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Physics in Very Strong Magnetic Fields

期刊

SPACE SCIENCE REVIEWS
卷 191, 期 1-4, 页码 13-25

出版社

SPRINGER
DOI: 10.1007/s11214-015-0137-z

关键词

Magnetic fields; Stars; Accretion

资金

  1. NSF [AST-1008245, 1211061]
  2. NASA [NNX12AF85G]
  3. Division Of Astronomical Sciences
  4. Direct For Mathematical & Physical Scien [1211061] Funding Source: National Science Foundation
  5. NASA [75184, NNX12AF85G] Funding Source: Federal RePORTER

向作者/读者索取更多资源

This paper provides an introduction to a number of astrophysics problems related to strong magnetic fields. The first part deals with issues related to atoms, condensed matter and high-energy processes in very strong magnetic fields, and how these issues influence various aspects of neutron star astrophysics. The second part deals with classical astrophysical effects of magnetic fields: Even relatively weak fields can play a strong role in various astrophysical problems, ranging from stars, accretion disks and outflows, to the formation and merger of compact objects.

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