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    The magnetic field and turbulence of the cosmic web measured using a brilliant fast radio burst.

    Access Status
    Fulltext not available
    Authors
    Ravi, V.
    Shannon, Ryan
    Bailes, M.
    Bannister, K.
    Bhandari, S.
    Bhat, N.
    Burke-Spolaor, S.
    Caleb, M.
    Flynn, C.
    Jameson, A.
    Johnston, S.
    Keane, E.
    Kerr, M.
    Tiburzi, C.
    Tuntsov, A.
    Vedantham, H.
    Date
    2016
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Ravi, V. and Shannon, R. and Bailes, M. and Bannister, K. and Bhandari, S. and Bhat, N. and Burke-Spolaor, S. et al. 2016. The magnetic field and turbulence of the cosmic web measured using a brilliant fast radio burst. Science. 354 (6317): pp. 1249-1252.
    Source Title
    Science
    DOI
    10.1126/science.aaf6807
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/22740
    Collection
    • Curtin Research Publications
    Abstract

    Fast radio bursts (FRBs) are millisecond-duration events thought to originate beyond the Milky Way galaxy. Uncertainty surrounding the burst sources, and their propagation through intervening plasma, has limited their use as cosmological probes. We report on a mildly dispersed (dispersion measure 266.5 ± 0.1 parsecs per cubic centimeter), exceptionally intense (120 ± 30 janskys), linearly polarized, scintillating burst (FRB 150807) that we directly localize to 9 square arc minutes. On the basis of a low Faraday rotation (12.0 ± 0.7 radians per square meter), we infer negligible magnetization in the circum-burst plasma and constrain the net magnetization of the cosmic web along this sightline to <21 nanogauss, parallel to the line-of-sight. The burst scintillation suggests weak turbulence in the ionized intergalactic medium.

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