How do I solve this integral using partial integration?

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Discussion Overview

The discussion revolves around solving a specific integral related to the Stefan-Boltzmann law using partial integration and other methods. Participants explore various approaches to the integral, including substitutions and the use of infinite series, while addressing issues with LaTeX graphics and integration limits.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant expresses difficulty in integrating a function and seeks guidance on using partial integration.
  • Another suggests simplifying the problem by considering a different function, x/[e^x-1], or using infinite series as alternatives.
  • A participant identifies the integral as a Fermi integral and references its relation to the Riemann zeta function and gamma function.
  • Concerns are raised about the visibility of LaTeX graphics, which some participants are unable to view.
  • A participant recounts their professor's explanation of the integral in the context of deriving the Stefan-Boltzmann law, noting its complexity.
  • There is a discussion about the sign of a value obtained during substitution, with one participant questioning whether it should be positive.
  • Another participant clarifies the origin of a negative sign in a calculation related to the integral and discusses the importance of changing integration limits when making substitutions.
  • Participants engage in clarifying the integration limits when substituting variables, emphasizing the need to account for the direction of integration.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the best method to solve the integral, and multiple competing views and approaches remain throughout the discussion.

Contextual Notes

Some participants express uncertainty about the use of infinite series and the implications of changing integration limits, indicating a need for further clarification on these topics.

Who May Find This Useful

This discussion may be useful for students and individuals interested in advanced integration techniques, particularly in the context of physics and mathematical applications related to the Stefan-Boltzmann law.

P3X-018
"Simple" integral

Hey. I'm having problems with integrating the following function:

http://www.mainboard.dk/upload/files/Math.bmp

I used partial integration (if it's called that in english?), and end up with the same term. In equation (1.2) I just tried to integrate the middle term in (1.1), and as you can see it didn't work with parial integration. How do I then solve it?
By the way, I'm not on higher education, only in "senior high school". So it would best if you could show how you get to the solution.
 
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well you alreaedy beat me by integrating 1/(e^x-1) but axxording to my basic philosophy of "make the rpoblem easier" you might try just doing x/[e^x-1].

or use infinite series as a last resort.
 
No, I can't just do x/((e^x) -1)). I need the first value, in calculating stefan-boltzmanns law. But I don't know anything about integrating by use of the infinite series.
 
The integral is called a Fermi integral. Look up the general form, the solution is a product of the Riemann zeta function and the gamma function.

[tex]\int^{\inf} _{0} \frac{x^{n-1}}{e^{x} - 1} dx = \Gamma (n) \zeta (n)[/tex]
 
Why am I unable to see the latex graphic? It keeps saying: "LaTeX graphic is being generated. Reload this page in a moment."
And it's not helping by refreshing the page.
 
My phyiscs professor in my first year at the university derived the Stefan-Boltzmann law the same way you are trying to do from the Planck's BB radiation formula. He made the same substitution but on encountering the integral you mention he said "this is just the area undre a certain curve which can be shown to be [itex]\pi^4 / 15[/itex]". I guess it's quite a tricky integral...
 
Yea, I know it's 6,49 (pi^4/15). You can calculate the area, on the calculator, but I just wanted to know how you get to the solution. Well Dr Transport tells also how to solve it. But I can't see the latex graphic. Why? Is it because you've writin the command wrong?? Would you pls rewrite it again (not the last one, which is pi^4/15). I would appreciate that!
 
Now we are talking about the substitution, I got the value -2pi(kT)^4. but shouldn't it be with af positive sign??
 
I'm not sure what you mean, what value is that you got there?

The final answer is the intensity of the radiation is: [itex]I=\sigma T^4[/itex] (with [itex]\sigma[/itex] the stefan Boltzmann constant. This constant turns out to be not fundamental if you work everything out:

[tex]\sigma = \frac{2 k^4 \pi^5}{15 h^3 c^2}[/tex]

The easiest way is to substitute [itex]x= hc/ \lambda kT[/itex] when integrating Plancks law over all wavelengths (now x) to get the total intensity (Stefan-Boltzmann law).

Note: You can see the latex code if you click on the (nongenerated) latex image
 
  • #10
Yes I know that da willem (check the link at #1). But I mean that after the substitution i get a negative value. (See the attached document). Can you tell why I get a negativ value (-kT)?
Or is it supposed to be negativ?
 

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  • #11
You get the minus sign from the differential d(lambda)=-(hc/kT)x^-2 dx. But you forgot to cancel it with the minus introduced by changing your integration limits.
 
  • #12
The LateX graphics have had some trouble since the server switch the other day. If you look at what was written, the general formula has been given. The problem is being fixed.

dt
 
  • #13
Phew I was wondering about what was going wrong with the TeX--- I thought it was just something I was experiencing, nice to know that that is indeed not the case.
 
  • #14
Ok. I thougt the same as Theelectricchild, that it was only me who was experiencing that!

By the way "da willem" what do you mean by "changing the integration limits"? Where do you change it? I mean you can't just change them.
 
  • #15
You have to integrate the wavelength from 0 to infinity. You made the substitution x= hc/ (wavelength)kT. So when the wavelength goes from 0 to infinity, x goes from infinity to 0 (because of the inverse relation between x and the wavelength). So you have to change your integration limits from (from 0 to infinity) to (from infinity to zero). You evaluated the integral from 0 to infinity where you should have evaluated from infinity to zero...

Thisis allowed; but you have to take into account another minus sign which you forgot. Because:

[tex]\int _a^b f(t) dt = - \int _b^a f(t) dt[/tex]

Got it?
 
  • #16
Yea I got ya. Well, thanks for help :)
 
  • #17
let's try this again

[tex]\int^{\infty} _{0} \frac{x^{n-1}}{e^{x} - 1} dx = \Gamma (n) \zeta (n)[/tex]
 

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