中文

局部星际电子宇宙射线光谱

天体物理学 2011-08-19 v4

摘要

我们考虑过去 30 年校正了太阳效应后,对电子与正电子的直接测量结果。 resulting overall electron spectrum may be fitted with a single power law above few GeV with spectral index (γ=3.41±0.02\gamma_{-} = 3.41 \pm 0.02), consistent with the spectral index of the positron spectrum (γ+=3.40±0.06\gamma_{+} = 3.40 \pm 0.06), therefore suggesting a common acceleration process for both species. We propose that the engine was a shock wave originating from the last supernova explosion among those that formed the local bubble. In addition, at low energy, the electron spectrum measured during the last A+A+ solar phase is damped, whereas the positron spectrum is well represented by a single power law down to the lowest inferred local interstellar energy (0.8 GeV). We suggest that this difference arises from a time- and charge-dependent effect of the solar modulation that is not taken into account by the force-field approximation.

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引用

@article{arxiv.astro-ph/0302307,
  title  = {The Local Interstellar Spectrum of Cosmic Ray Electrons},
  author = {Diego Casadei and Veronica Bindi},
  journal= {arXiv preprint arXiv:astro-ph/0302307},
  year   = {2011}
}

备注

10 pages, 9 figures, 1 table. OBSOLETE: please refer to ApJ 612 (2004) 262-267, that is the final version of this work