Astrophysics: Number of pp-reactions occuring in the Sun

Click For Summary
SUMMARY

The discussion focuses on calculating the number of proton-proton (pp) reactions occurring in the Sun each second, specifically within the context of the proton-proton chain (PPI chain). The relevant equation for determining the reaction rate is given as \(\frac{N_{ix}}{\Delta t} = n_{i}σv\), where \(n_{i}\) represents the number density of protons, \(σ\) is the cross-section, and \(v\) is the relative velocity of the particles. Participants emphasize the need for data on the Sun's temperature and density, as well as the energy released per pp-reaction, to accurately compute the reaction rate.

PREREQUISITES
  • Understanding of the proton-proton chain (PPI chain) in stellar physics
  • Familiarity with the equation \(\frac{N_{ix}}{\Delta t} = n_{i}σv\)
  • Knowledge of cross-section concepts in nuclear reactions
  • Basic principles of thermodynamics as they apply to stellar energy generation
NEXT STEPS
  • Research the energy output of the proton-proton chain reactions in the Sun
  • Learn about the calculation of cross-sections in nuclear physics
  • Investigate the temperature and density profiles of the Sun
  • Explore the concept of steady state in astrophysical contexts
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in stellar processes and energy generation mechanisms in stars, particularly those studying the Sun's nuclear reactions.

kirstlen
Messages
3
Reaction score
0

Homework Statement


Calculate the number of proton-proton reactions that occur in the Sun each second. For simplicity consider only the energy generation produced by the PPI chain. Consider that the Sun produces its energy in a steady state from the pp chain.


Homework Equations


4H[itex]\rightarrow[/itex]He+2e[itex]^{+}[/itex]+2[itex]\nu_{e}[/itex]+2[itex]\gamma[/itex]
[itex]\frac{N_{ix}}{\Delta t}[/itex] = n[itex]_{i}[/itex]σv <-- this equation was given in class as the reactions per time.


The Attempt at a Solution


I'm pretty sure you need to use the equation that was given in class however I'm not sure. The textbook gives that σ [itex]\propto[/itex] 1/E so would it help to find the energy produced in the PPI chain to find σ? As for n[itex]_{i}[/itex] and v I'm not sure what those are or how to find them.
 
Physics news on Phys.org
What you wrote is the sum of multiple reactions, not a single reaction, so it does not have a well-defined cross-section.

You need some data about the sun. One option is the microscopic way - find temperature, density, cross-sections and so on, and calculate the rate. I don't think you are supposed to do that, however. There is also the macroscopic way, where "steady state" comes into play: how much energy does the sun lose due to radiation? What is the energy released per pp-reaction (including follow-up reactions, but excluding neutrinos)?
 

Similar threads

  • · Replies 49 ·
2
Replies
49
Views
6K
Replies
1
Views
4K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 54 ·
2
Replies
54
Views
11K
Replies
3
Views
2K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 35 ·
2
Replies
35
Views
5K
Replies
1
Views
2K
  • · Replies 6 ·
Replies
6
Views
1K
Replies
1
Views
2K