Zevatron: Difference between revisions
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Named after the Bevatron I would assume, as it was first... |
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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 [[Lawrence Berkeley National Laboratory]]'s [[Bevatron]] and Fermi Lab's [[Tevatron]], are highly exotic hypothetical astrophysical sources capable of accelerating particles to 1 ZeV (10<small><sup>21</sup></small> [[electronvolt|eV]]). |
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Recently, there was a consideration of possibility of [[galactic jet]]s actings as Zevatrons, due to diffusive acceleration of particles caused by shock waves inside the jets. In particular, models suggested that shock waves from the nearby [[Elliptical Galaxy M87|M87]] [[galactic jet]] could accelerate an iron nucleus to ZeV ranges{{ref|1}}. |
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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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#{{note|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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[[pt:Zevatron]] |
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Latest revision as of 03:00, 21 October 2019
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