Ultra-high energy cosmic rays: 40 years retrospective of continuous observations at the Yakutsk array: Part 1. Cosmic ray spectrum in the energy range 1015–1018 eV and its interpretation
Ultra-high energy cosmic rays: 40 years retrospective of continuous observations at the Yakutsk array: Part 1. Cosmic ray spectrum in the energy range 1015–1018 eV and its interpretation
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超高能宇宙射线:雅库茨克阵列连续观测 40 年回顾:第 1 部分:1015-1018 eV 能量范围内的宇宙射线谱及其解释
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发表时间:
2015
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通讯作者:
Yu
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作者:
Stanislav Knurenkoa;Igor Petrovb;Zim Petrov;Ivan Sleptsov;Yu
The experimental data on the cosmic ray energy spectrum obtained from the Small Cherenkov Array in Yakutsk on the measurement of Cherenkov radiation in showers with energy 10 15 –10 18 eV are discussed. The data were obtained by means of continuous array operation since 1994. The all particle spectrum in this energy region was found to have a complex shape and cannot be described by a simple exponential function with a single slope indicator, g. After the first kink at energy 3 · 10 15 eV (knee), the spectrum becomes steeper at Δγ = 0.4 up to energy 16 eV, then part of the spectrum becomes flat to >8 · 10 16 eV, the slope of the spectrum is 2.92 ± 0.03 and then again changes slope by Δγ = 0.32 ± 0.05 from about ∼2· 10 17 eV. The second kink in the spectrum observed at the Yakutsk EAS array at ∼2·10 17 eV, or also called second knee, is a significant result for space astrophysics of ultra-high cosmic rays. In this paper we discuss possible scenarios for spectrum formation of cosmic rays by galactic sources to energies 17 eV, mainly supernovae remnants (SNR) and Metagalactic origins in the energy range 10 17 –10 18 eV. Most likely, that measurement of the second knee is related with the transitional region, galactic to extragalactic origin of cosmic rays.