Protostar formation in the early universe

Mathematics – Logic

Scientific paper

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Cosmology: Theory, Molecular Processes, Radiative Transfer

Scientific paper

We study the formation of primordial proto-stars in a ΛCDM universe using ultra high-resolution cosmological simulations. Our approach includes all the relevant atomic and molecular physics to follow the thermal evolution of a prestellar gas cloud to “stellar” densities. We describe the numerical implementation of the physics. We also show the result of a simulation of the formation of primordial stars in a reionized gas.

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