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- W2557281625 abstract "We study the effects of the cosmic ray instabilities excited by the current associated with an inhomogeneous distribution of sources of extragalactic cosmic rays, with average density ns. We find that under certain conditions, the resulting current can excite a non-resonant instability that forces particles with energy below some critical value to be confined within a distance n 1=3 s from the sources. This also causes the existence of a pervasive intergalactic magnetic field with a strength of order 0:01 nG." @default.
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- W2557281625 date "2016-08-18" @default.
- W2557281625 modified "2023-09-25" @default.
- W2557281625 title "Cosmic ray streaming instability generated in the intergalactic medium" @default.
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- W2557281625 doi "https://doi.org/10.22323/1.236.0534" @default.
- W2557281625 hasPublicationYear "2016" @default.
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