Abstract
A classical fluid description is used to investigate nonlinear interactions between an electron-type neutrino burst and a collisionless magnetized electron-positron plasma. It is found that the symmetry between the electron and positron dynamics is broken due to the presence of intense neutrino bursts. The latter can excite strong upper-hybrid wakefields, which can produce unlimited acceleration of pairs across the external magnetic field direction via a surfatron mechanism. Implications of our results to the production of high-energy electrons and positrons in astrophysical environments are discussed.
Original language | English |
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Pages (from-to) | 466-473 |
Number of pages | 8 |
Journal | Journal of Experimental and Theoretical Physics |
Volume | 99 |
Issue number | 3 |
DOIs | |
Publication status | Published - 1 Sept 2004 |
Keywords
- electric excitation
- magnetic field effects
- magnetization
- plasmas
- positrons