4.6 Article

THE EXTENT OF POWER-LAW ENERGY SPECTRA IN COLLISIONLESS RELATIVISTIC MAGNETIC RECONNECTION IN PAIR PLASMAS

期刊

ASTROPHYSICAL JOURNAL LETTERS
卷 816, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.3847/2041-8205/816/1/L8

关键词

acceleration of particles; galaxies: jets; gamma-ray burst: general; magnetic reconnection; pulsars: general; relativistic processes

资金

  1. DOE [DE-SC0008409, DE-SC0008655]
  2. NASA [NNX12AP17G]
  3. NSF [AST-1411879, 0171134, 0933959, 1041709, 1041710, CNS-0821794]
  4. National Science Foundation (NSF) [ACI-1053575]
  5. University of Tennessee through the use of the Kraken computing resource at the National Institute for Computational Sciences
  6. University of Colorado Boulder
  7. Division Of Astronomical Sciences
  8. Direct For Mathematical & Physical Scien [1411879] Funding Source: National Science Foundation

向作者/读者索取更多资源

Using two-dimensional particle-in-cell simulations, we characterize the energy spectra of particles accelerated by relativistic magnetic reconnection (without guide field) in collisionless electron-positron plasmas, for a wide range of upstream magnetizations sigma and system sizes. L. The particle spectra are well-represented by a power law gamma(-alpha), with a combination of exponential and super-exponential high-energy cutoffs, proportional to sigma and L, respectively. For large L and sigma, the power-law index alpha approaches about 1.2.

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