The Origin of Stellar Energy by Professor G Srinivasan

The Origin of Stellar Energy by Professor G Srinivasan

International Centre for Theoretical Sciences via YouTube Direct link

Summer course 2018 - A Random walk in astro-physics

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Summer course 2018 - A Random walk in astro-physics

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The Origin of Stellar Energy by Professor G Srinivasan

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  1. 1 Summer course 2018 - A Random walk in astro-physics
  2. 2 The Origin of Stellar Energy Lecture-08
  3. 3 What are the stars?
  4. 4 Stars as globes of perfect gas
  5. 5 Hydrostatic Equilibrium
  6. 6 Boyle's Law
  7. 7 Equation of Hydrostatic Equilibrium
  8. 8 Stars are globes of gas in which the inward pull of gravity is balanced by the combined effect of the pressure of an ideal gas and the pressure of radiation.
  9. 9 Eddington's theory of stars
  10. 10 Radiation Pressure
  11. 11 Hydrostatic Equilibrium
  12. 12 Why do the stars shine?
  13. 13 Why does the Sun shine?
  14. 14 Virial Theorem applied to the Sun
  15. 15 How long will the heat last?
  16. 16 Sir Arthur Eddington
  17. 17 Mass Deficit
  18. 18 Proton - proton collision
  19. 19 Maxwell-Boltzmann Distribution
  20. 20 Quantum Tunnelling
  21. 21 Energy production in the Sun
  22. 22 proton - proton reaction
  23. 23 Nuclear cycles
  24. 24 To burn or not to burn? That is the question
  25. 25 Coulomb barrier
  26. 26 Fusion reactions
  27. 27 Onion skin model of a star
  28. 28 The composition of the core when nuclear reactions finally stop
  29. 29 Lifetime of stars
  30. 30 Why doesn't the Sun blow up?
  31. 31 The Safety Valve
  32. 32 Q&A

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