How Is Lambda Max Derived from Planck's Law?

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In summary, to find the maximum wavelength (Lambda_max) for a given temperature (T), you need to find the maximum of a function by setting its derivative equal to 0. The derivative is calculated using Planck's radiation formula for energy density per unit wavelength. However, there is no analytical solution and the equation must be solved numerically. An alternative is to first solve for Lambda_max*T and then find Lambda_max.
  • #1
georgeh
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I have a problem that states
Show that the wavelength Lamba_max=(2892 micro meters*K)/T
hint: set the dS/DLamba=0.
i have no idea how to do this.
 
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  • #2
You need to find the maximum of a function. The maximum of a function is given when f'(x) = 0. So taking Planck's radiation formula for energy density per unit wavelength;

[tex]S_{\lambda} = \frac{8\pi hc}{\lambda^{5}} \cdot \frac{1}{e^{\frac{hc}{\lambda kT}} - 1}[/tex]

The constant term [itex]8\pi hc[/itex] does not effect the position of the peak and can therefore be ignored. Thus the derivative becomes;

[tex]\frac{d}{d\lambda} = \frac{1}{\lambda^5}\cdot \frac{1}{e^{\frac{hc}{\lambda kT}} - 1} \;\; d\lambda = 0[/tex]

Once you have found the derivative all that remains is to solve the equation. As far as I know there exists no analytical solution to the equation and it must be solved numerically. However, if I have time I may venture into the maths forums and inquire as to whether an analytical solution exists.

HINT: Solve numerically for [itex]\lambda_{max}T[/itex] first.

~H
 
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  • #3


First, let's break down Planck's spectral radiation law. It states that the spectral radiance of a black body at a given wavelength (λ) and temperature (T) can be calculated using the following equation:

B(λ,T) = (2hc^2/λ^5) * (1/(e^(hc/λkT) - 1))

Where:
- B(λ,T) is the spectral radiance
- h is Planck's constant
- c is the speed of light
- k is the Boltzmann constant

To find the maximum wavelength, we need to find the wavelength (λ) that maximizes the spectral radiance (B(λ,T)). This can be done by setting the derivative of the spectral radiance with respect to wavelength (dS/dλ) equal to 0 and solving for λ.

So, let's start by taking the derivative of the spectral radiance:

dS/dλ = (2hc^2/λ^5) * (1/(e^(hc/λkT) - 1)) - (10hc^2/λ^6) * (1/(e^(hc/λkT) - 1)^2) * (e^(hc/λkT))

Next, we can simplify this equation by multiplying both terms by λ^6 and rearranging:

dS/dλ = (2hc^2/λ^4) * (1/(e^(hc/λkT) - 1)) - (10hc^2/λ^4) * (1/(e^(hc/λkT) - 1)^2) * (e^(hc/λkT))

Now, let's set this derivative equal to 0 and solve for λ:

dS/dλ = 0
(2hc^2/λ^4) * (1/(e^(hc/λkT) - 1)) - (10hc^2/λ^4) * (1/(e^(hc/λkT) - 1)^2) * (e^(hc/λkT)) = 0
2/(e^(hc/λkT) - 1) - 10/(e^(hc/λkT) - 1)^2 * (e^(hc/λkT)) = 0
2 - 10e^(hc/λkT)
 

FAQ: How Is Lambda Max Derived from Planck's Law?

What is Planck's spectral radiation law?

Planck's spectral radiation law, also known as Planck's law or Planck's black body radiation law, is a mathematical equation that describes the spectral brightness of a black body at a given temperature. It explains how the intensity of electromagnetic radiation emitted by a black body varies with wavelength and temperature.

Who discovered Planck's spectral radiation law?

Max Planck, a German physicist, discovered and first published Planck's law in 1900. It was a significant breakthrough in understanding the behavior of electromagnetic radiation and led to the development of quantum mechanics.

What is a black body in relation to Planck's spectral radiation law?

A black body is an ideal object that absorbs all incoming radiation and emits radiation at all wavelengths. It is an important concept in physics and is used to understand the behavior of real objects, such as stars and planets, which emit electromagnetic radiation.

How does Planck's spectral radiation law relate to the study of thermal radiation?

Planck's law is a fundamental equation in the study of thermal radiation. It explains how the distribution of electromagnetic radiation emitted by a black body changes with temperature. This is essential in understanding the properties of heated objects and their emission of light at different temperatures.

How is Planck's spectral radiation law used in practical applications?

Planck's law has various practical applications, including in the design of light bulbs, lasers, and other sources of electromagnetic radiation. It is also used in astrophysics to study the properties of stars and other celestial objects. Additionally, it has implications in the development of technologies such as solar panels and thermal imaging devices.

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