Use Saha-Boltzmann statistics to get the relative number densities

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The discussion centers on the application of the Saha equation in calculating electron pressure and number densities. It highlights the challenge of determining electron density (n_e), which is necessary for calculating the electron pressure (P_e). The relationship P_e = n_e kT is emphasized, indicating that both n_e and P_e are interdependent yet initially unknown. Participants seek clarification on how to derive or estimate n_e to effectively use the Saha equation. Understanding these relationships is crucial for accurate calculations in astrophysical contexts.
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Homework Statement
Use Saha-Boltzmann statistics to get an idea of the relative number densities of H, H+, H−, and H(n = 3).
Gather information from Gray’s book concerning the partition functions (hint: with its two electrons H−
is He-like; H+ is a naked proton, so U(p) = 1), the electron pressure, and so on. Assume T = 5772 K
(S 0 = 1, as Gray labels it in the relevant plots) and solar surface gravity. Take care with the units!
· What do you learn from comparing N(H−) and N(H, n = 3)?
Relevant Equations
The Saha equation N_i+1/N_i
for i:s energy levels.
When I am using the Saha equation, how i am suppose to know the electron pressure?
Which are required to calculate the ration?
Since: P_e = n_ekT (electron pressure and n_e is related to each other, but n_e is also unknown based on my understanding).
 
I want to find the solution to the integral ##\theta = \int_0^{\theta}\frac{du}{\sqrt{(c-u^2 +2u^3)}}## I can see that ##\frac{d^2u}{d\theta^2} = A +Bu+Cu^2## is a Weierstrass elliptic function, which can be generated from ##\Large(\normalsize\frac{du}{d\theta}\Large)\normalsize^2 = c-u^2 +2u^3## (A = 0, B=-1, C=3) So does this make my integral an elliptic integral? I haven't been able to find a table of integrals anywhere which contains an integral of this form so I'm a bit stuck. TerryW

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