Magnetic Reconnection on Jet-Accretion disk Systems
Fast Magnetic Reconnection is currently regarded as an important process also beyond the solar system, specially in magnetically dominated regions of galactic and extragalactic sources like the surrounds of black holes and relativistic jets. In this lecture we discuss briefly the theory of fast magn...
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| Veröffentlicht in: | arXiv.org 2016-08 |
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| creator | Elisabete M de Gouveia Dal Pino del Valle, Maria Victoria Kadowaki, Luis H S Khiali, Behoruz Kowal, Grzergorz Mizuno, Yosuke Singh, Chandra B |
| description | Fast Magnetic Reconnection is currently regarded as an important process also beyond the solar system, specially in magnetically dominated regions of galactic and extragalactic sources like the surrounds of black holes and relativistic jets. In this lecture we discuss briefly the theory of fast magnetic reconnection, specially when driven by turbulence which is very frequent in Astrophysical flows, and its implications for relativistic particle acceleration. Then we discuss these processes in the context of the sources above, showing recent analytical and multidimensional numerical MHD studies that indicate that fast reconnection can be a powerful process to accelerate particles to relativistic velocities, produce the associated high energy non-thermal emission, and account for efficient conversion of magnetic into kinetic energy in these flows. |
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| issn | 2331-8422 |
| language | eng |
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| source | Free E- Journals |
| subjects | Accretion disks Black holes Computational fluid dynamics High energy astronomy Kinetic energy Particle acceleration Relativism Relativistic effects Relativistic particles Relativistic velocity Solar system Thermal emission |
| title | Magnetic Reconnection on Jet-Accretion disk Systems |
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