Diffraction gratings Knowledge-Based Study

Physics · Light & Optics · Physics · Physical Optics

Physics topic explanations on Diffraction gratings.

Study notes

  1. What is a Diffraction Grating?

    A diffraction grating is an optical component consisting of a periodic structure of a very large number of equally spaced, closely positioned parallel slits or reflective grooves. While Young's double-slit experiment demonstrates basic interference using two slits, a diffraction grating typically incorporates hundreds or thousands of lines per millimeter.

    The distance between the centers of two adjacent slits is called the grating spacing or slit separation, denoted by dd. If a grating has NN lines (or grooves) per unit length (such as per meter or per millimeter), the grating spacing is calculated as:

    d=1Nd = \frac{1}{N}

    For example, a grating labeled with 500 lines per millimeter has a slit spacing of:

    d=1 mm500=2×10−3 mm=2×10−6 md = \frac{1\text{ mm}}{500} = 2 \times 10^{-3}\text{ mm} = 2 \times 10^{-6}\text{ m}

    Condition for Constructive Interference

    When monochromatic light of wavelength λ\lambda is incident normally on a transmission grating, each slit acts as a coherent source of cylindrical secondary wavelets (according to Huygens' principle). Waves emerging from adjacent slits at an angle θ\theta relative to the original beam direction travel different distances.

    The path difference between rays from two adjacent slits is:

    ΔL=dsin⁡θ\Delta L = d \sin\theta

    Constructive interference across all slits occurs simultaneously when this path difference is an integer multiple of the wavelength. This yields the fundamental diffraction grating equation:

    dsin⁡θ=mλwhere m=0,±1,±2,…d \sin\theta = m\lambda \quad \text{where } m = 0, \pm 1, \pm 2, \dots
    • m=0m = 0 corresponds to the central maximum (zero-order maximum), where all waves travel identical path lengths and exit undeflected (θ=0\theta = 0).
    • m=±1,±2,…m = \pm 1, \pm 2, \dots are the first-order, second-order, and higher-order principal maxima.

    Because sin⁡θ\sin\theta cannot exceed 1, the total number of observable diffraction orders is strictly limited by the physical constraint:

    ∣m∣≤dλ|m| \le \frac{d}{\lambda}

    Why Gratings Produce Sharp Spectral Lines

    In a double-slit setup, interference fringes vary smoothly in brightness across a broad angular range. In contrast, a diffraction grating produces extremely sharp, intense, and narrow principal maxima separated by wide dark regions.

    As the total number of illuminated slits increases, light completely cancels out at angles just slightly off the principal maximum direction because wavelets from widely separated slits destructively interfere. As a result, the angular width of each maximum decreases proportionally to 1/N1/N, producing fine lines suitable for high-precision spectroscopic measurement.

    Angular Dispersion

    Angular dispersion (DD) quantifies the angular separation between two spectral lines differing by a unit wavelength:

    D=dθdλ=mdcos⁡θD = \frac{\mathrm{d}\theta}{\mathrm{d}\lambda} = \frac{m}{d \cos\theta}

    Dispersion increases with higher diffraction orders (mm) and smaller slit separations (dd).

    Resolving Power of a Grating

    The ability of an optical grating to distinguish two closely spaced wavelengths λ\lambda and λ+Δλ\lambda + \Delta\lambda is characterized by its resolving power (RR):

    R=λΔλ=Ntotal⋅mR = \frac{\lambda}{\Delta\lambda} = N_{\text{total}} \cdot m

    Here, NtotalN_{\text{total}} is the total number of illuminated grating lines and mm is the spectral order. According to the Rayleigh criterion, two adjacent spectral peaks are just resolved when the central maximum of one falls on the first minimum of the other.

    Diffraction of Polychromatic Light

    When white light illuminates a grating:

    • The zero-order maximum (m=0m = 0) remains white because all wavelengths satisfy θ=0\theta = 0.
    • For m≥1m \ge 1, because sin⁡θ=mλ/d\sin\theta = m\lambda / d, longer wavelengths diffract at greater angles than shorter wavelengths. Consequently, red light (≈700 nm\approx 700\text{ nm}) diffracts more strongly than violet light (≈400 nm\approx 400\text{ nm}), spreading white light into a continuous rainbow spectrum with violet closest to the center and red furthest away.
    • Higher-order spectra (such as m=2m = 2 and m=3m = 3) may partially overlap when the angular deflection of blue wavelengths in the higher order matches that of red wavelengths in the lower order.