The problem involves understanding the behavior of a black body and its spectral energy density, particularly how the peak wavelength of the black body radiation shifts when the temperature changes. This is governed by Wien's Displacement Law, which states:
\(\lambda_{\text{max}} T = b\)
where \(\lambda_{\text{max}}\) is the wavelength corresponding to the maximum spectral energy density, \(T\) is the absolute temperature of the black body, and \(b\) is Wien's constant (approximately \(2.898 \times 10^{-3} \, \text{m} \cdot \text{K}\)).
Let's analyze the given statement:
\(T \rightarrow 2T\),
\(\lambda_{\text{max,new}} \cdot 2T = b\)
\(\lambda_{\text{max,new}} = \frac{\lambda_{\text{max}}}{2}\).
Next, let's examine the behavior of the area under the curve:
The area under the spectral energy density curve is representative of the total energy emitted by the black body, which is given by the Stefan-Boltzmann Law:
\(E = \sigma T^4\)
Where \(\sigma\) is the Stefan-Boltzmann constant.
\(E' = \sigma (2T)^4 = \sigma \cdot 16T^4 = 16E\)
In conclusion, the correct choices are:
Thus, the correct answer is: "the maximum of \(u_T(\lambda)\) shifts to \(\lambda_{\text{max}}/2\)" and "the area under the curve becomes 16 times the original area".
