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Cosmic-Ray Transport in Varying Galactic Environments
Lucia Armillotta
,
Eve C. Ostriker
, Yan Fei Jiang
Astrophysical Sciences
Princeton Center for Theoretical Science (PCTS)
Princeton Institute for Computational Science and Engineering
Research output
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Contribution to journal
›
Article
›
peer-review
35
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Scopus citations
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Dive into the research topics of 'Cosmic-Ray Transport in Varying Galactic Environments'. Together they form a unique fingerprint.
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Keyphrases
Cosmic Rays
100%
Galactic Environment
100%
Cosmic Ray Transport
100%
Star Formation Rate
57%
Mid-plane
42%
Pressure Gradient
28%
Alfvn Waves
28%
Gas Properties
14%
Magnetohydrodynamic Simulation
14%
Galactic
14%
High-resolution
14%
Transport Processes
14%
Surface Density
14%
Magnetic Field
14%
Interstellar Medium
14%
Galactic Plane
14%
Gas Pressure
14%
Disk Galaxies
14%
Star-forming
14%
Pressure Profile
14%
Advection
14%
Diffusion Coefficient
14%
Supernovae
14%
Wave Damping
14%
Galactic Disks
14%
ISM
14%
Gravitational Potential
14%
Pressure Decrease
14%
Local Patch
14%
High Velocity
14%
Background Gas
14%
Fountain
14%
Wave Excitation
14%
Simulation Modeling
14%
Media Environment
14%
Combined Transport
14%
Cosmic Ray Propagation
14%
Physics
Star Formation Rate
100%
Pressure Gradient
50%
High Resolution
25%
Magnetohydrodynamic Simulation
25%
Magnetic Field
25%
Interstellar Matter
25%
Gas Pressure
25%
Disk Galaxy
25%
Supernovae
25%
Advection
25%
Gravitational Field
25%
Diffusion Coefficient
25%
Wave Excitation
25%
Transport Process
25%