The position of the \( m \)-th bright fringe for a given wavelength \( \lambda \) is calculated as: \[ y_m = \frac{m \lambda D}{d} \]
For bright fringes from both wavelengths to align, their positions must be equal: \[ \frac{m \lambda_1 D}{d} = \frac{n \lambda_2 D}{d} \] Simplified to: \[ m \lambda_1 = n \lambda_2 \] Which yields the ratio: \[ \frac{m}{n} = \frac{\lambda_2}{\lambda_1} \]
Calculate the ratio of fringe orders: \[ \frac{m}{n} = \frac{\lambda_2}{\lambda_1} = \frac{450 \times 10^{-9}}{600 \times 10^{-9}} = \frac{3}{4} \]
The smallest integer values satisfying this ratio are \( m = 3 \) and \( n = 4 \).
The minimum distance \( y \) where fringes overlap is: \[ y = \frac{m \lambda_1 D}{d} = \frac{3 \times 600 \times 10^{-9} \times 1}{0.5 \times 10^{-3}} = 3.6 \, \text{mm} \]
The bright fringes from both wavelengths coincide at the minimum distance of 3.6 mm from the central maximum.