The position of the \( m \)-th bright fringe for wavelength \( \lambda \) is given by: \[ y_m = \frac{m \lambda D}{d} \]
For the bright fringes due to both wavelengths to coincide, their positions must be the same: \[ \frac{m \lambda_1 D}{d} = \frac{n \lambda_2 D}{d} \] Simplifying: \[ m \lambda_1 = n \lambda_2 \] \[ \frac{m}{n} = \frac{\lambda_2}{\lambda_1} \]
\[ \frac{m}{n} = \frac{\lambda_2}{\lambda_1} = \frac{450 \times 10^{-9}}{600 \times 10^{-9}} = \frac{3}{4} \]
Thus, the smallest values of \( m = 3 \) and \( n = 4 \).
The least distance \( y \) where the fringes coincide 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 least distance from the central maximum where the bright fringes due to both wavelengths coincide is **3.6 mm**.