The weak force and effective coupling

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SUMMARY

The discussion centers on the weak force and its effective coupling in the context of the pp cycle, specifically the reaction p + p -> d + e^+ + v_e, where a positron and an electron neutrino are produced. It is established that weak interactions can occur at low energies, such as the 1.5 x 10^7 K found in the Sun's core, despite the effective coupling being small. The conversation highlights that while weak interactions are most effective near the mass shell of the W and Z bosons (approximately 80 GeV and 90 GeV respectively), they can still proceed at lower energy levels without leading to nucleon fragmentation, which is crucial for deuterium formation.

PREREQUISITES
  • Understanding of weak interactions and their role in nuclear reactions
  • Familiarity with the pp cycle in stellar nucleosynthesis
  • Knowledge of particle physics, specifically W and Z bosons
  • Basic thermodynamics related to stellar core temperatures
NEXT STEPS
  • Study the properties and interactions of W and Z bosons in particle physics
  • Research the role of weak interactions in stellar nucleosynthesis
  • Explore the implications of low energy limits on particle interactions
  • Investigate the dynamics of the pp cycle and its significance in stellar evolution
USEFUL FOR

Physicists, astrophysicists, and students of particle physics interested in the mechanisms of nuclear reactions and the role of weak interactions in stellar processes.

ian2012
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I just read something about the creation of deuteron in the first step of the pp cycle. Given that you have the reaction: p + p -> d + e^+ + v_e, where e^+ is a positron and v_e is an electron neutrino. Since there is a neutrino present, it is a weak interaction. In addition, as the interaction is weak (and at low energies?) the effective coupling is small.

My question is, do weak interactions only proceed at low energies? I have read about 'low energy limits' and how this means only virtual W's can be made. How is it then that this process can proceed at roughly 1.5 x 10^7 K in the Sun's core?
 
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Weak interactions in generally occur most readily at energies where the intermediate gauge boson is very close to its mass shell (about 80 GeV for the W and 90 GeV for the Z). However, at that kind of energy the nucleons involved tend to fragment, so you wouldn't get deuterium.

Also, not that 1.5 x 10^7 K does not get you to terribly high energy. It only amounts to an avererage of 1.3 keV kinetic energy per proton, which is, as these things go, rather low energy. (Remember, the electron's mass is 511 keV and the proton's is 938 MeV.)
 
Okay then, so weak interactions don't really proceed at low energies? (i am not too sure what the ideal energies are for strong interactions).
 

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