Final answer:
The line density of a diffraction grating can be calculated using the formula d ⋅ sin(θ) = m ⋅ λ, where the inverse of d gives the line density in lines/cm. To find additional bright spots and their respective angles, we use the same equation with higher order numbers until the sine of the angle exceeds 1, indicating no further spots are visible.
Step-by-step explanation:
When laser light of wavelength 633.2 nm passes through a diffraction grating, the first bright spots occur at ±18.6° from the central maximum, we can use the equation for diffraction grating maxima, which is d ⋅ sin(θ) = m ⋅ λ, where d is the distance between grating lines, θ is the angle of the bright spot, m is the order number, and λ is the wavelength of the light. To calculate the line density, which is the inverse of d and typically expressed as lines per centimeter, we can rearrange this equation and use m = 1 for the first order maximum.
A. To find the line density (N), N = ⅛ / d, we first calculate d using d = m ⋅ λ / sin(θ) and then take its inverse. For θ = 18.6° and λ = 633.2 nm, the line density N comes out to be the inverse of “d” calculated value.
B. To determine the number of additional pairs of bright spots beyond the first, we need to calculate at which order number (m) the sine of the angle exceeds 1, since the sine function cannot exceed 1 (sine values are between -1 and 1). This represents the number of visible pairs of bright spots.
C. & D. To find the angles for the second and third bright spots, we use m = 2 and m = 3 in the formula given above and solve for θ, keeping in mind that as θ approaches 90°, no more bright spots will be observable beyond that angle.