The resolving power \( R \) of a diffraction grating is given by:
\[ R = nN \]
where:
The number of minima \( m \) between two principal maxima is related to the number of slits \( N \) by:
\[ m = N - 1 \]
Substituting \( m = 40 \):
\[ N = m + 1 = 40 + 1 = 41 \]
Given:
The slit separation is:
\[ d - a = 4\mu m - 2\mu m = 2\mu m \]
The first-order diffraction (\( n = 1 \)) is typically used for maximum resolving power.
Substituting \( n = 1 \) and \( N = 41 \) into the resolving power formula:
\[ R = nN = 1 \times 41 = 41 \]
The maximum order \( n \) for diffraction can be determined using the grating equation:
\[ n\lambda \leq d \]
where:
Solving for \( n \):
\[ n \leq \frac{d}{\lambda} = \frac{4}{0.6} \approx 6.67 \]
The maximum integer \( n \) is \( 6 \).
Substituting \( n = 6 \) and \( N = 41 \) into the resolving power formula:
\[ R = nN = 6 \times 41 = 246 \]
The maximum resolving power of the system is 246.
The motion of a particle in the XY plane is given by \( x(t) = 25 + 6t^2 \, \text{m} \); \( y(t) = -50 - 20t + 8t^2 \, \text{m} \). The magnitude of the initial velocity of the particle, \( v_0 \), is given by:
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/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)