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About Introduction To Astrophysics Tutorial 2: Polytropic Models: 1 Summary of The Equations of Stellar Structure
1. The document introduces polytropic models, which use a power-law equation of state to model stellar structure and solve the equations of hydrostatic equilibrium. 2. A polytropic equation of state takes the form P = Kργ, which allows the structure equations to be transformed into the Lane-Emden equation. 3. The Lane-Emden equation depends on the polytropic index n and has analytical solutions for n = 0, 1, 5. It can be used to determine properties like the stellar radius and mass.
Detailed Information
| Author: | ['عمر الفاروق عبيدية'] |
|---|---|
| Publication Year: | 2020 |
| Pages: | 6 |
| Language: | English |
| Format: | |
| Price: | FREE |
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