Solve Stellar Structure with Lane-Emden Equation

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SUMMARY

The Lane-Emden equation (LEE) is applicable in the context of the Standard Solar Model (SSM) for studying stellar structure. The equation integrates Newtonian gravity with the ideal gas law, utilizing the polytropic index to connect pressure and density. Different polytropic indices yield various solutions known as polytropes, which are essential for modeling the stratified layers within stars. The Sun's structure includes a convection zone with a polytropic index of 3/2 and a radiation zone with an index of 3, highlighting the complexity of stellar modeling.

PREREQUISITES
  • Understanding of the Lane-Emden equation
  • Familiarity with polytropic indices
  • Knowledge of Newtonian gravity
  • Basic principles of the ideal gas law
NEXT STEPS
  • Study the derivation of the Lane-Emden equation
  • Explore the concept of polytropes in stellar modeling
  • Investigate the Standard Solar Model (SSM) in detail
  • Learn about the stratification of stellar interiors
USEFUL FOR

Astronomy students, astrophysicists, and researchers focused on stellar structure and modeling will benefit from this discussion.

wasi-uz-zaman
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HI, I have a question can Lane-Emden equation be use in SSM( standard stellar model) and overall for the study of stellar structure in todays latest research.
thanks
HI, I have a question can Lane-Emden equation be use in SSM( standard stellar model) and overall for the study of stellar structure in todays latest research.
thanks
 
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SSM is the standard solar model not the standard stellar model. How could there be a standard stellar model if there are so many different kinds of stars?
The Lane-Emden equation is an equation that merges Newtonian gravity with the ideal gas law. It is instructive to study its derivation. The critical parameter is called the polytropic index, used to relate pressure to density. For different polytropic indices, we get solutions to LEE called polytropes. A simple star model would assume a single index throughout the star, however the innards of stars are usually stratified into layers with different indices, so we have to create a composite polytrope, and graft different polytropes together smoothly. The Sun has a convection zone ( index = 3/2 ) and a radiation zone ( index = 3 ). The polytropic index is half the degrees of freedom of the substance.
The SSM is likely very complicated but the LEE is within the grasp of a college physics student.
 
Thanks a lot , it indeed clear my query to a great extent.
 

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