The Beginning of Homogeneous Nucleation of Iron/Nickel Cores in Homogeneous Young Stars

Authors: Jeffrey Joseph Wolynski

To begin the process of forming homogeneous iron/nickel cores it is required that the young, hot stars be homogeneous in their interiors. To form an iron/nickel core as the star evolves, no nuclear core can be present. It would be too hot for the iron/nickel vapor to clump together and it would get in the way of the differentiation process.

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[v1] 2017-04-13 22:15:25

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