Power for a blackbody radiation

AI Thread Summary
The power emitted by a blackbody in equilibrium with its surrounding electromagnetic field is described by the equation P = cu/4, which relates to the energy density of the field. There is some confusion regarding the derivation of this equation, with references to issues in existing resources like Hyperphysics. The standard derivation found in texts, such as Reif's book, is noted to be clear and helpful. Additionally, the temperature of the blackbody significantly influences the power spectrum, as higher temperatures lead to increased radiated energy. Overall, understanding these relationships is crucial for grasping blackbody radiation concepts.
dEdt
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If a blackbody is in equilibrium with the surrounding electromagnetic field, the power emitted by the surface of the blackbody will be related to the energy density of the electromagnetic field by P=\frac{cu}{4}. Try as I might, I haven't found a good derivation for this equation (the Hyperphysics one has several problems). I thought that it shouldn't be too hard to derive, but playing with Poynting's theorem led me nowhere, so now I humbly turn to physicsforums for help.
 
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Wouldn't it also depend upon the temperature?
 
dEdt said:
Try as I might, I haven't found a good derivation for this equation (the Hyperphysics one has several problems).

What's wrong with the standard derivation in texts? See e.g. pp. 385-388 of Reif.

UltrafastPED said:
Wouldn't it also depend upon the temperature?

The usual temperature dependence of the blackbody power spectrum is contained in the expression for the energy density of the photon gas in the cavity.
 
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WannabeNewton said:
What's wrong with the standard derivation in texts? See e.g. pp. 385-388 of Reif.

I just checked Reif's book and found his derivation to be very clear. Thanks.
 
dEdt said:
I just checked Reif's book and found his derivation to be very clear. Thanks.

No problem! It's a brilliant gem of a book.
 
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