The power of the laser beam is \( P = 15.7 \, \text{mW} = 15.7 \times 10^{-3} \, \text{W} \), and the diameter of the beam is \( d = 4 \, \text{mm} = 4 \times 10^{-3} \, \text{m} \). The area of the beam cross-section is: \[ A_{\text{beam}} = \pi \left(\frac{d}{2}\right)^2 = \pi \left(\frac{4 \times 10^{-3}}{2}\right)^2 = \pi (2 \times 10^{-3})^2 = 4\pi \times 10^{-6} \, \text{m}^2. \] The intensity \( I \) is given by: \[ I = \frac{P}{A_{\text{beam}}}. \] Substituting the values: \[ I = \frac{15.7 \times 10^{-3}}{4\pi \times 10^{-6}} = \frac{15.7 \times 10^{-3}}{12.566 \times 10^{-6}} \approx 1250 \, \text{W/m}^2. \]
The intensity \( I \) of an electromagnetic wave is related to the amplitude of the magnetic field \( B_0 \) by: \[ I = \frac{B_0^2 c}{2\mu_0}, \] where: - \( \mu_0 = \frac{1}{\epsilon_0 c^2} \) is the permeability of free space, - \( c \) is the speed of light.
Rearrange the formula to solve for \( B_0^2 \): \[ B_0^2 = \frac{2 I \mu_0}{c}. \] Using \( \mu_0 = \frac{1}{\epsilon_0 c^2} \), the expression becomes: \[ B_0^2 = \frac{2 I}{\epsilon_0 c^3}. \] Therefore: \[ B_0 = \sqrt{\frac{2 I}{\epsilon_0 c^3}}. \] Comparing with the given form \( B_0 = \frac{A}{\sqrt{\epsilon_0 c^3}} \), we identify: \[ A = \sqrt{2I}. \]
Substituting \( I = 1250 \, \text{W/m}^2 \): \[ A = \sqrt{2 \times 1250} = \sqrt{2500} = 50. \]
The value of \( A \) is: 50.
At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)