On the Initial Mass Function of Population III Stars

@inproceedings{Nakamura2001OnTI,
  title={On the Initial Mass Function of Population III Stars},
  author={Fumitaka Nakamura and Masayuki Umemura},
  year={2001}
}
The collapse and fragmentation of filamentary primordial gas clouds are explored using onedimensional and two-dimensional hydrodynamical simulations coupled with the nonequilibrium processes of hydrogen molecule formation. The cloud evolution is computed from the initial central density nc = 10 − 10 cm. The simulations show that depending upon the initial density, there are two occasions for the fragmentation of primordial filaments. If a filament has relatively low initial density such as nc… CONTINUE READING

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