Astrophysics - triple alpha core Temp

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SUMMARY

The discussion focuses on the triple alpha process in astrophysics, specifically addressing why stages 1 and 2 of this process commence only when a star's core temperature reaches approximately 10^8K. The equations involved are 4He + 4He = 8Be for step 1 and 8Be + 4He = 12C for step 2. Participants emphasize the role of gravitational potential energy in achieving the necessary conditions for helium fusion, which leads to the formation of beryllium and carbon. Understanding the relationship between core temperature and nuclear fusion processes is crucial for comprehending stellar evolution.

PREREQUISITES
  • Understanding of the triple alpha process in stellar nucleosynthesis
  • Familiarity with nuclear fusion equations and reactions
  • Knowledge of gravitational potential energy in astrophysical contexts
  • Basic concepts of stellar evolution and core temperature dynamics
NEXT STEPS
  • Research the conditions for helium fusion in stars post-hydrogen fusion
  • Study the role of gravitational potential energy in stellar core dynamics
  • Learn about the implications of core temperature on nuclear fusion rates
  • Explore the triple alpha process in detail, including energy calculations
USEFUL FOR

Astronomy students, astrophysicists, and educators seeking to deepen their understanding of stellar nucleosynthesis and the conditions required for helium fusion in stars.

supersam
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Homework Statement


Explain why stage 1 and 2 of the triple alpha process will not being until the core Temp of the star is around 10^8K.

Homework Equations



4He+4He = 8Be (step 1)
8Be+4He = 12C (Step 2)

The Attempt at a Solution



I "think" I need to work out the nuclear energies... However I am a little stuck on how to do this. This is a marked assignment so I'd appreciate a nudge in the right direction, rather than any form of a solution.

I have a suspicion that I need to use T^v, where v = (EG/4kT)^1/3 - 2/3; where EG is the gammon energy. However I would like just a heads up if this is the right idea.

Thanks
 
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supersam said:

Homework Statement


Explain why stage 1 and 2 of the triple alpha process will not being until the core Temp of the star is around 10^8K.

Homework Equations



4He+4He = 8Be (step 1)
8Be+4He = 12C (Step 2)

The Attempt at a Solution



I "think" I need to work out the nuclear energies... However I am a little stuck on how to do this. This is a marked assignment so I'd appreciate a nudge in the right direction, rather than any form of a solution.

I have a suspicion that I need to use T^v, where v = (EG/4kT)^1/3 - 2/3; where EG is the gammon energy. However I would like just a heads up if this is the right idea.

Thanks

Perhaps you should review some of the basics of the triple alpha reaction first before going down the rabbit hole:

http://en.wikipedia.org/wiki/Triple-alpha_process

It takes a while before a star with a hydrogen core eagerly fusing away accumulates enough helium to interfere with that reaction. And when hydrogen fusion is interrupted, what happens in the core?
 
Okay - looks like I might have been getting ahead of myself. So the Helium "burning" starts due to huge temperatures when the core of the star collapses. Which in turn creates Beryllium and then Carbon. However I am still not exactly sure how the 10^8K value is determined. I can understand that the energy comes from the Gravitational Potential energy - but how do you show that 10^8K is the magic number?
 
supersam said:
Okay - looks like I might have been getting ahead of myself. So the Helium "burning" starts due to huge temperatures when the core of the star collapses. Which in turn creates Beryllium and then Carbon. However I am still not exactly sure how the 10^8K value is determined. I can understand that the energy comes from the Gravitational Potential energy - but how do you show that 10^8K is the magic number?

Look at the conditions necessary for helium fusion to take place after hydrogen fusion is no longer able to support the core against collapse.

http://en.wikipedia.org/wiki/Helium_flash
 

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