Change of variables in Planck's radiation integral

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So i don't really know where to paste this.

I'm reading a example in my modern physics book and i don't understand what they did.

[tex]\int[/tex] (2(pi)hc2)/([tex]\lambda[/tex]5(ehc/[tex]\lambda[/tex]kT-1))d[tex]\lambda[/tex]

if we make the change of variable x=hc/[tex]\lambda[/tex]kT

(2(pi)k4T4)/(c2h3)[tex]\int[/tex]((x3)/(ex-1))dx

so how did they get to this:

(2(pi)k4T4)/(c2h3)[tex]\int[/tex]((x3)/(ex-1))dx

when I solve for [tex]\lambda[/tex] in x=hc/[tex]\lambda[/tex]kT and plug it into the first ingetral I get:

(2(pi)x5k5T5)/(h4c3)

basically, I'm off by 1 power for everything except for x (that I'm off by 2).

can someone explain this?
 
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phyguy321 said:
So i don't really know where to paste this.

I'm reading a example in my modern physics book and i don't understand what they did.

[tex]\int[/tex] (2(pi)hc2)/([tex]\lambda[/tex]5(ehc/[tex]\lambda[/tex]kT-1))d[tex]\lambda[/tex]
That's
[tex]\int \frac{2\pi hc^2}{\lambda^5 e^{\frac{hc}{\lambda}kT^{-1}-1} d\lambda[/tex]?

if we make the change of variable x=hc/[tex]\lambda[/tex]kT

(2(pi)k4T4)/(c2h3)[tex]\int[/tex]((x3)/(ex-1))dx

so how did they get to this:

(2(pi)k4T4)/(c2h3)[tex]\int[/tex]((x3)/(ex-1))dx

when I solve for [tex]\lambda[/tex] in x=hc/[tex]\lambda[/tex]kT and plug it into the first ingetral I get:

(2(pi)x5k5T5)/(h4c3)

basically, I'm off by 1 power for everything except for x (that I'm off by 2).

can someone explain this?
Did you forget to replace "[itex]d\lambda[/itex]" as well?
[tex]x= \frac{hc}{kT}\lambda^{-1}[/tex]
so [tex]dx= -\frac{hc}{kT}\lambda^{-2}d\lambda[/tex]
Solving that for [itex]d\lambda[/itex],
[tex]d\lambda= -\frac{kT}{hc}\lambda^2 dx[/itex]<br /> and since [itex]\lambda= (hc)/(kT) x^{-1}[/itex], [itex]\lambda^2= (h^2c^2)/(k^2T^2) x^{-2}[/itex] giving<br /> [tex]d\lambda= \frac{hc}{kT}x^{-2}dx[/tex].[/tex]