An analytical model bridges cosmological to protostellar scales for Population III stars, showing halo-scale star formation efficiency varies from 10^{-3} to 0.5 depending on halo properties and dissociating radiation.
(A13) in the left hand side, and substituting Eq
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Towards A Universal Analytical Model of Population III Star Formation: A Bridge Between Cosmological Scales and Protostars
An analytical model bridges cosmological to protostellar scales for Population III stars, showing halo-scale star formation efficiency varies from 10^{-3} to 0.5 depending on halo properties and dissociating radiation.