Pondermotive acceleration of charged particles along the relativistic jets of an accreting blackhole View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2014-05

AUTHORS

T. Ebisuzaki, T. Tajima

ABSTRACT

Accreting blackholes such as miniquasars and active galactic nuclei can contribute to the highest energy components of intra- (∼1015 eV) galactic and extra-galactic components (∼1020 eV) of cosmic rays. Alfven wave pulses which are excited in the accretion disk around blackholes propagate in relativistic jets. Because of their highly non-linear nature of the waves, charged particles (protons, ions, and electrons) can be accelerated to high energies in relativistic jets in accreting blackhole systems, the central engine of miniquasars and active galactic nuclei. More... »

PAGES

1113-1120

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1140/epjst/e2014-02162-6

DOI

http://dx.doi.org/10.1140/epjst/e2014-02162-6

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1053260377


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49 schema:description Accreting blackholes such as miniquasars and active galactic nuclei can contribute to the highest energy components of intra- (∼1015 eV) galactic and extra-galactic components (∼1020 eV) of cosmic rays. Alfven wave pulses which are excited in the accretion disk around blackholes propagate in relativistic jets. Because of their highly non-linear nature of the waves, charged particles (protons, ions, and electrons) can be accelerated to high energies in relativistic jets in accreting blackhole systems, the central engine of miniquasars and active galactic nuclei.
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