タイトル | Numerical Simulation of the Anomalous Transport of High-Energy Cosmic Rays in Galactic Superbubble |
本文(外部サイト) | http://hdl.handle.net/2060/20140002601 |
著者(英) | MeWaldt, R. A.; Price, E. M.; Barghouty, A. F. |
発行日 | 2013-07-02 |
言語 | eng |
内容記述 | A continuous-time random-walk (CTRW) model to simulate the transport and acceleration of high-energy cosmic rays in galactic superbubbles has recently been put forward (Barghouty & Schnee 2102). The new model has been developed to simulate and highlight signatures of anomalous transport on particles' evolution and their spectra in a multi-shock, collective acceleration context. The superbubble is idealized as a heterogeneous region of particle sources and sinks bounded by a random surface. This work concentrates on the effects of the bubble's assumed astrophysical characteristics (cf. geometry and roughness) on the particles' spectra. |
NASA分類 | Astrophysics |
レポートNO | M13-2459 |
権利 | Copyright, Distribution as joint owner in the copyright |