Power radiated through a hole in small wavelength distribution

In summary, the power radiated through the hole is σT^4. This is because the cavity approximates a blackbody and the radiation is coming out of the hole.
  • #1
PsychonautQQ
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Homework Statement


A cavity at Temperature 6000k has an energy distribution corresponding to a blackbody. We make a small hole in it 1mm in diameter.

Calculate the power radiated through the hole of wavelength interval between 550nm and 551nm.
HINT: when dλ is small (such in this case), certain assumptions can be made regarding λ and a product can be used to approximate an integral

2. Cool Equation that's probably useful:
u(λ)= 8*pi*h*c*(λ^-5)*(e^(hc/λkt)-1)^(-1)

λT = 2.898*10^-3 maybe this will be useful? (wiens shiznit)

R=σT^4

The Attempt at a Solution


Hope someone is smart out there :X hah.

Alright so first of all I'm having some conceptual problems with this... the power radiated THROUGH the hole isn't dependent on the overall surface area of the cavity? It seems it's not as it gave us no information about the size or shape of the cavity.. so that's a bit offputting from the start...

So the total power radiated from the cavity is σT^4, because the cavity approximates a blackbody. But how much is radiated through the HOLE at that wavelength? any guidance?
 
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  • #2
You can imagine the hole as being the sole source of radiation. Looking at a hole in a 5800K cavity is no different than looking at the 5800K Sun. It looks like your cool equation is for power per unit surface area per unit of wavelength. How can you find power per unit surface area?
 
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  • #3
ahh I was thinking about the radiation being radiated OUT of the hole.. into it! duh.. thanks man :D.

By sureface area you just mean the area of the hole? No information is given on the surface area of the cavity.. thanks again dood
 
  • #4
The radiation is coming out of the hole. It doesn't matter how big the cavity is, the radiation can only escape through the hole. So yes, I mean the surface area of the hole.
 
  • #5
can radiation not strike the atoms making the cavity of the wall, increasing their temperature and then radiate away NOT through the hole as thermal power?

So what I have done so far is I have
u(λ)dλ = (8*pi*hc*λ^(-5) * dλ ) / (e^(hc/λkT)-1)
where I put λ = 550.5 since that's between 550 and 551.
I put λ as 1 nm and the rest are constants or given information.
So I can get a numerical value for this equation, which gives me the energy density inside the cavity for the wavelength's between 550 and 551.

Any tips as what do to from here?
 
  • #6
To find the power radiated would I take through the hole R(lambda) = c/4 * u(lambda)? I feel like I would have to add information about the radius of the hole somewhere right? Would R(Lambda) = c/4 * u(lambda) the total power?
 

What is power radiated through a hole in small wavelength distribution?

Power radiated through a hole in small wavelength distribution refers to the amount of energy that is emitted from a source through a small opening at a specific range of wavelengths. This phenomenon is commonly observed in electromagnetic radiation, where the size of the opening is comparable to the wavelength of the radiation being emitted.

How is power radiated through a hole in small wavelength distribution calculated?

The power radiated through a hole in small wavelength distribution can be calculated using the formula P = A * (4π/λ) * I, where P is the power, A is the area of the opening, λ is the wavelength of the radiation, and I is the intensity of the emitted radiation.

What factors affect the power radiated through a hole in small wavelength distribution?

The power radiated through a hole in small wavelength distribution is affected by the size of the opening, the wavelength of the radiation, and the intensity of the radiation. Other factors that may also influence this phenomenon include the material and shape of the opening, as well as any obstructions in the path of the radiation.

How does the power radiated through a hole in small wavelength distribution relate to the inverse square law?

The power radiated through a hole in small wavelength distribution follows the inverse square law, which states that the intensity of radiation at a certain distance from a source is inversely proportional to the square of the distance. This means that the further the distance from the source, the lower the intensity of the radiation.

What are some real-life applications of power radiated through a hole in small wavelength distribution?

One of the most common real-life applications of power radiated through a hole in small wavelength distribution is in radio wave transmission. Antennas with small openings are used to emit radio waves at specific wavelengths, allowing for efficient and targeted communication. This phenomenon is also utilized in astronomy, where telescopes with small openings can capture and analyze specific wavelengths of electromagnetic radiation from distant objects in space.

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