Including radiative transfer, cosmic rays, and magnetic fields in ~20 pc cosmological zoom simulations makes star formation burstier and reproduces JWST-era UV luminosity functions from z≈14 to z≈3 without calibrating the non-thermal model to those data.
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The Azahar Project: Non-Thermal Physics Drives Star Formation Burstiness and the Evolution of the UV Luminosity Density at Cosmic Dawn
Including radiative transfer, cosmic rays, and magnetic fields in ~20 pc cosmological zoom simulations makes star formation burstier and reproduces JWST-era UV luminosity functions from z≈14 to z≈3 without calibrating the non-thermal model to those data.