Confused - nucleosynthesis of carbon

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Discussion Overview

The discussion revolves around the nucleosynthesis of carbon and oxygen, focusing on the energy states of these elements during fusion processes. Participants explore the conditions under which carbon is produced rapidly compared to the slower production of oxygen, examining the implications of energy levels and conservation laws in nuclear reactions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant notes that carbon nucleosynthesis is rapid because one of its excited state energies is slightly higher than the total energy of beryllium (Be) and helium (He), allowing the necessary energy to be obtained from their kinetic energy.
  • Another participant questions why oxygen production is slower, suggesting that oxygen could eliminate excess energy through increased kinetic motion or particle ejection, but acknowledges this may conflict with energy and momentum conservation.
  • A third participant references Sir Martin Rees, explaining that when two nuclei collide, the resulting nucleus must occupy specific energy states, and if the combined energy is not appropriate, the nuclei may not fuse and could instead bounce off each other.
  • One participant emphasizes that in the center of mass frame of the collision, nuclei have well-defined allowed energy values, and fusion is unlikely if the total energy does not match these values.
  • Another participant confirms that oxygen, which has slightly less mass/energy than the total mass/energy of beryllium and helium, can form through processes like photon emission, but these processes are infrequent.
  • Another participant discusses the importance of proton binding in fusion, indicating that more protons bound results in more energy released.

Areas of Agreement / Disagreement

Participants express differing views on the mechanisms and conditions affecting the rates of carbon and oxygen production, indicating that multiple competing perspectives remain without consensus on the specifics of the processes involved.

Contextual Notes

Participants highlight the complexity of energy states and conservation laws in nuclear fusion, noting that certain assumptions about energy levels and the likelihood of fusion events are not fully resolved.

Who May Find This Useful

This discussion may be of interest to those studying nuclear physics, astrophysics, or anyone curious about the processes of nucleosynthesis and the conditions affecting elemental formation in stars.

thatoekhant
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Confused -- nucleosynthesis of carbon

May I ask a question please! I read that nucleosynthesis of carbon was rapid because its one of the excited state energies was only a little higher than the total energy of Be and He. So, the required energy could be obtained through the kinetic energy of Be and He.

But, as for oxygen, its one of the excited state energies was a little lower than the total energy of C and He. So, this stage was not as rapid as carbon production stage. So, all of carbons didn't convert to oxygen.

I don't understand why oxygen production rate is slow because I think ( maybe I'm wrong) oxygen that carried the total energy of C and He plus their kinetic energy could eliminate the extra energy in the form of own more rapid motion ( kinetic energy) or particle ejection from nucleus to regain its excited state.

Oxygen's Excited energy state that was a little lower than total energy of C and Be is a problem .
But, carbon's Excited energy state that was a little higher than the total energy of Be and He is not a problem. Why ?
 
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thatoekhant said:
I don't understand why oxygen production rate is slow because I think ( maybe I'm wrong) oxygen that carried the total energy of C and He plus their kinetic energy could eliminate the extra energy in the form of own more rapid motion ( kinetic energy) or particle ejection from nucleus to regain its excited state.
This does not work with energy and momentum conservation. Just view the reaction in the rest frame of the oxygen to see why.

But, carbon's Excited energy state that was a little higher than the total energy of Be and He is not a problem. Why ?
In the rest frame of the system (=the frame of the target nucleus), the initial nuclei will always have a positive kinetic energy.
 
According to Sir Martin Rees, ""Resonance works like this. When two nuclei collide and stick together, new nucleus that is formed carries the combined mass-energy of two nuclei, plus the combined energy of their motion, their kinetic energ (and minus a small amount of energy from the strong force, the binding energy that holds the new nucleus together). The new nucleus "wants" to occupy one of the steps on its own energy ladder, and if this combined energy from the incoming particles is not just right then the excess has to be eliminated, int he form of leftover kinetic energy, or as a particle ejected from the nucleus. This reduces the likelihood that the two colliding nuclei will stick together; in many cases, they simply bounce off each other and continue to lead their separate lives."

A dummy like me can't understand the relationship between the bold words and underlined words.
 
In the center of mass frame of the collision: Nuclei cannot exist with arbitrary energies, they just have very well-defined allowed energy values. If your total energy of the collision is not one of the allowed values (with some small range -> uncertainty principle), there is "no"* way for the two nuclei to fuse to a single nucleus. For light nuclei, if they cannot fuse to a single nucleus, they will just bounce off as described in the text.

*it is still possible via other processes (like a direct emission of a photon), but then it is much less likely.
 
You mean that oxygen that has a little less mass/energy than total mass/energy of beryllium and helium can form through some processes like emission of a photon , but it is not frequent , do you ?
 
Thanks a lot, mfb. You make my confusion clear :D
 
look at the protons, fusion is all about proton binding - more protons bounded, more energy released. The disassembled atoms give up their binding energy in favor of a lower energy state.
 

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