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Formation of large-scale cosmic structure by the Doppler instability
Y. B. Band
Department of Chemistry
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peer-review
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Dive into the research topics of 'Formation of large-scale cosmic structure by the Doppler instability'. Together they form a unique fingerprint.
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Keyphrases
Atomic Density
50%
Balmer Lines
50%
Conduction-radiation
50%
Conductor-like Screening Model for Real Solvents (COSMO-RS)
50%
Cosmic Structure
100%
Dynamical Effect
50%
Electromagnetic Radiation
50%
Energy Range
50%
Growth Rate
50%
He II
50%
Heat Conduction
50%
Hydrogen Density
50%
Instability Growth Rate
50%
Large-scale Structure of Universe
50%
Microwave Radiation
50%
Photon Density
100%
Photon number
50%
Pressure Effect
50%
Pressure Limit
50%
Radiation Attenuation
100%
Radiation Loss
50%
Radiation Trapping
100%
Recombination
100%
Resonance Line
100%
Resonant Radiation
50%
Resonant Scattering
50%
Viscosity Effect
100%
Viscous Limit
50%
Earth and Planetary Sciences
Conductive Heat Transfer
50%
Electromagnetic Radiation
50%
Large-Scale Structure of the Universe
50%
Microwave
50%
Photon Density
100%
Radiation Trapping
100%
Resonance Line
100%
Physics
Conductive Heat Transfer
50%
Electromagnetic Radiation
50%
Large-Scale Structure of the Universe
50%
Microwave
50%
Radiation Trapping
100%
Resonance Line
100%
Resonance Scattering
50%