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Hayakawa, T · 2024 · DOI 10.1093/mnras/stae302

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Cosmic-Ray Spectra and Metal Budget Regulated by the Galactic Wind

astro-ph.HE · 2026-02-18 · unverdicted · novelty 4.0

Galactic wind advection with a peak velocity of ~700 km/s reproduces cosmic ray spectral hardening from hundreds of GV and softening from a few TV without diffusion breaks, predicts a hard spectrum (index ~2) at 3-5 kpc altitudes consistent with Fermi bubbles, and shows the wind maintains disk metal

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  • Cosmic-Ray Spectra and Metal Budget Regulated by the Galactic Wind astro-ph.HE · 2026-02-18 · unverdicted · none · ref 32

    Galactic wind advection with a peak velocity of ~700 km/s reproduces cosmic ray spectral hardening from hundreds of GV and softening from a few TV without diffusion breaks, predicts a hard spectrum (index ~2) at 3-5 kpc altitudes consistent with Fermi bubbles, and shows the wind maintains disk metal