Stefan-Boltzman law derivation and integral tricks

In summary, the conversation was about trying to derive the Stefan-Boltzmann law from Planck's formula and getting stuck with an integral. The speaker asked for help in solving the integral, which involved a summation. They were given guidance on how to evaluate the integral and summation, which ultimately led to the value of $\pi^4/15$ for the original integral.
  • #1
clumps tim
39
0
HI people,

I was trying to derive the stefan-boltzman law from the planc's formula, I kind of got stuck with an integral
$$ \int_{0}^{\infty} \frac{x^3}{e^x -1} dx $$

I tried simplifying it with

$$ \int_{0}^{\infty} x^3 e^{-x} \sum_{n=0}^{\infty} e^{-nx} dx $$

Now I don't know what to do with the summation. I could evaluate

$$ \int_{0}^{\infty} x^3 e^{-x} dx = 6$$

pleas help me to get the rest of it, I see the answer comes with $\pi$, how do I get it in this kind of equation? Is there any special trick to solve these type of integrals?
thanks in advance.
 
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  • #2
cooper607 said:
HI people,

I was trying to derive the stefan-boltzman law from the planc's formula, I kind of got stuck with an integral
$$ \int_{0}^{\infty} \frac{x^3}{e^x -1} dx $$

I tried simplifying it with

$$ \int_{0}^{\infty} x^3 e^{-x} \sum_{n=0}^{\infty} e^{-nx} dx $$

Now I don't know what to do with the summation. I could evaluate

$$ \int_{0}^{\infty} x^3 e^{-x} dx = 6$$

pleas help me to get the rest of it, I see the answer comes with $\pi$, how do I get it in this kind of equation? Is there any special trick to solve these type of integrals?
thanks in advance.
You are on the right lines. Write the integral as \(\displaystyle \int_{0}^{\infty} x^3 \sum_{n=1}^{\infty} e^{-nx} dx\). Now take the sum outside the integral (which is justified because the negative exponential makes everything converge rapidly), to get \(\displaystyle \sum_{n=1}^{\infty}\int_{0}^{\infty} x^3 e^{-nx} dx\). The integral \(\displaystyle \int_{0}^{\infty} x^3 e^{-nx} dx\) can be evaluated by integrating by parts three times, giving the answer $\dfrac6{n^4}.$ Therefore \(\displaystyle \int_{0}^{\infty} \frac{x^3}{e^x -1} dx = \sum_{n=1}^\infty \dfrac6{n^4}.\) Finally, \(\displaystyle \sum_{n=1}^\infty \dfrac1{n^4}\) is a well-known series, with sum $\dfrac{\pi^4}{90}.$ So the value of your integral is $\dfrac{\pi^4}{15}$ unless I have made a mistake.
 
  • #3
Ah great, thank you very much, I almost got it on the track now, this is

$$ \int_{0}^{\infty} x^3 e^{-(n+1)x} dx = 6 (n+1)^{-4}$$

can you just tell me a little about how to evaluate the summation of $$\sum \frac{1}{(n+1)^4}$$ though, I think I forgot this evaluation.

thanks in advance
 
  • #4
cooper607 said:
can you just tell me a little about how to evaluate the summation of $$\sum \frac{1}{(n+1)^4}$$ though, I think I forgot this evaluation.
Probably the simplest way is to use Parseval's theorem from Fourier theory. See here, for example.
 

FAQ: Stefan-Boltzman law derivation and integral tricks

What is the Stefan-Boltzman law and why is it important?

The Stefan-Boltzman law is a physical law that describes the relationship between the temperature and the total energy radiated by a blackbody. It is important because it provides a fundamental understanding of how objects emit and absorb thermal radiation, which has many practical applications in fields such as astrophysics, engineering, and materials science.

How is the Stefan-Boltzman law derived?

The Stefan-Boltzman law can be derived using the principles of thermodynamics and electromagnetic theory. Specifically, it can be derived by considering a small cavity containing a blackbody and applying the laws of thermodynamics to determine its equilibrium state. This derivation involves solving differential equations and applying mathematical techniques such as integration and differentiation.

What are some integral tricks used in the derivation of the Stefan-Boltzman law?

One integral trick commonly used in the derivation of the Stefan-Boltzman law is the substitution method, which involves substituting a new variable in place of the original variable in an integral to simplify the calculation. Another integral trick is the use of trigonometric identities, which can help to simplify complex integrals involving trigonometric functions.

Can the Stefan-Boltzman law be applied to non-blackbody objects?

Yes, the Stefan-Boltzman law can be applied to non-blackbody objects by using an emissivity factor, which accounts for how well an object emits thermal radiation compared to a perfect blackbody. This factor can range from 0 to 1, with 0 representing a perfect reflector and 1 representing a perfect emitter.

What are some real-world examples of the Stefan-Boltzman law in action?

The Stefan-Boltzman law has many practical applications, including in the design of solar panels, thermal imaging cameras, and temperature sensors. It is also used in astrophysics to calculate the energy output of stars and planets. Additionally, the law can be applied in industries such as metallurgy and glass manufacturing to control and optimize thermal radiation processes.

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