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arXiv · 1106.0362

Synchrotron Emission on the Largest Scales: Radio Detection of the Cosmic-Web

Shea Brown
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Abstract

Shocks and turbulence generated during large-scale structure formation are predicted to produce large-scale, low surface-brightness synchrotron emission. On the largest scales, this emission is globally correlated with the thermal baryon distribution, and constitutes the "Synchrotron Cosmic- Web". I present the observational prospects and challenges for detecting this faint emission with upcoming SKA pathfinders.

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Shea Brown. 2011-06-02. Synchrotron Emission on the Largest Scales: Radio Detection of the Cosmic-Web. https://doi.org/10.1007/s12036-011-9114-4

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