Last Updated:2025/11/21

The stability of white dwarf stars is largely attributed to the Pauli exclusion principle.

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The stability of white dwarf stars is largely attributed to the Pauli exclusion principle.

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白色矮星の安定性は主に、同一のフェルミオンが同じ量子状態を同時に占有できないとするパウリの排他原理に起因しています。

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