Light



1. Introduction to Light
  • Light: A form of energy that enables us to see objects around us.

  • Key Properties:

    • Light itself is invisible, but its presence makes other objects visible.

    • Speed of Light: \(3 \times 10^8 \text{ m/s}\) in vacuum or air.

    • Light travels in straight paths (rectilinear propagation).

    • Light can travel through a vacuum.


2. Reflection of Light
  • Definition: The phenomenon of bouncing back of light rays when they strike the surface of an object.

  • Key Components:

    • Incident Ray: The incoming ray of light that strikes the surface.

    • Reflected Ray: The ray of light that bounces back from the surface.

    • Normal: An imaginary line drawn perpendicular to the surface at the point of incidence.

    • Angle of Incidence (\(\angle i\)): The angle between the incident ray and the normal.

    • Angle of Reflection (\(\angle r\)): The angle between the reflected ray and the normal.

  • Laws of Reflection:

    1. First Law: The angle of incidence is equal to the angle of reflection (\(\angle i = \angle r\)).

    2. Second Law: The incident ray, reflected ray, and normal at the point of incidence all lie in the same plane.


3. Image Formation by Plane Mirrors
  • Lateral Inversion: A phenomenon where the left side of an object appears as the right side in its mirror image, and vice versa.

    • Application: The word "AMBULANCE" is written laterally inverted on the front of ambulance vehicles so drivers ahead can read it correctly in their rear-view mirrors.

  • Characteristics of Images Formed by Plane Mirrors:

    • Virtual and Erect: Cannot be captured on a screen and is upright.

    • Same Size: The size of the image is equal to the size of the object.

    • Same Distance: The image is formed behind the mirror at the same distance as the object is in front of it.

    • Laterally Inverted.

    • Focal Length: The focal length of a plane mirror is infinite (\(\infty\)).


4. Spherical Mirrors

Spherical mirrors are curved mirrors whose reflecting surfaces form part of a hollow sphere.

  • Types of Spherical Mirrors:

    • Concave Mirror: Curved inwards (like a cave) with the outer side polished; acts as a converging mirror.

    • Convex Mirror: Curved outwards with the inner side polished; acts as a diverging mirror.

  • Key Terminology:

    • Pole (\(P\)): The midpoint or center of the reflecting surface.

    • Center of Curvature (\(C\)): The center of the sphere of which the mirror forms a part.

    • Radius of Curvature (\(R\)): The distance between the Pole (\(P\)) and Center of Curvature (\(C\)).

    • Principal Axis: The straight line passing through the Pole (\(P\)) and Center of Curvature (\(C\)).

    • Principal Focus (\(F\)): The midpoint between \(C\) and \(P\) where parallel light rays converge or appear to diverge.

    • Focal Length (\(f\)): The distance between the Focus (\(F\)) and Pole (\(P\)). \[\mathbf{R = 2f} \quad \text{or} \quad \mathbf{f = \frac{R}{2}} \quad\]

    • Aperture: The effective diameter of the circular reflecting surface.

  • Rules for Ray Diagrams (Spherical Mirrors):

    1. A ray parallel to the principal axis passes through (or appears to diverge from) the principal focus after reflection.

    2. A ray passing through (or directed towards) the focus becomes parallel to the principal axis after reflection.

    3. A ray passing through the Center of Curvature (\(C\)) retraces its path back along the same path after reflection.

    4. A ray incident obliquely at the pole reflects obliquely at the same angle with the principal axis.


5. Image Formation & Uses of Spherical Mirrors
Image Formation by Concave Mirror:
  1. Object at Infinity: Image formed at \(F\); highly diminished (point-sized); Real & Inverted.

  2. Object Beyond \(C\): Image formed between \(C\) and \(F\); diminished; Real & Inverted.

  3. Object at \(C\): Image formed at \(C\); same size as object; Real & Inverted.

  4. Object Between \(C\) and \(F\): Image formed beyond \(C\); enlarged; Real & Inverted.

  5. Object at \(F\): Rays reflect parallel towards infinity; image is not formed / highly enlarged.

  6. Object Between \(P\) and \(F\): Image formed behind the mirror; enlarged; Virtual & Erect.

  • Uses of Concave Mirrors:

    • Shaving & Makeup Mirrors: Provide a magnified upright view when the face is close.

    • Dentist Mirrors: Provide an enlarged view of teeth.

    • Solar Furnaces: Concentrate parallel sunlight at the focus to generate intense heat.

    • Headlights & Torches: Bulbs placed near the focus produce powerful parallel beams of light.

Image Formation by Convex Mirror:
  1. Object at Infinity: Image formed at \(F\) (behind mirror); highly diminished (point-sized); Virtual & Erect.

  2. Object at Any Finite Distance: Image formed between \(P\) and \(F\) (behind mirror); diminished; Virtual & Erect.

  • Uses of Convex Mirrors:

    • Rear-View Mirrors in Vehicles: Offer a wider field of view and form upright, diminished images of traffic behind.

    • Surveillance / Security Cameras: Used in shops and doorways for wider area visibility.


6. Sign Convention & Mirror Formula
  • New Cartesian Sign Convention:

    • Distances measured to the left of the pole (against incident light) are negative.

    • Distances measured to the right of the pole (along incident light) are positive.

    • Heights measured above the principal axis are positive.

    • Heights measured below the principal axis are negative.

    • Object Distance (\(u\)) is always negative.

    • Focal Length (\(f\)):

      • Concave Mirror: Negative.

      • Convex Mirror: Positive.

  • Mirror Formula: \[\mathbf{\frac{1}{v} + \frac{1}{u} = \frac{1}{f}} \quad\] (where \(v\) = image distance, \(u\) = object distance, \(f\) = focal length).

  • Magnification (\(m\)): \[\mathbf{m = \frac{\text{Height of Image }(h_i)}{\text{Height of Object }(h_o)} = -\frac{v}{u}} \quad\]

    • Negative \(m\): Image is Real and Inverted.

    • Positive \(m\): Image is Virtual and Erect.

    • \(|m| > 1\): Image is enlarged.

    • \(|m| < 1\): Image is diminished.


7. Refraction of Light
  • Definition: The phenomenon of bending of light rays when passing obliquely from one transparent medium to another due to a change in the speed of light.

  • Bending Behavior:

    • Rarer to Denser Medium: Light bends towards the normal.

    • Denser to Rarer Medium: Light bends away from the normal.

  • Laws of Refraction:

    1. First Law: Incident ray, refracted ray, and normal at the point of incidence all lie in the same plane.

    2. Second Law (Snell's Law): The ratio of the sine of the angle of incidence (\(\sin i\)) to the sine of the angle of refraction (\(\sin r\)) is constant for a given pair of media: \[\mathbf{\frac{\sin i}{\sin r} = \text{Constant}} \quad\]

  • Refraction through a Rectangular Glass Slab:

    • Light undergoes refraction twice (air-to-glass and glass-to-air).

    • Angle of incidence (\(\angle i\)) = Angle of emergence (\(\angle e\)).

    • The emergent ray is parallel to the incident ray but displaced laterally (Lateral Displacement).


8. Refractive Index (\(n\))
  • Definition: A measure of a medium's ability to bend light rays passing through it.

  • Key Relationships:

    • Higher Refractive Index \(\rightarrow\) Greater light bending ability.

    • Higher Refractive Index \(\rightarrow\) Greater optical density.

    • Higher Refractive Index \(\rightarrow\) Lower speed of light in that medium (\(n \propto \frac{1}{v}\)).

  • Absolute Refractive Index: \[\mathbf{n = \frac{c}{v}} \quad\] (where \(c = 3 \times 10^8 \text{ m/s}\) in vacuum/air, \(v\) = speed of light in medium). Refractive index of air is 1.

  • Relative Refractive Index:

    • Refractive index of Medium 2 with respect to Medium 1 (\(n_{21}\)): \[\mathbf{n_{21} = \frac{n_2}{n_1} = \frac{v_1}{v_2}} \quad\]


9. Refraction by Spherical Lenses

Spherical lenses are transparent optical materials bounded by two spherical surfaces.

  • Types of Lenses:

    • Convex Lens: Thicker at the center, thinner at the edges; acts as a converging lens.

    • Concave Lens: Thinner at the center, thicker at the edges; acts as a diverging lens.

  • Key Terminology:

    • Optical Center (\(O\)): Center point of the lens.

    • Principal Focus: Represented as \(F_1\) and \(F_2\) on either side of the lens.

    • Center points are represented as \(2F_1\) and \(2F_2\) instead of \(C\).

  • Rules for Ray Diagrams (Lenses):

    1. A ray parallel to the principal axis passes through \(F_2\) (convex) or appears to diverge from \(F_1\) (concave).

    2. A ray passing through \(F_1\) emerges parallel to the principal axis.

    3. A ray passing through the Optical Center (\(O\)) passes straight without any bending (zero deviation).

Image Formation by Convex Lens:
  1. Object at Infinity: Image formed at \(F_2\); point-sized; Real & Inverted.

  2. Object Beyond \(2F_1\): Image formed between \(F_2\) and \(2F_2\); diminished; Real & Inverted.

  3. Object at \(2F_1\): Image formed at \(2F_2\); same size as object; Real & Inverted.

  4. Object Between \(2F_1\) and \(F_1\): Image formed beyond \(2F_2\); enlarged; Real & Inverted.

  5. Object at \(F_1\): Image formed at infinity.

  6. Object Between \(F_1\) and \(O\): Image formed on the same side as object; enlarged; Virtual & Erect.

  • Uses: Magnifying glasses, microscopes, telescopes, hypermetropia correction.

Image Formation by Concave Lens:
  1. Object at Infinity: Image formed at \(F_1\); point-sized; Virtual & Erect.

  2. Object at Any Finite Distance: Image formed between \(F_1\) and \(O\); diminished; Virtual & Erect.

  • Uses: Correction of myopia, door peepholes, laser flashlights, and torches.


10. Lens Formula, Magnification & Power of Lens
  • Lens Formula: \[\mathbf{\frac{1}{v} - \frac{1}{u} = \frac{1}{f}} \quad\]

  • Magnification for Lens (\(m\)): \[\mathbf{m = \frac{h_i}{h_o} = \frac{v}{u}} \quad\]

  • Sign Convention for Focal Length (\(f\)):

    • Concave Lens: Negative.

    • Convex Lens: Positive.

  • Power of a Lens (\(P\)):

    • Definition: The degree of convergence or divergence of light rays achieved by a lens.

    • Formulae: \[\mathbf{P = \frac{1}{f \text{ (in meters)}}} \quad \text{or} \quad \mathbf{P = \frac{100}{f \text{ (in cm)}}} \quad\]

    • SI Unit: Dioptre (\(D\)).

    • 1 Dioptre Definition: The power of a lens whose focal length is \(1 \text{ meter}\) (\(1\text{ D} = 1\text{ m}^{-1}\)).

    • Power Signs:

      • Convex Lens: Positive Power.

      • Concave Lens: Negative Power.

    • Combination of Lenses: Net Power \(P_{\text{net}} = P_1 + P_2 + P_3 + \dots\).