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In-Class Activities
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8.5 In-Class Activities - Blackbody Radiation
When light enters a material, it can be reflected, absorbed ot transmitted.
A blackbody can be imagined to be a perfect material that do not transmit nor reflect light. It absorbs all incoming light.
This does not mean that the blackbody itself does not emit light. In fact a blackbody will emit light as long as its temperature is not zero.
Blackbody emission is broadband. The intensity profile (over a range of wavelengths) is given by
\begin{equation} I_\lambda = A \frac{2hc^2}{\lambda^5}\frac{1}{\exp(\frac{hc}{\lambda kT})-1} \end{equation}
where h=6.63 \times 10^{-34} \text{ m}^2 \text{kgs}^{-1}, c = 3.0 \times 10^8 \text{ ms}^{-1}, k=1.38 \times 10^{-23} \text{ m}^2 \text{kgs}^{-2} \text{K}^{-1}, \lambda is the wavelength in meters (not nm), T is the temperature in Kelvins, and A is a geometrical scaling factor.
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Activity 1: Stefan-Boltzmann Law
The total intensity of the radiation over all wavelength is given by the integral
I = \int^{\infin}_0 I_\lambda d\lambda
Show that
I \propto T^4
Do a bit of rescaling by letting \frac{hc}{kT} = \frac{1}{T'}, and perform the integration with a software.
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Activity 2: Wein's Law
The peak of the blackbody emission profile can be found by finding its derivative and equate to 0, i.e. \frac{d I_\lambda}{d \lambda} =0. Show that
\lambda_{mode}T = 0.29 \text{ cm K}
After differentiating, let \lambda T = x
Show that the maximum wavelength corresponds to photon energy of the order of kT.
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Activity 3: Finding the temperature of a blackbody emisison
Download the spectrum of an incandescent light bulb collected by an optical spectrometer in Canvas.
Using A and T as your fitting parameter, fit the data with Eq.(
Also try fitting the data with
\begin{equation} \tilde I_\lambda = A\frac{2hc^2}{\lambda^5}\exp \left(-\frac{hc}{\lambda kT}\right) \end{equation}
Does it fit well?
Eq.(
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Activity 4: Rayleigh-Jeans
When E = \frac{hc}{\lambda} \ll kT,
\begin{equation} I_\lambda \approx 2ckT\lambda^{-4} \end{equation}
This is the approximated expression for the other end of the spectrum known as the Rayleigh-Jean side. Show Eq.(