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Revision: Interference and Diffraction Physics HSC Science (General) 12th Standard Board Exam Maharashtra State Board

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Definitions [7]

Definition: Fringe

A fringe is a bright or dark band formed on the screen due to constructive or destructive interference.

Definition: Interference of Light

Interference is the phenomenon in which light intensity is modified due to the superposition of two or more light waves.

Definition: Fringe Width

Fringe width is the distance between two consecutive bright fringes or two consecutive dark fringes.

Definition: Resolution (Rayleigh's Criterion)

The condition where the images of two point objects close to each other are regarded as resolved (separated), if the central maximum of one falls on the first minimum of the other, is called Rayleigh's criterion for resolution.

Definition: Not Resolved (Unresolved)

When the separation between the central maxima of two objects is less than the distance between the central maximum and the first minimum of any of the two objects, the images are said to be 'not resolved' or unresolved.

Definition: Just Resolved

When the separation between the central maxima of the two objects is just equal to the distance between the central maximum and first minimum of any of the two objects, the images are said to be just resolved.

Definition: Well Resolved

When the separation between the central maxima of two objects is greater than the distance between the central maximum and first minimum of any of the two objects, the images are said to be well resolved.

Formulae [7]

Formula: Fringe Width (β)

\[\beta=\frac{\lambda D}{d}\]

Formula: Angular fringe width (α)

\[\alpha=\frac{\beta}{D}=\frac{\lambda}{d}\]

Formula: Distance between n-th bright and m-th dark

\[x_n-x_m=\left[n-\frac{(2m-1)}{2}\right]\beta\]

Formula: Position of m-th dark fringe

\[\begin{array} {cc} & x_m=\frac{(2m-1)\lambda D}{2d} \end{array}\]

Formula: Position of n-th bright fringe

\[\begin{array} {c}x_n=\frac{n\lambda D}{d}=n\beta \end{array}\]

Formula: Limit of resolution of Microscope

Limit of resolution (self-luminous objects):

d = \[\frac{1.22\lambda}{2\sin\theta}=\frac{0.61\lambda}{\sin\theta}\]

Limit of resolution (objects illuminated by light of wavelength λ):

d = \[\frac{\lambda}{2\sin\theta}\]

If a liquid of refractive index μμ is between object and objective:

d = \[\frac{\lambda}{2\mu\sin\theta}\]

where θθ is the angle subtended by an object at the objective.

Formula: Smallest Angular Separation of Telescope

Smallest angular separation dθdθ (Circular aperture):

\[d\theta=\frac{1.22\lambda}{D}\]

where D is the aperture (diameter) of objective of the telescope.

Smallest angular separation (Rectangular aperture):

\[d\theta=\frac{d}{D}\]

where d is slit separation and D is distance.

Theorems and Laws [1]

Law: Rayleigh's Criterion for Resolution

Statement: According to Lord Rayleigh, the images of two point objects close to each other are regarded as resolved (separated), if the central maximum of one falls on the first minimum of the other.

The reasoning of Rayleigh's criterion is given by considering the intensity distribution in the diffraction pattern produced by two objects.

Three Conditions:

Condition Description
Not Resolved Separation between central maxima < distance between central maximum and first minimum of either object
Just Resolved Separation between central maxima = distance between central maximum and first minimum of either object
Well Resolved Separation between central maxima > distance between central maximum and first minimum of either object

Important Questions [34]

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