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Magnetic fields in the intergalactic medium and in the cosmic web

Published online by Cambridge University Press:  03 March 2020

Marcus Brüggen
Affiliation:
University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany email: mbrueggen@hs.uni-hamburg.de
Shane O’Sullivan
Affiliation:
University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany email: mbrueggen@hs.uni-hamburg.de
Annalisa Bonafede
Affiliation:
University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany email: mbrueggen@hs.uni-hamburg.de Dipartimento di Fisica e Astronomia, Universita di Bologna, via P. Gobetti 93/2, 40129, Bologna, Italy INAF - Istituto di Radioastronomia, Bologna Via Gobetti 101, I-40129 Bologna, Italy
Franco Vazza
Affiliation:
University of Hamburg, Gojenbergsweg 112, 21029 Hamburg, Germany email: mbrueggen@hs.uni-hamburg.de Dipartimento di Fisica e Astronomia, Universita di Bologna, via P. Gobetti 93/2, 40129, Bologna, Italy INAF - Istituto di Radioastronomia, Bologna Via Gobetti 101, I-40129 Bologna, Italy
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Abstract

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In these proceedings we discuss advances in the theory and observation of magnetic fields in the intergalactic medium and in the cosmic web. We make the point that, despite perhaps unsurmountable obstacles in simulating a small-scale dynamo, currently most cosmological magnetohydrodynamical simulations paint a similar picture of magnetic field amplification in the cosmos. However, observations of magnetic fields in the intergalactic medium turn out to be very difficult. As a case in point, we present recent work on Faraday rotation measurement in the direction of a giant galaxy with the Low Frequency Array (LOFAR). These observations demonstrate the currently unique capability of LOFAR to measure Faraday rotation at the high accuracy and angular resolution required to investigate the magnetisation of large-scale structure filaments of the cosmic web.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

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