Helios
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The QM degeneracy pressure puts up a fight but the immensity of the star wins out. Why is this? Is the Pauli Exclusion Principle really a principle? Why does it surrender in this case?
The Pauli exclusion principle never surrenders, all the principle says is that the electrons reach a ground state where they cannot lose any more heat. Losing heat is normally how a star gradually succumbs to gravity, but the PEP prevents that from proceeding to its ultimate conclusion. However, there is still a way that gravity can win out-- by releasing enough energy to make the electrons go relativistic before the whole system reaches its ground state. Relativistic electrons have a different relationship between momentum and kinetic energy, which makes them able to be in their ground state without uniquely specifying a radius-- any radius will do. This makes them susceptible to drastic contraction, especially if processes are going on (like neutronization) that remove kinetic energy via the escape of neutrinos. So we should not say the PEP surrenders, we should say that gravity finds a way to collapse the core without violating the PEP.Helios said:The QM degeneracy pressure puts up a fight but the immensity of the star wins out. Why is this? Is the Pauli Exclusion Principle really a principle? Why does it surrender in this case?