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