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Tagged with white-dwarf degenerate-matter
2 questions
8
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2
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Why does the Chandrasekhar limit affect white dwarfs differently?
The Chandrasekhar limit is the maximum mass of a stable white dwarf star. Beyond this, a carbon-oxygen white dwarf will typically explode in a type 1a supernova, due to the nuclear reactions at those ...
- 8,196
9
votes
2
answers
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Are white dwarf stars supported by proton degeneracy as well?
In general, fermions form a degenerate gas under high density or extremely low temperature. It's clear that white dwarf stars are supported by electron degeneracy pressure. However, there are still a ...
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