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courses:ast402:stellar-structure

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courses:ast402:stellar-structure [2026/06/07 22:07] shuvocourses:ast402:stellar-structure [2026/06/07 22:08] (current) – [Stellar Models and Simulation] shuvo
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 ===== Stellar Models and Simulation ===== ===== Stellar Models and Simulation =====
  
-Stellar models are constructed by numerically solving the four fundamental differential equations (hydrostatic equilibrium, mass conservation, energy generation, and energy transport). +Stellar models are constructed by numerically solving the four fundamental differential equations (hydrostatic equilibrium, mass conservation, energy generation, and energy transport). \\ 
 **Numerical Modeling:** The star is divided into **concentric shells (zones)**, and differential equations are replaced by **difference equations**. Solutions require matching **boundary conditions** at the center ($M_r \to 0, L_r \to 0$) and surface ($P \to 0, T \to 0$).\\ **Numerical Modeling:** The star is divided into **concentric shells (zones)**, and differential equations are replaced by **difference equations**. Solutions require matching **boundary conditions** at the center ($M_r \to 0, L_r \to 0$) and surface ($P \to 0, T \to 0$).\\
  
courses/ast402/stellar-structure.txt · Last modified: by shuvo

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