary cosmic microwave background anisotropies in a universe reionized in patches'. Together they form a unique fingerprint.

  • Cite this