Planck's Law of Blackbody Radiation
1. Introduction
Classical physics predicted the Rayleigh–Jeans law, which led to the ultraviolet catastrophe at high frequencies.
In 1900, Max Planck proposed a quantum hypothesis to explain blackbody radiation correctly.
2. Planck's Quantum Hypothesis
Energy of an oscillator of frequency \( \nu \) is quantized:
- \(h\) = Planck’s constant
- \(\nu\) = frequency of radiation
3. Average Energy of Oscillator
Using Bose–Einstein statistics, the average energy is:
where
4. Density of States
Number of electromagnetic modes between \( \nu \) and \( \nu + d\nu \):
5. Planck's Radiation Formula
Energy density per unit frequency interval:
Stefan's Law :
It states that the total energy radiated per unit area per unit time by a black body at any temperature T is directly proportional to the fourth power of it's absolute temperature .
Mathematically: $E \propto T^{4}$
$$
\begin{aligned}
& \text { or } \\
& E / A=\sigma T^{4} \quad\left(\sigma=5.67 \times 10^{-8} \mathrm{~W} / \mathrm{m}^{2}-K^{4}\right. \text { called as Stefan's Constant.) }
\end{aligned}
$$
Proof :
Energy density in the frequency range $f$ and $f+d f$
$$
\begin{aligned}
& \frac{d}{d \lambda}\left(E_{\lambda}\right)=\frac{d}{d \lambda}\left(\frac{8 \pi h c \lambda^{-5}}{e^{\frac{h c}{\lambda k T}}-1}\right)=0 \\
& \Rightarrow-5 \lambda^{-6}\left(e^{\frac{h c}{\lambda k T}}-1\right)^{-1}+\lambda^{-5}\left(e^{\frac{h c}{\lambda k T}}-1\right)^{-2} e^{\frac{h c}{\lambda k T}} \frac{h c}{k T} \lambda^{-2}=0 \\
& \Rightarrow-\frac{5}{\lambda^{6}} \frac{1}{e^{\frac{h c}{\lambda k T}}-1}+\frac{1}{\lambda^{7}} \frac{h c}{k T\left(e^{\frac{h c}{\lambda k T}}-1\right)^{2}}=0 \\
& \Rightarrow \frac{5}{\lambda^{6}}=\frac{1}{e^{\frac{h c}{\lambda k T}}-1}\left(\frac{h c}{k T}\right) \frac{1}{\lambda^{7}} \\
& \Rightarrow e^{\frac{h c}{\lambda k T}}-1=\frac{e^{\frac{h c}{\lambda k T}} h c}{5 \lambda k T} \\
& \Rightarrow e^{\frac{h c}{\lambda k T}}\left(1-\frac{h c}{5 \lambda k T}\right)=1 \\
& \Rightarrow e^{x}\left(1-\frac{x}{5}\right)=1 \\
& \Rightarrow x=4.965 \\
& \Rightarrow \frac{h c}{\lambda k T}=4.965 \\
& \Rightarrow \lambda_{m} T=\frac{4.965 k}{h c}=b=2 \cdot 898 \times 10^{-3} m-K \\
& \therefore \lambda_{m} \alpha \frac{1}{T}
\end{aligned}
$$
This is Planck’s Law of Blackbody Radiation.
$$
\begin{aligned}
\Rightarrow u(f) d f&=\frac{E(f) d f}{V}\\
&=\frac{8 \pi h f^{3} d f}{c^{3}\left(e^{\frac{h f}{k T}}-1\right)} \\
& \left.=8 \pi h\left(\frac{k T}{h}\right)^{3} \frac{k T}{h} \int_{0}^{\infty} \frac{x^{3} d x}{c^{3}\left(e^{x}-1\right)} \quad \text { Putting } \frac{h f}{k T}=x \Rightarrow f=x k T / h, \Rightarrow d f=d x k T / h\right) \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty} \frac{x^{3} d x}{\left(e^{x}-1\right)} \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty} \frac{x^{3} e^{-x} d x}{e^{-x}\left(e^{x}-1\right)} \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty} \frac{x^{3} e^{-x} d x}{\left(1-e^{-x}\right)} \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty} x^{3} e^{-x}\left(1-e^{-x}\right)^{-1} d x \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty} x^{3} e^{-x}\left(1+e^{-x}+e^{-2 x}+e^{-3 x}+\ldots\right) d x \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}} \int_{0}^{\infty}\left(x^{3} e^{-x}+x^{3} e^{-2 x}+x^{3} e^{-3 x}+x^{3} e^{-4 x}+\ldots\right) d x \\
& =\frac{8 \pi k^{4} T^{4}}{c^{3} h^{3}}\left(6\left(1+\frac{1}{2^{4}}+\frac{1}{3^{4}}+\frac{1}{4^{4}}+\ldots\right)\right) \text { using } \int_{0}^{\infty} x^{3} e^{-a x} d x=\frac{6}{a^{4}} \\
& =\left(\frac{8 \pi^{5} k^{4}}{15 c^{3} h^{3}} T^{4}\right. \\
& \therefore u_{f} \alpha T^{4}
\end{aligned}
$$
Determination of Stefan's Constant :
$$
\begin{aligned}
& \Rightarrow \frac{1}{4} c u_{f}=\sigma T^{4} \\
& \Rightarrow \frac{1}{4} c \frac{8 \pi^{5} k^{4}}{15 c^{3} h^{3}} T^{4}=\sigma T^{4} \\
& \Rightarrow \sigma=\frac{2 \pi^{5} k^{4}}{15 c^{2} h^{3}}=5.67 \times 10^{-8} \mathrm{~W} / \mathrm{m}^{2}-K
\end{aligned}
$$
Number of Photons in Volume $\mathbf{V}$ at any temperature T is :
$$
\begin{aligned}
N&=\int_{0}^{\infty} n(f) d f \\
& =\int_{0}^{\infty} \frac{8 \pi V f^{2} d f}{c^{3}\left(e^{\frac{b f}{k T}}-1\right)} \\
& =\frac{8 \pi V}{c^{3}} \int_{0}^{\infty} \frac{f^{2} d f}{\left(e^{\frac{H f}{h_{T}}}-1\right)} \\
& =\frac{8 \pi}{c^{3}}\left(\frac{k T}{h}\right)^{2 \infty} \frac{x^{2} d x}{\left(e^{x}-1\right)}\left(\frac{k T}{h}\right) \quad \text { Substituiting } \frac{h f}{k T}=x \\
& =8 \pi\left(\frac{k T}{h c}\right) \int_{0}^{3 \infty} \frac{x^{2} d x}{\left(e^{x}-1\right)} \\
& =8 \pi\left(\frac{k T}{h c}\right) \int_{0}^{3 \infty} \frac{x^{2} e^{-x} d x}{e^{-x}\left(e^{x}-1\right)} \\
& =8 \pi\left(\frac{k T}{h c}\right)^{3 \infty} \int_{0}^{2} e^{-x}\left(1-e^{-x}\right)^{-1} d x \\
& =8 \pi\left(\frac{k T}{h c}\right)^{3 \infty} \int_{0}^{2} x^{2} e^{-x}\left(1+e^{-x}+e^{-2 x}+e^{-3 x}+e^{-4 x}+\ldots\right) d x \\
& =8 \pi\left(\frac{k T}{h c}\right)^{3 \infty} \int_{0}^{2}\left(x^{2} e^{-x}+x^{2} e^{-2 x}+x^{2} e^{-3 x}+x^{2} e^{-4 x}+x^{2} e^{-5 x}+\ldots\right) d x \\
& =8 \pi\left(\frac{k T}{h c}\right)^{3} \times 2 \times \sum \frac{1}{n^{3}} \quad \text { using } \int_{0}^{\infty} x^{m} e^{-a x} d x=\frac{m!}{n^{m+1}}
\end{aligned}
$$
6. Limiting Cases
6.1 Low Frequency Limit (hν ≪ kBT)
Proof :
Energy density in the frequency range $f$ and $f+d f$Determination of Stefan's Constant :
Number of Photons in Volume $\mathbf{V}$ at any temperature T is :
6. Limiting Cases
6.1 Low Frequency Limit (hν ≪ kBT)
Using approximation \( e^x \approx 1 + x \):
This reduces to the Rayleigh–Jeans law.
6.2 High Frequency Limit (hν ≫ kBT)
Then:
This reduces to Wien’s law.
7. Wien’s Displacement Law
Maximum intensity occurs at:
Thus, peak wavelength decreases as temperature increases.
8. Stefan–Boltzmann Law
Total energy density:
Total emitted power:
where \( \sigma \) is the Stefan–Boltzmann constant.
9. Importance of Planck's Law
- Resolved ultraviolet catastrophe.
- Introduced concept of energy quantization.
- Foundation of quantum mechanics.
10. Important Result
It marks the birth of quantum theory.