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A fundamental problem in plasma and astrophysics is the interaction between energetic particles and magnetized plasmas. Besides plasmas in fusion devices, energetic particles can be found in different astrophysical scenarios. Examples are so-called Solar Energetic Particles (SEPs) and Cosmic Rays. These particles experience strong scattering while they propagate through the interplanetary or interstellar space. Describing those scattering effects theoretically is important in order to understand the motion of Cosmic Rays through the Universe and the mechanism of diffusive shock acceleration. The latter mechanism is important for understanding the origin of cosmic radiation.
In recent years we have achieved a more complete understanding of the fundamental scattering mechanisms due to the development of computer simulations and non-linear diffusion theories. Currently, our research team explores those scattering mechanisms to achieve further progress in the theory of charged particle transport by using numerical and analytical tools. The results are applied to different physical scenarios such as Cosmic Ray propagation and acceleration of particles at interplanetary shocks and supernova remnants.
A fundamental problem in plasma and astrophysics is the interaction between energetic particles and magnetized plasmas. Besides plasmas in fusion devices, energetic particles can be found in different astrophysical scenarios. Examples are so-called Solar Energetic Particles (SEPs) and Cosmic Rays. These particles experience strong scattering while they propagate through the interplanetary or interstellar space. Describing those scattering effects theoretically is important in order to understand the motion of Cosmic Rays through the Universe and the mechanism of diffusive shock acceleration. The latter mechanism is important for understanding the origin of cosmic radiation.
In recent years we have achieved a more complete understanding of the fundamental scattering mechanisms due to the development of computer simulations and non-linear diffusion theories. Currently, our research team explores those scattering mechanisms to achieve further progress in the theory of charged particle transport by using numerical and analytical tools. The results are applied to different physical scenarios such as Cosmic Ray propagation and acceleration of particles at interplanetary shocks and supernova remnants.
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ADVANCES IN SPACE RESEARCHno. 1 (2024): 1073-1082
A. Shalchi, V. Arendt
Advances in Space Research (2023)
The Cherenkov Telescope Array Consortium,:,H. Abdalla,H. Abe,F. Acero,A. Acharyya,R. Adam,I. Agudo, A. Aguirre-Santaella,R. Alfaro,J. Alfaro, C. Alispach,
H. E. S. S. Collaboration,A. Abramowski,F. Acero, F. Aharonian, A. G. Akhperjanian,G. Anton,A. Barnacka,U. Barres de Almeida,A. R. Bazer-Bachi,Y. Becherini, J. Becker,B. Behera,
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Roberta Zanin,H. Abdalla, H. Abe, S. Abe, A. Abusleme, F. Acero,A. Acharyya,V. Acin Portella, K. Ackley, R. Adam, C. Adams, S.S. Adhikari,
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021) (2021)
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