Magnetic Fields in the Large-Scale Structure of the Universe
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  • 作者：D. Ryu (1) ryu@canopus.cnu.ac.kr
    D. R. G. Schleicher (2) dschleic@astro.physik.uni-goettingen.de
    R. A. Treumann (3) treumann@issibern.ch
    C. G. Tsagas (4) tsagas@astro.auth.gr
    L. M. Widrow (5) widrow@astro.queensu.ca
  • 关键词：Large ; scale structure of the universe – ; Magnetic field – ; Turbulence
  • 刊名：Space Science Reviews
  • 出版年：2012
  • 出版时间：May 2012
  • 年：2012
  • 卷：166
  • 期：1-4
  • 页码：1-35
  • 全文大小：2.7 MB
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  • 作者单位：1. Department of Astronomy and Space Science, Chungnam National University, Daejeon, 305-764 Korea2. Institut f眉r Astrophysik, Georg-August-Universit盲t, Friedrich-Hund-Platz 1, 37077 G枚ttingen, Germany3. ISSI, Hallerstrasse 6, 3012 Bern, Switzerland4. Department of Physics, Aristotle University of Thessaloniki, Thessaloniki, 54124 Greece5. Department of Physics, Queen鈥檚 University, Kingston, Ontario K7L 3N6, Canada
  • 刊物类别：Physics and Astronomy
  • 刊物主题：Physics
    Astronomy
    Extraterrestrial Physics and Space Sciences
    Astrophysics
    Planetology
  • 出版者：Springer Netherlands
  • ISSN：1572-9672
文摘
Magnetic fields appear to be ubiquitous in astrophysical environments. Their existence in the intracluster medium is established through observations of synchrotron emission and Faraday rotation. On the other hand, the nature of magnetic fields outside of clusters, where observations are scarce and controversial, remains largely unknown. In this chapter, we review recent developments in our understanding of the nature and origin of intergalactic magnetic fields, and in particular, intercluster fields. A plausible scenario for the origin of galactic and intergalactic magnetic fields is for seed fields, created in the early universe, to be amplified by turbulent flows induced during the formation of the large scale structure. We present several mechanisms for the generation of seed fields both before and after recombination. We then discuss the evolution and role of magnetic fields during the formation of the first starts. We describe the turbulent amplification of seed fields during the formation of large scale structure and the nature of the magnetic fields that arise. Finally, we discuss implications of intergalactic magnetic fields.

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