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un:heat-transfer-in-stars

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un:heat-transfer-in-stars [2025/10/27 00:23] asadun:heat-transfer-in-stars [2025/10/27 00:23] (current) asad
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 $$ $$
  
-where \(\kappa\) is the [[uv:opcaity|opacity]] in m\(^2\) kg\(^{-1}\), the effective cross-section for absorption and scattering per unit mass.  +where \(\kappa\) is the [[opacity]] in m\(^2\) kg\(^{-1}\), the effective cross-section for absorption and scattering per unit mass.  
 Opacity represents the resistance of the medium to the flow of radiation — the larger the opacity, the shorter the mean free path. Opacity represents the resistance of the medium to the flow of radiation — the larger the opacity, the shorter the mean free path.
  
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