I Determining Degenerate Gas in Stellar Structure

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Determining whether a gas in a star is degenerate involves assessing if the electron degeneracy pressure is exceeded at zero temperature. This assessment relies solely on the concentration of electrons present in the gas. If the electron concentration is high enough, the gas is classified as degenerate. Understanding this distinction is crucial for accurate modeling of stellar structure and equations of state. Accurate identification of degenerate gas influences the behavior and evolution of stars.
Haynes Kwon
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When modeling stellar structure and formulating equation of states, I've seen various cases where you have to take into account whether the constituent gas of a star is degenerate or not. But how do you determine if the gas is degenerate or not?
 
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Haynes Kwon said:
When modeling stellar structure and formulating equation of states, I've seen various cases where you have to take into account whether the constituent gas of a star is degenerate or not. But how do you determine if the gas is degenerate or not?
Simplest check is whenever "electron degeneracy pressure" at zero temperature is exceeded or not. It depends only on electrons concentration.
 
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