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Physics

18

Geometrical Optics

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⚡ Quick Summary
Geometrical optics deals with light as rays traveling in straight lines, bending when reflected or refracted. Diffraction effects are negligible due to the small wavelength of light compared to obstacle sizes.
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  • Light behaves as a wave of short wavelength.
  • A ray of light indicates the direction of propagation of light.
  • In the absence of obstacles, light rays travel in straight lines.
  • Reflection and refraction occur when light meets a surface separating two transparent media, causing the light rays to bend.
  • Diffraction occurs when light bends around the edge of an obstacle, but this effect is often negligible in geometrical optics.

Reflection at Smooth Surfaces

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⚡ Quick Summary
Light reflects off smooth surfaces following two laws: the angle of incidence equals the angle of reflection, and the incident ray, reflected ray, and normal are coplanar.
['Angle of incidence = Angle of reflection']
  • Laws of Reflection:
    1. The angle of incidence (i) is equal to the angle of reflection (r).
    2. The incident ray, the reflected ray, and the normal to the reflecting surface are coplanar (lie in the same plane).

Image Formation by Plane Mirror

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⚡ Quick Summary
Rays reflected from a plane mirror appear to diverge from a point behind the mirror, creating a virtual image. The distance from the object to the mirror is equal to the distance from the image to the mirror.
['Object distance = Image distance (for plane mirrors)']
  • Reflected rays from a point source S placed before a plane mirror appear to diverge from a point I behind the mirror.
  • The point I is the image of the object S.
  • The distance from the object to the mirror (SA) is equal to the distance from the image to the mirror (AI), i.e., SA = AI.

Reflection at Curved Surfaces

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⚡ Quick Summary
The laws of reflection apply to both plane and curved surfaces. A normal to a curved surface is drawn by finding the tangent plane at a point and then drawing a line perpendicular to that plane.
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  • The basic laws of reflection are the same for plane and curved surfaces.
  • A normal can be drawn from any point of the curved surface by first drawing the tangent plane from that point and then drawing the line perpendicular to that plane.
  • Angles of incidence and reflection are defined from this normal.

Spherical Mirrors

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⚡ Quick Summary
Spherical mirrors are sections of a hollow sphere. A convex mirror reflects from the outer surface, while a concave mirror reflects from the inner surface. Key terms include center of curvature, radius of curvature, pole, and principal axis.
  • A spherical mirror is a part cut from a hollow sphere.
  • Spherical mirrors are generally constructed from glass with one surface silvered.
  • Convex Mirror: Reflection takes place at the convex (outer) surface.
  • Concave Mirror: Reflection takes place at the concave (inner) surface.
  • Center of Curvature: The center of the sphere of which the mirror is a part.
  • Radius of Curvature: The radius of the sphere of which the mirror is a part.
  • Pole: The point on the mirror at the middle of the surface.
  • Principal Axis: The line joining the pole and the center of curvature.

Focus of concave mirror

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⚡ Quick Summary
When a parallel beam of light hits a concave mirror, the reflected rays converge at a point called the focus.
  • Suppose a light beam travelling in a direction parallel to the principal axis is incident on a concave mirror.

Spherical Mirrors - Extended Objects and Magnification

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⚡ Quick Summary
Deals with image formation by spherical mirrors for extended objects and defines lateral magnification.
['Mirror Equation (alternative forms): 1/v + 1/u = 1/f', 'Magnification: m = h₂/h₁ = -v/u']

Extended Objects and Magnification

When an object AB is placed perpendicular to the principal axis of a spherical mirror, the image A'B' is formed. Two key rays, one parallel to the principal axis (BD) and another directed towards the centre of curvature (BE), are used to trace the image of point B (B'). A perpendicular from B' to the principal axis gives A', the image of A. Figure 18.8 illustrates this setup in different scenarios.

Lateral Magnification: The ratio of the height of the image (h₂) to the height of the object (h₁) is called lateral or transverse magnification. By convention, heights above the principal axis are positive, and heights below are negative. Erect images have positive heights, and inverted images have negative heights. Considering the ray BP hitting the mirror at the pole P, the right-angled triangles ABP and A'B'P are similar.

Refraction at Plane Surfaces

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⚡ Quick Summary
Light bends when it passes from one transparent medium to another. Snell's Law describes this bending.
["Snell's Law: sin(i)/sin(r) = v₁/v₂ = m₂/m₁", 'Where:', 'i = angle of incidence', 'r = angle of refraction', 'v₁ = speed of light in medium 1', 'v₂ = speed of light in medium 2', 'm₁ = refractive index of medium 1', 'm₂ = refractive index of medium 2']

Refraction at Plane Surfaces

When a light ray encounters a surface separating two transparent media, it bends. This bending is governed by Snell's Law.

Image Formation by Lenses

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⚡ Quick Summary
Lenses form images by refracting light. The position and size of the image depend on the object's distance and the lens's focal length.
['m = h2 / h1 (Lateral Magnification)', 'm = v / u (Magnification in terms of image and object distances)']
  • The principal axis must pass through the focus F.
  • The lateral or transverse magnification is defined as m = h2/h1, where h2 = height of the image and h1 = height of the object.

Power of a Lens

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⚡ Quick Summary
The power of a lens is the reciprocal of its focal length, measured in dioptres. Converging lenses have positive power, while diverging lenses have negative power.
['P = 1/f (Power of a lens)']
  • The power P of a lens is defined as P = 1/f, where f is the focal length.
  • The SI unit of power of a lens is m–1, also known as dioptre.
  • The focal length of a converging lens is positive and that of a diverging lens is negative. Thus, the power of a converging lens is positive and that of a diverging lens is negative.

Thin Lenses in Contact

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⚡ Quick Summary
When thin lenses are placed in contact, their combined focal length can be found by adding the reciprocals of their individual focal lengths.
['1/F = 1/f1 + 1/f2 (Effective focal length of lenses in contact)']
  • Consider two lenses L1 and L2 placed in contact with focal lengths f1 and f2, respectively.
  • If the combination is replaced by a single lens of focal length F such that it forms the image of O at the same position I.