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.

- 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.

- Laws of Reflection:
- First Law: The angle of incidence (i) is equal to the angle of reflection (r):
i=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.
- 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=ho).
- Position: The image distance behind the mirror is identical to the object distance in front of the mirror (v=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.

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.

* **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.

Terms Used in the Study of Spherical Mirrors

- Center of Curvature (C): The center of the hollow sphere of glass of which the mirror surface forms a part.
- Radius of Curvature (R or CP): 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 (C) and the pole (P).
- Pole (P): The geometric midpoint or center point of the reflecting surface of a spherical mirror.
- Principal Axis (X–Y): The straight reference line passing through the center of curvature (C) and the pole (P) of the mirror.
- Principal Focus (F):
- 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 (f): The linear distance measured between the pole (P) and the principal focus (F) of the spherical mirror.
- Relationship Between Radius of Curvature and Focal Length: The radius of curvature (R) of a spherical mirror is twice its focal length (f):
R=2f
f=2R
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 (F) after reflection.
- Convex Mirror: A ray parallel to the principal axis reflects such that it appears to diverge from the principal focus (F) located behind the mirror.

- Rule 2 (Rays Passing Through or Directed Towards Focus):
- Concave Mirror: A light ray passing through the principal focus (F) emerges parallel to the principal axis after reflection.
- Convex Mirror: A light ray directed toward the principal focus (F) 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 (C) 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 (C) reflects back along its original path.
- Rule 4 (Rays Directed Obliquely to the Pole):
- Concave & Convex Mirrors: A ray directed obliquely toward the pole (P) reflects obliquely, obeying the law of reflection (i=r) relative to the principal axis.
- Object Position: At Infinity
- Image Position: At the principal focus (F).
- Image Size: Highly diminished, point-sized.
- Image Nature: Real and inverted.
- Object Position: Beyond Center of Curvature (C)
- Image Position: Between the focus (F) and center of curvature (C).
- Image Size: Diminished.
- Image Nature: Real and inverted.

- Object Position: At Center of Curvature (C)
- Image Position: At the center of curvature (C).
- Image Size: Same size as the object.
- Image Nature: Real and inverted.
- Object Position: Between Center of Curvature (C) and Focus (F)
- Image Position: Beyond the center of curvature (C).
- Image Size: Enlarged.
- Image Nature: Real and inverted.
- Object Position: At Focus (F)
- Image Position: At infinity.
- Image Size: Highly enlarged/magnified.
- Image Nature: Real and inverted.
- Object Position: Between Focus (F) and Pole (P)
- Image Position: Behind the mirror.
- Image Size: Enlarged.
- Image Nature: Virtual and erect.
- Object Position: At Infinity
- Image Position: Behind the mirror at principal focus (F).
- Image Size: Highly diminished, point-sized.
- Image Nature: Virtual and erect.
- Object Position: Between Infinity and Pole (P)
- Image Position: Behind the mirror between pole (P) and focus (F).
- 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.

* *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.

New Cartesian Sign Convention for Spherical Mirrors
- Origin Reference: The pole (P) of the mirror is treated as the origin (0,0) 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 (P).
- Distances measured in the direction of incident light (to the right of the pole along the +x-axis) are positive (+).
- Distances measured opposite to the direction of incident light (to the left of the pole along the −x-axis) are negative (−).
- Vertical Measurement:
- Heights measured perpendicular to and above the principal axis (along the +y-axis) are positive (+).
- Heights measured perpendicular to and below the principal axis (along the −y-axis) are negative (−).
- Convention Summary for Mirrors:
- Object distance (u) is always negative (−).
- Focal length (f) of a concave mirror is always negative (−).
- Focal length (f) of a convex mirror is always positive (+).
- Mirror Formula: Mathematical relationship connecting object distance (u), image distance (v), and focal length (f):
v1+u1=f1
- Magnification (m): The ratio of image height (hi) to object height (ho):
m=hohi
- Distance Relation to Magnification: Magnification can also be expressed in terms of image distance (v) and object distance (u):
m=−uv
- Combined Magnification Formula:
m=hohi=−uv
- 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).

- 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 (i), angle of refraction (r), and angle of emergence (e). For parallel slab boundaries, i=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 (i) to the sine of the angle of refraction (r) is a constant value for light of a given color and for a given pair of media:
sin(r)sin(i)=constant
Refractive Index
- Absolute Refractive Index (n): The ratio of the speed of light in vacuum or air (c) to the speed of light in a specific medium (v):
n=vc
- Relative Refractive Index (n21): The refractive index of medium 2 with respect to medium 1 is defined as the ratio of light speed in medium 1 (v1) to light speed in medium 2 (v2):
n21=Speed of light in medium 2Speed of light in medium 1=v2v1
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 (F2) on the opposite side.
- Concave Lens: A light ray parallel to the principal axis diverges upon refraction, appearing to originate from the focus (F1) located on the same side as the incident ray.
- Rule 2 (Focal Rays):
- Convex Lens: A light ray passing through the focus (F1) emerges parallel to the principal axis after refraction.
- Concave Lens: A light ray directed toward the focus (F2) 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 (O) of the lens travels straight through without undergoing any observable angular deviation.
- Object Position: At Infinity
- Image Position: At Focus F2.
- Image Size: Highly diminished, point-sized.
- Image Nature: Real and inverted.
- Object Position: Beyond 2F1
- Image Position: Between F2 and 2F2
- Image Size: Diminished.
- Image Nature: Real and inverted.
- Object Position: At 2F1
- Image Position: At 2F2
- Image Size: Same size as the object.
- Image Nature: Real and inverted.
- Object Position: Between 2F1 and F1
- Image Position: Beyond 2F2
- Image Size: Enlarged.
- Image Nature: Real and inverted.
- Object Position: At Focus F1
- Image Position: At infinity.
- Image Size: Highly enlarged/magnified.
- Image Nature: Real and inverted.
- Object Position: Between Focus F1 and Optical Center (O)
- Image Position: On the same side of the lens as the object.
- Image Size: Enlarged.
- Image Nature: Virtual and erect.
- Object Position: At Infinity
- Image Position: At Focus F1 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 (O)
- Image Position: Between Focus F1 and Optical Center (O) 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 (O) 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 (f) of a Convex lens is positive (+).
- Focal length (f) of a Concave lens is negative (−).
- Lens Formula: Mathematical relationship connecting object distance (u), image distance (v), and focal length (f):
v1−u1=f1
- Magnification Produced by Lenses (m): Ratio of image height (hi) to object height (ho):
m=hohi
- Distance Relation to Lens Magnification:
m=uv
- Combined Lens Magnification Formula:
m=hohi=uv
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=f(m)1
f(m)=P1
- SI Unit: The SI unit of lens power is Dioptre (D).
- Definition of 1 Dioptre: 1 Dioptre is the optical power of a lens having a focal length of 1 meter (1D=1m−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 (−).