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The observational methods for detecting and measuring extragalactic magnetic fields are discussed, along with some new indirect methods which could be used for inferring field strengths at large redshifts which are otherwise beyond the reach of direct measurement. Various cosmological seed field generation mechanisms are reviewed, which could generate seed fields for the subsequently formed galaxies. The question of whether the original seed fields were produced in galaxies, or the pre-recombination early Universe must await a clearer picture of how the first stars and galaxies formed.
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P. P. Kronberg (Fri,) studied this question.
synapsesocial.com/papers/6a1edf36c803c9f817ac8742 — DOI: https://doi.org/10.1088/0034-4885/57/4/001
P. P. Kronberg
University of Toronto
Reports on Progress in Physics
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