Simulating the Formation of Primordial Proto-Stars

Details Simulating the Formation of Primordial Proto-Stars Simulating the Formation of Primordial Proto-Stars

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990...21y&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 21-24 (2008).

Mathematics

Logic

Population Iii Stars, Cosmology, Star Formation, Numerical Simulation, Solution Of Equations, Hydrodynamics, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

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

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