Astrophysics: Number of pp-reactions occuring in the Sun

In summary, the task is to calculate the number of proton-proton reactions that occur in the Sun each second, taking into account only the energy generation produced by the PPI chain. This can be done by considering the steady state energy production from the pp chain and using data such as temperature, density, and cross-sections. Another approach is to calculate the energy released per pp-reaction and take into account the energy lost due to radiation.
  • #1
kirstlen
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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.
 
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  • #2
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)?
 

FAQ: Astrophysics: Number of pp-reactions occuring in the Sun

What is the significance of the number of pp-reactions occurring in the Sun?

The pp-reactions, or proton-proton reactions, are the primary source of energy production in the Sun. These reactions involve the fusion of hydrogen atoms to form helium, releasing a large amount of energy in the process. The number of pp-reactions directly affects the amount of energy being produced by the Sun, which in turn affects its temperature, luminosity, and overall lifespan.

How many pp-reactions occur in the Sun per second?

It is estimated that approximately 3.86 x 10^38 pp-reactions occur in the Sun per second. This number may vary slightly depending on the current conditions of the Sun, such as its temperature and density.

What factors influence the number of pp-reactions in the Sun?

The number of pp-reactions in the Sun is primarily influenced by its temperature and density. Higher temperatures and densities will result in more frequent and energetic collisions between hydrogen atoms, increasing the rate of pp-reactions. Other factors such as the Sun's composition and magnetic fields may also play a role.

How does the number of pp-reactions in the Sun compare to other stars?

The number of pp-reactions in the Sun is relatively low compared to other stars. This is because the Sun is a relatively small and stable star, while larger and more massive stars have a higher rate of pp-reactions due to their stronger gravitational forces and higher temperatures.

Can we observe the number of pp-reactions in the Sun from Earth?

No, we cannot directly observe the number of pp-reactions occurring in the Sun from Earth. However, scientists can estimate this number by studying the Sun's energy output and using mathematical models and simulations to understand the processes happening within the Sun's core.

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