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#redirect [[Ultra-high-energy cosmic ray]] {{R from merge|Ultra-high-energy cosmic ray}} {{R printworthy}} |
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'''Zevatrons''', named in analogy to Fermi Lab's [[Tevatron]], are highly exotic hypothetical astrophysical sources capable of accelerating particles to 1 ZeV (10<small><sup>21</small></sup> [[electronvolt|eV]]) . |
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Recently, there was a consideration of possibility of [[galactic jet]]s actings as Zevatrons, due to the diffusive acceleration of particles by shock waves inside the jets. In particular, models suggested that shock waves from the nearby [[M87]] [[galactic jet]] could accelerate an iron nucelus to Zev ranges. <small><sup>[1]</small></sup>. |
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== See Also == |
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*[[Cosmic ray]] |
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[[Category:Astrophysics]] |
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{{astro-stub}} |
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==References== |
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[1] Honda M, Honda YS, Filamentary jets as a cosmic-ray "Zevatron", Astrophysical Journal 617 (1): L37-L40 Part 2 DEC 10 2004 |
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Latest revision as of 03:00, 21 October 2019
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