A Full-Physics galaxy formation model with radiative transfer, cosmic rays, and magnetic fields reproduces JWST-observed compact, self-regulated galaxy sizes at z=3–12, while HD and HD-Boost models are respectively too compact and too extended.
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Non-Thermal Physics Drives Compact, Self-Regulated Galaxy Morphologies at Cosmic Dawn
A Full-Physics galaxy formation model with radiative transfer, cosmic rays, and magnetic fields reproduces JWST-observed compact, self-regulated galaxy sizes at z=3–12, while HD and HD-Boost models are respectively too compact and too extended.