Exhaustive Notes on Light: Reflection and Refraction

Fundamentals of Light

  • Definition: Light is a form of electromagnetic radiation and energy that enables the perception of objects.
  • Mechanism of Vision: When light falls on an object, the surface reflects a portion of that light. When this reflected light enters human eyes, vision occurs.

Flashlight lighting an object and reflecting into human eye

  • Rectilinear Propagation: Light travels in straight lines under uniform atmospheric conditions.
  • Common Optical Phenomena:
    • Formation of shadows when opaque objects obstruct light paths.
    • Formation of images by plane, spherical mirrors, and spherical lenses.
    • Bending of light rays as they transition across different medium boundaries (refraction).
    • Twinkling of stars in the night sky due to atmospheric refraction.
    • Formation of rainbows due to dispersion and internal reflection within water droplets.

Reflection of Light

  • Definition: Reflection is the phenomenon in which light striking a highly polished, reflective surface (such as a mirror) is sent back into the same medium.

Reflection of light showing incident ray, normal, reflected ray, angle of incidence, and angle of reflection on a plane mirror

  • Laws of Reflection:
    • First Law: The angle of incidence (ii) is equal to the angle of reflection (rr):

i=ri = r

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

Image Formation by a Plane Mirror

  • Characteristics of Images Formed by Plane Mirrors:
    • Orientation: The image formed is erect (upright).
    • Size: The image size is equal to the object size (hi=hoh_i = h_o).
    • Position: The image distance behind the mirror is identical to the object distance in front of the mirror (v=uv = u).
    • Nature: The image is virtual, meaning light rays do not actually intersect at the image point and it cannot be projected or captured onto a screen.
    • Lateral Inversion: The image exhibits lateral inversion, where the left side of the object appears as the right side of the image and vice versa.

Virtual image formation and lateral inversion in a plane mirror

Spherical Mirrors

  • Definition: A spherical mirror is a curved mirror whose reflective surface forms part of a hollow sphere of glass.
  • Types of Spherical Mirrors:
    • Concave Mirror: A spherical mirror whose reflective surface is curved inward toward the center of the sphere. It acts as a converging mirror because rays parallel to its principal axis converge to a point after reflection.

Convergence of parallel light rays at the principal focus of a concave mirror

*   **Convex Mirror**: A spherical mirror whose reflective surface is curved outward away from the center of the sphere. It acts as a diverging mirror because rays parallel to its principal axis diverge upon reflection and appear to emanate from a virtual focal point behind the mirror.

Divergence of parallel light rays from the principal focus of a convex mirror

Terms Used in the Study of Spherical Mirrors

Spherical mirror parameters showing center of curvature C, focal point F, pole P, and principal axis

  • Center of Curvature (CC): The center of the hollow sphere of glass of which the mirror surface forms a part.
  • Radius of Curvature (RR or CPCP): The radius of the hollow sphere of glass of which the mirror forms a part; it represents the linear distance between the center of curvature (CC) and the pole (PP).
  • Pole (PP): The geometric midpoint or center point of the reflecting surface of a spherical mirror.
  • Principal Axis (XYX\text{--}Y): The straight reference line passing through the center of curvature (CC) and the pole (PP) of the mirror.
  • Principal Focus (FF):
    • For a Concave Mirror: The point on the principal axis where light rays traveling parallel to the principal axis actually converge/meet after reflecting off the mirror surface.
    • For a Convex Mirror: The point on the principal axis behind the mirror from which light rays traveling parallel to the principal axis appear to diverge after reflection.
  • Focal Length (ff): The linear distance measured between the pole (PP) and the principal focus (FF) of the spherical mirror.
  • Relationship Between Radius of Curvature and Focal Length: The radius of curvature (RR) of a spherical mirror is twice its focal length (ff):

R=2fR = 2f

f=R2f = \frac{R}{2}

Rules for Ray Tracing in Spherical Mirrors

  • Rule 1 (Rays Parallel to Principal Axis):
    • Concave Mirror: A ray parallel to the principal axis passes directly through the principal focus (FF) after reflection.
    • Convex Mirror: A ray parallel to the principal axis reflects such that it appears to diverge from the principal focus (FF) located behind the mirror.

Ray parallel to principal axis passing through focus in a concave mirror

  • Rule 2 (Rays Passing Through or Directed Towards Focus):
    • Concave Mirror: A light ray passing through the principal focus (FF) emerges parallel to the principal axis after reflection.
    • Convex Mirror: A light ray directed toward the principal focus (FF) reflects and emerges parallel to the principal axis.
  • Rule 3 (Rays Passing Through or Directed Towards Center of Curvature):
    • Concave Mirror: A ray passing through the center of curvature (CC) strikes the mirror surface normally (i = 0^\n\circ) and reflects back along the exact same line.
    • Convex Mirror: A ray directed toward the center of curvature (CC) reflects back along its original path.
  • Rule 4 (Rays Directed Obliquely to the Pole):
    • Concave & Convex Mirrors: A ray directed obliquely toward the pole (PP) reflects obliquely, obeying the law of reflection (i=ri = r) relative to the principal axis.

Image Formation by Concave Mirror

  • Object Position: At Infinity
    • Image Position: At the principal focus (FF).
    • Image Size: Highly diminished, point-sized.
    • Image Nature: Real and inverted.
  • Object Position: Beyond Center of Curvature (CC)
    • Image Position: Between the focus (FF) and center of curvature (CC).
    • Image Size: Diminished.
    • Image Nature: Real and inverted.

Image formation by concave mirror when object is beyond C

  • Object Position: At Center of Curvature (CC)
    • Image Position: At the center of curvature (CC).
    • Image Size: Same size as the object.
    • Image Nature: Real and inverted.
  • Object Position: Between Center of Curvature (CC) and Focus (FF)
    • Image Position: Beyond the center of curvature (CC).
    • Image Size: Enlarged.
    • Image Nature: Real and inverted.
  • Object Position: At Focus (FF)
    • Image Position: At infinity.
    • Image Size: Highly enlarged/magnified.
    • Image Nature: Real and inverted.
  • Object Position: Between Focus (FF) and Pole (PP)
    • Image Position: Behind the mirror.
    • Image Size: Enlarged.
    • Image Nature: Virtual and erect.

Image Formation by Convex Mirror

  • Object Position: At Infinity
    • Image Position: Behind the mirror at principal focus (FF).
    • Image Size: Highly diminished, point-sized.
    • Image Nature: Virtual and erect.
  • Object Position: Between Infinity and Pole (PP)
    • Image Position: Behind the mirror between pole (PP) and focus (FF).
    • Image Size: Diminished.
    • Image Nature: Virtual and erect.

Practical Applications of Spherical Mirrors

  • Applications of Concave Mirrors:
    • Torches, Searchlights, and Vehicle Headlights: The light source is placed at the principal focus of a concave reflector to generate powerful, parallel beams of light.
    • Shaving Mirrors and Makeup Mirrors: When held close to the face (within the focal length), they produce an enlarged, virtual, and erect image of the face.
    • Dentists' Mirrors: Dentists use concave mirrors to see enlarged virtual images of patients' teeth.

Dentist using a concave mirror to view enlarged image of teeth

*   *Solar Furnaces*: Large concave mirrors concentrate parallel solar radiation at their focus to achieve high temperatures for thermal power generation.
  • Applications of Convex Mirrors:
    • Vehicle Rear-View Mirrors: Used as side/rear-view mirrors on automobiles because they always yield an erect, diminished image and afford a significantly wider field of view compared to plane mirrors.

Convex rear-view mirror on a vehicle showing wide field of view

New Cartesian Sign Convention for Spherical Mirrors

  • Origin Reference: The pole (PP) of the mirror is treated as the origin (0,00,0) on a Cartesian coordinate plane.
  • Object Placement: The object is always placed to the left of the mirror, meaning incident light travels from left to right.
  • Horizontal Measurement: All distances parallel to the principal axis are measured from the pole (PP).
    • Distances measured in the direction of incident light (to the right of the pole along the +x+x-axis) are positive (++).
    • Distances measured opposite to the direction of incident light (to the left of the pole along the x-x-axis) are negative (-).
  • Vertical Measurement:
    • Heights measured perpendicular to and above the principal axis (along the +y+y-axis) are positive (++).
    • Heights measured perpendicular to and below the principal axis (along the y-y-axis) are negative (-).
  • Convention Summary for Mirrors:
    • Object distance (uu) is always negative (-).
    • Focal length (ff) of a concave mirror is always negative (-).
    • Focal length (ff) of a convex mirror is always positive (++).

Mirror Formula and Magnification

  • Mirror Formula: Mathematical relationship connecting object distance (uu), image distance (vv), and focal length (ff):

1v+1u=1f\frac{1}{v} + \frac{1}{u} = \frac{1}{f}

  • Magnification (mm): The ratio of image height (hih_i) to object height (hoh_o):

m=hihom = \frac{h_i}{h_o}

  • Distance Relation to Magnification: Magnification can also be expressed in terms of image distance (vv) and object distance (uu):

m=vum = -\frac{v}{u}

  • Combined Magnification Formula:

m=hiho=vum = \frac{h_i}{h_o} = -\frac{v}{u}

  • Sign Interpretation for Magnification:
    • A negative (--) magnification value signifies a real and inverted image.
    • A positive (++-) magnification value signifies a virtual and erect image.

Refraction of Light

  • Definition: Refraction is the bending of light at the boundary when it travels obliquely from one transparent medium into another due to changes in optical density and light speed.
  • Behavior Across Media:
    • Optically Rarer to Optically Denser Medium: Light slows down and bends towards the normal.
    • Optically Denser to Optically Rarer Medium: Light speeds up and bends away from the normal.

Refraction Through a Rectangular Glass Slab

  • Interface Refractions: When light passes through a glass slab, it undergoes refraction twice: first at the air-glass interface (bending toward the normal) and second at the glass-air interface (bending away from the normal).

Refraction of light passing through a rectangular glass slab showing lateral displacement

  • Parallel Emergence: The emergent ray is parallel to the initial incident ray because the extent of bending at the two parallel opposite faces of the slab is equal and opposite.
  • Lateral Displacement: The perpendicular distance separating the path of the original straight-line incident ray and the emergent ray is known as lateral displacement or lateral shift.
  • Angles Involved: Angle of incidence (ii), angle of refraction (rr), and angle of emergence (ee). For parallel slab boundaries, i=ei = e.

Laws of Refraction of Light

  • First Law: The incident ray, the refracted ray, and the normal to the interface of two transparent media at the point of incidence all lie in the same plane.
  • Second Law (Snell's Law of Refraction): The ratio of the sine of the angle of incidence (ii) to the sine of the angle of refraction (rr) is a constant value for light of a given color and for a given pair of media:

sin(i)sin(r)=constant\frac{\sin(i)}{\sin(r)} = \text{constant}

Refractive Index

  • Absolute Refractive Index (nn): The ratio of the speed of light in vacuum or air (cc) to the speed of light in a specific medium (vv):

n=cvn = \frac{c}{v}

  • Relative Refractive Index (n21n_{21}): The refractive index of medium 2 with respect to medium 1 is defined as the ratio of light speed in medium 1 (v1v_1) to light speed in medium 2 (v2v_2):

n21=Speed of light in medium 1Speed of light in medium 2=v1v2n_{21} = \frac{\text{Speed of light in medium 1}}{\text{Speed of light in medium 2}} = \frac{v_1}{v_2}

Spherical Lenses

  • Definition: A spherical lens is a transparent optical material bounded by two surfaces, where at least one or both of the surfaces are spherical.
  • Types of Lenses:
    • Convex Lens (Converging Lens): Thicker in the middle and thinner at the edges. Light rays traveling parallel to the principal axis converge to a real point on the principal axis after passing through the lens.
    • Concave Lens (Diverging Lens): Thinner in the middle and thicker at the edges. Light rays traveling parallel to the principal axis diverge after refraction, appearing to originate from a focal point located on the same side of the lens.

Rules for Ray Tracing in Spherical Lenses

  • Rule 1 (Parallel Rays):
    • Convex Lens: A light ray parallel to the principal axis refracts through the lens and passes through the principal focus (F2F_2) on the opposite side.
    • Concave Lens: A light ray parallel to the principal axis diverges upon refraction, appearing to originate from the focus (F1F_1) located on the same side as the incident ray.
  • Rule 2 (Focal Rays):
    • Convex Lens: A light ray passing through the focus (F1F_1) emerges parallel to the principal axis after refraction.
    • Concave Lens: A light ray directed toward the focus (F2F_2) on the opposite side emerges parallel to the principal axis after refraction.
  • Rule 3 (Optical Center Rays):
    • Convex & Concave Lenses: A light ray passing through the optical center (OO) of the lens travels straight through without undergoing any observable angular deviation.

Image Formation by Convex Lens

  • Object Position: At Infinity
    • Image Position: At Focus F2F_2.
    • Image Size: Highly diminished, point-sized.
    • Image Nature: Real and inverted.
  • Object Position: Beyond 2F12F_1
    • Image Position: Between F2F_2 and 2F22F_2
    • Image Size: Diminished.
    • Image Nature: Real and inverted.
  • Object Position: At 2F12F_1
    • Image Position: At 2F22F_2
    • Image Size: Same size as the object.
    • Image Nature: Real and inverted.
  • Object Position: Between 2F12F_1 and F1F_1
    • Image Position: Beyond 2F22F_2
    • Image Size: Enlarged.
    • Image Nature: Real and inverted.
  • Object Position: At Focus F1F_1
    • Image Position: At infinity.
    • Image Size: Highly enlarged/magnified.
    • Image Nature: Real and inverted.
  • Object Position: Between Focus F1F_1 and Optical Center (OO)
    • Image Position: On the same side of the lens as the object.
    • Image Size: Enlarged.
    • Image Nature: Virtual and erect.

Image Formation by Concave Lens

  • Object Position: At Infinity
    • Image Position: At Focus F1F_1 on the same side of the lens.
    • Image Size: Highly diminished, point-sized.
    • Image Nature: Virtual and erect.
  • Object Position: Between Infinity and Optical Center (OO)
    • Image Position: Between Focus F1F_1 and Optical Center (OO) on the same side.
    • Image Size: Diminished.
    • Image Nature: Virtual and erect.

Sign Convention for Spherical Lenses

  • Reference Point: Distances are measured from the Optical Center (OO) acting as the Cartesian origin.
  • Directions: Follows identical rules to spherical mirrors regarding left (-), right (++), above principal axis (++), and below principal axis (-).
  • Focal Length Conventions:
    • Focal length (ff) of a Convex lens is positive (++).
    • Focal length (ff) of a Concave lens is negative (-).

Lens Formula and Magnification

  • Lens Formula: Mathematical relationship connecting object distance (uu), image distance (vv), and focal length (ff):

1v1u=1f\frac{1}{v} - \frac{1}{u} = \frac{1}{f}

  • Magnification Produced by Lenses (mm): Ratio of image height (hih_i) to object height (hoh_o):

m=hihom = \frac{h_i}{h_o}

  • Distance Relation to Lens Magnification:

m=vum = \frac{v}{u}

  • Combined Lens Magnification Formula:

m=hiho=vum = \frac{h_i}{h_o} = \frac{v}{u}

Power of a Lens

  • Definition: Power of a lens measures its ability to converge or diverge light rays; it is quantitatively defined as the reciprocal of the focal length expressed in meters.
  • Formula:

P=1f(m)P = \frac{1}{f(\text{m})}

f(m)=1Pf(\text{m}) = \frac{1}{P}

  • SI Unit: The SI unit of lens power is Dioptre (D\text{D}).
  • Definition of 1 Dioptre: 1 Dioptre is the optical power of a lens having a focal length of 1 meter (1D=1m11\,\text{D} = 1\,\text{m}^{-1}).
  • Sign Conventions for Power:
    • A convex lens has a positive focal length, so its power is positive (++).
    • A concave lens has a negative focal length, so its power is negative (-).