Comprehensive Light Properties, Phenomena, and Applications for Physics Students

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30 Terms

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Light

Light is the source of energy that provides us with the sensation of seeing.

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Luminous Objects

Objects that emit light, such as the Sun, flames, electric lamps, and lightning.

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Non-luminous Objects

Objects that do not emit light.

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Examples of Light Sources from Electric Discharge

Spark plugs, lightning, fluorescent lamps, mercury-vapor lamps, sodium-vapor lamps.

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Main Properties of Light

Light travels in a straight line, is an electromagnetic wave, can travel through a vacuum, is a transverse wave, moves at 3×10⁸ m/s in vacuum, changes wavelength when moving between media, casts shadows when blocked, and is the fastest thing in the universe.

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Seven Principles of Light

Reflection, refraction, diffraction, interference, polarization, dispersion, and scattering.

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Five Basic Characteristics of Light

Travels in a straight line, is an electromagnetic wave, can travel in a vacuum, is a transverse wave, travels at 3×10⁸ m/s in vacuum.

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Reflection of Light

The bouncing back of light from a surface.

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First Law of Reflection

The angle of incidence is always equal to the angle of reflection (θᵢ = θᵣ).

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Second Law of Reflection

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

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Specular Reflection

Reflection from a smooth surface where reflected rays remain parallel (mirror-like).

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Diffuse Reflection

Reflection from a rough surface that scatters light in many directions.

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Refraction of Light

The bending of light when it passes from one medium to another due to change in speed.

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Laws of Refraction

The incident ray, refracted ray, and normal all lie in the same plane. The ratio of sinθᵢ to sinθᵣ is constant (Snell's Law).

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Snell's Law (concept)

States that n₁ sinθ₁ = n₂ sinθ₂, relating refractive indices and angles of incidence/refraction.

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Index of Refraction

Ratio of the speed of light in vacuum to the speed of light in a medium (n = c/v, n ≥ 1).

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Constant When Light Passes Between Media

Frequency (ƒ) stays constant; speed and wavelength change.

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Dispersion of Light

Splitting of white light into component colors because refractive index depends on wavelength.

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Example of Dispersion in Real Life

Prisms and rainbows.

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Absorption of Light

When light energy is partially converted into heat in a medium, reducing intensity.

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Polarization of Light

When light waves vibrate in only one plane perpendicular to the direction of travel (plane-polarized light).

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Ways Light Can Become Polarized

Reflection from a surface or passing through a polarizing filter.

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Formation of a Rainbow

Light refracts into a raindrop, reflects internally, then refracts out, producing a spectrum of colors (red ≈ 42°, violet ≈ 40°).

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Critical Angle

The angle of incidence where the refracted ray travels along the boundary (θ₂ = 90°).

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Total Internal Reflection (TIR)

When light travels from a denser medium to a rarer medium at an angle greater than the critical angle, it is completely reflected back into the denser medium.

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Applications of Total Internal Reflection

Fiber optics (telecom, endoscopy) and sparkle of diamonds.

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Contributions to Light Theory

Newton proposed particle theory; Huygens proposed wave theory; Young proved wave theory by interference; Maxwell showed light is an EM wave; Planck showed EM radiation is quantized; Einstein explained photoelectric effect (particle nature).

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Photon

A quantum (particle) of light energy that has both wave and particle properties.

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Formula for Energy of a Photon

E = hƒ, where h = 6.63 × 10⁻³⁴ J·s and ƒ = frequency.

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Light Ray

An imaginary line that shows the direction of light travel, perpendicular to wavefronts.