The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence

We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical expe...
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Autor*in:	Na-Na Gao [verfasserIn] Jian-Fu Zhang [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Schlagwörter:	Magnetohydrodynamics Interplanetary turbulence Interplanetary particle acceleration Interstellar medium Cosmic rays

Übergeordnetes Werk:	In: The Astrophysical Journal - IOP Publishing, 2022, 961(2024), 1, p 80
Übergeordnetes Werk:	volume:961 ; year:2024 ; number:1, p 80

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3847/1538-4357/ad0d9e

Katalog-ID:	DOAJ09759041X

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520			\|a We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions.
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spelling	10.3847/1538-4357/ad0d9e doi (DE-627)DOAJ09759041X (DE-599)DOAJ627210fefc034240a9f4673d3ce242f8 DE-627 ger DE-627 rakwb eng QB460-466 Na-Na Gao verfasserin aut The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions. Magnetohydrodynamics Interplanetary turbulence Interplanetary particle acceleration Interstellar medium Cosmic rays Astrophysics Jian-Fu Zhang verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 80 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 80 https://doi.org/10.3847/1538-4357/ad0d9e kostenfrei https://doaj.org/article/627210fefc034240a9f4673d3ce242f8 kostenfrei https://doi.org/10.3847/1538-4357/ad0d9e kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 80
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allfieldsSound	10.3847/1538-4357/ad0d9e doi (DE-627)DOAJ09759041X (DE-599)DOAJ627210fefc034240a9f4673d3ce242f8 DE-627 ger DE-627 rakwb eng QB460-466 Na-Na Gao verfasserin aut The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions. Magnetohydrodynamics Interplanetary turbulence Interplanetary particle acceleration Interstellar medium Cosmic rays Astrophysics Jian-Fu Zhang verfasserin aut In The Astrophysical Journal IOP Publishing, 2022 961(2024), 1, p 80 (DE-627)269019219 (DE-600)1473835-1 15384357 nnns volume:961 year:2024 number:1, p 80 https://doi.org/10.3847/1538-4357/ad0d9e kostenfrei https://doaj.org/article/627210fefc034240a9f4673d3ce242f8 kostenfrei https://doi.org/10.3847/1538-4357/ad0d9e kostenfrei https://doaj.org/toc/1538-4357 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2014 GBV_ILN_2088 GBV_ILN_2522 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 961 2024 1, p 80
language	English
source	In The Astrophysical Journal 961(2024), 1, p 80 volume:961 year:2024 number:1, p 80
sourceStr	In The Astrophysical Journal 961(2024), 1, p 80 volume:961 year:2024 number:1, p 80
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Magnetohydrodynamics Interplanetary turbulence Interplanetary particle acceleration Interstellar medium Cosmic rays Astrophysics
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container_title	The Astrophysical Journal
authorswithroles_txt_mv	Na-Na Gao @@aut@@ Jian-Fu Zhang @@aut@@
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callnumber-first	Q - Science
author	Na-Na Gao
spellingShingle	Na-Na Gao misc QB460-466 misc Magnetohydrodynamics misc Interplanetary turbulence misc Interplanetary particle acceleration misc Interstellar medium misc Cosmic rays misc Astrophysics The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence
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topic_title	QB460-466 The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence Magnetohydrodynamics Interplanetary turbulence Interplanetary particle acceleration Interstellar medium Cosmic rays
topic	misc QB460-466 misc Magnetohydrodynamics misc Interplanetary turbulence misc Interplanetary particle acceleration misc Interstellar medium misc Cosmic rays misc Astrophysics
topic_unstemmed	misc QB460-466 misc Magnetohydrodynamics misc Interplanetary turbulence misc Interplanetary particle acceleration misc Interstellar medium misc Cosmic rays misc Astrophysics
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title	The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence
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title_auth	The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence
abstract	We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions.
abstractGer	We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions.
abstract_unstemmed	We numerically study the diffusion and scattering of cosmic rays (CRs) together with their acceleration processes in the framework of the modern understanding of magnetohydrodynamic (MHD) turbulence. Based on the properties of compressible MHD turbulence obtained from observations and numerical experiments, we investigate the interaction of CRs with plasma modes. We find that (1) the gyroradius of particles exponentially increases with the acceleration timescale; (2) the momentum diffusion presents the power-law relationship with the gyroradius in the strong turbulence regime, and shows a plateau in the weak turbulence regime implying a stochastic acceleration process; (3) the spatial diffusion is dominated by the parallel diffusion in the sub-Alfvénic regime, while it is dominated by the perpendicular diffusion in the super-Alfvénic one; (4) as for the interaction of CRs with plasma modes, the particle acceleration is dominated by the fast mode in the high β case, while in the low β case, it is dominated by the fast and slow modes; and (5) in the presence of acceleration, magnetosonic modes still play a critical role in the diffusion and scattering processes of CRs, which is in good agreement with earlier theoretical predictions.
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title_short	The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence
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The Diffusion and Scattering of Accelerating Particles in Compressible MHD Turbulence

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