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arXiv · 2011.01628

Fast magnetic field amplification in distant galaxyclusters

Gabriella Di Gennaro·Reinout J. van Weeren·Gianfranco Brunetti·Rossella Cassano·Marcus Brüggen·Matthias Hoeft·Timothy W. Shimwell·Huub J. A. Röttgering·Annalisa Bonafede·Andrea Botteon·Virginia Cuciti·Daniele Dallacasa·Francesco de Gasperin·Paola Domínguez-Fernández·Torsten A. Ensslin·Fabio Gastaldello·Soumyajit Mandal·Mariachiara Rossetti·Aurora Simionescu
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Abstract

In the present-day Universe, magnetic fields pervade galaxy clusters, with strengths of a few microGauss obtained from Faraday Rotation. Evidence for cluster magnetic fields is also provided by Megaparsec-scale radio emission, namely radio halos and relics. These are commonly found in merging systems and are characterized by a steep radio spectrum. It is widely believed that magneto-hydrodynamical turbulence and shock-waves (re-)accelerate cosmic rays, producing halos and relics. The origin and the amplification of magnetic fields in clusters is not well understood. It has been proposed that turbulence drives a small-scaledynamo that amplifies seed magnetic fields (primordial and/or injected by galactic outflows, as active galactic nuclei, starbursts, or winds). At high redshift, radio halos are expected to be faint, due to the Inverse Compton losses and dimming effect with distance. Moreover, Faraday Rotation measurements are difficult to obtain. If detected, distant radio halosprovide an alternative tool to investigate magnetic field amplification. Here, we report LOFAR observations which reveal diffuse radio emission in massive clusters when the Universe was only half of its present age, with a sample occurrence fraction of about 50%. The high radio luminosities indicate that these clusters have similar magnetic field strengths to those in nearby clusters, and suggest that magnetic field amplification is fast during the first phases ofcluster formation.

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Gabriella Di Gennaro, Reinout J. van Weeren, Gianfranco Brunetti, Rossella Cassano, Marcus Brüggen, Matthias Hoeft, Timothy W. Shimwell, Huub J. A. Röttgering, Annalisa Bonafede, Andrea Botteon, Virginia Cuciti, Daniele Dallacasa, Francesco de Gasperin, Paola Domínguez-Fernández, Torsten A. Ensslin, Fabio Gastaldello, Soumyajit Mandal, Mariachiara Rossetti, Aurora Simionescu. 2020-11-03. Fast magnetic field amplification in distant galaxyclusters. https://doi.org/10.1038/s41550-020-01244-5

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