// First Year Engineering · Applied Physics

Laser &
Fibre Optics

Interactive Study Guide · Animated Diagrams · Deep Explanations

Chapter 01

Laser Physics

① Spontaneous Emission

An atom has electrons that can exist in different energy levels. When an electron is in a higher (excited) energy state E₂ and no external trigger is needed, it randomly falls back to the lower ground state E₁.

While falling, it releases energy in the form of a photon. The energy of the photon equals exactly the difference between the two levels:

E_photon = h·ν = E₂ − E₁

The key word is spontaneous — it happens on its own, at a random time and in a random direction. Photons emitted this way are incoherent (different phases, different directions). This is what happens in a normal light bulb or LED.

// Animation: Spontaneous Emission
Random process — no external trigger
🔀Emitted photon: random phase & direction
💡Source of ordinary (incoherent) light
Lifetime in excited state ~10⁻⁸ s

② Stimulated Emission

Now imagine an excited atom (electron in E₂) is hit by an incoming photon whose energy exactly matches E₂ − E₁.

This incoming photon stimulates the electron to drop down, releasing a second photon. The magic is that the emitted photon is identical to the incoming photon in: phase, frequency, direction, and polarization.

So one photon enters → two coherent photons leave. This is the fundamental mechanism of laser amplification — Light Amplification by Stimulated Emission of Radiation.

ΔE = h·ν_incoming → Two identical photons emitted
// Animation: Stimulated Emission — 1 in, 2 out
🎯Triggered by matching-energy photon
🔗Emitted photon is COHERENT with incoming
✖2Signal amplification: 1 photon → 2
🔬This IS the lasing mechanism

③ Population Inversion

In thermal equilibrium, most atoms are in the ground state (low energy). If a photon travels through, it's more likely to be absorbed than to cause stimulated emission. So no amplification happens!

For a laser to work, we need the opposite situation: more atoms in the excited state than in the ground state. This abnormal condition is called Population Inversion.

We achieve this by pumping energy into the medium (using light, electricity, or chemical reactions) to keep pushing atoms to higher levels faster than they fall back.

N₂ > N₁ ← Population Inversion condition
// Animation: Before vs After Population Inversion (pumping)
🔋Achieved by external pumping (optical/electrical)
📊N₂ > N₁ (more atoms excited than ground)
⚠️Without this, medium absorbs instead of amplifies
🏗️Requires 3-level or 4-level energy systems

④ Metastable State

Atoms normally stay excited for only ~10⁻⁸ seconds before spontaneously emitting. But for population inversion, we need atoms to stay excited longer.

A metastable state is a special energy level where atoms remain for a relatively long time (~10⁻³ seconds — a million times longer!). Atoms are pumped to a higher short-lived level, quickly drop to the metastable state, and accumulate there.

This is what makes population inversion possible. The metastable state acts like a "waiting room" — atoms collect there until a photon stimulates them all to emit together.

τ_metastable ≈ 10⁻³ s vs τ_normal ≈ 10⁻⁸ s
// Diagram: Energy levels — pump → metastable → ground
Lifetime ~10⁻³ s (very long for an atom)
📥Atoms accumulate here — population inversion builds
🔑Essential for lasing action
🏛️Example: E₃ in He-Ne, Nd:YAG lasers

⑤ Resonant Cavity (Optical Resonator)

A single pass of light through the gain medium isn't enough amplification. The resonant cavity solves this by bouncing light back and forth, amplifying it with each pass.

It consists of two mirrors: one fully reflective (100%) and one partially reflective (~95%). The partially reflective mirror lets a small fraction of the light out — this is the actual laser beam!

The cavity also acts as a frequency selector. Only wavelengths where an integer number of half-waves fit between the mirrors experience constructive interference and get amplified — others cancel out. This gives the laser its extremely narrow frequency.

L = n · (λ/2) where n = 1, 2, 3... (resonance condition)
// Animation: Light bouncing in resonant cavity, output beam
🪞Mirror 1: 100% reflective (back)
🔦Mirror 2: ~95% reflective (output coupler)
🔁Multiple passes → huge amplification
🎵Standing wave condition selects frequency

⑥ Helium-Neon (He-Ne) Laser

The He-Ne laser is a classic gas laser that produces a bright red beam at 632.8 nm. It uses a mixture of He and Ne gases in a glass tube.

How it works (step-by-step):
1. An electrical discharge (high voltage) excites Helium atoms to metastable states (E₁* and E₂*).
2. Excited He atoms collide with Neon atoms and transfer their energy — this is called resonant energy transfer because He and Ne have nearly identical energy levels.
3. Neon atoms reach their metastable upper lasing levels and population inversion is achieved in Neon.
4. Stimulated emission occurs in Neon, producing the 632.8 nm laser light.
5. The resonant cavity amplifies this into a coherent beam.

He(excited) + Ne(ground) → He(ground) + Ne(excited) [resonant collision] λ = 632.8 nm (red visible laser)
// Animation: He-Ne Laser — energy transfer & beam output
🔴Output: 632.8 nm (red) — most common
Pumping: electrical discharge through gas
🤝He excites, Ne lases (resonant transfer)
📐Highly monochromatic & coherent

⑦ LIDAR (Light Detection and Ranging)

LIDAR is the laser equivalent of RADAR. Instead of radio waves, it uses laser pulses to measure distances and create 3D maps of environments with incredible precision.

Working Principle:
A laser sends out a short pulse. The pulse hits an object and some light bounces back to a detector. By measuring the time of flight (time taken for the pulse to return), we calculate the exact distance:

Distance (d) = c × Δt / 2 where c = speed of light, Δt = round-trip time

By scanning millions of pulses in all directions, LIDAR builds a detailed 3D point cloud of the environment. Used in: autonomous cars, aircraft mapping, archaeology, meteorology (measuring cloud height), and even Mars rovers!

// Animation: LIDAR pulse sent & returned, distance calculated
🚗Used in self-driving cars (Tesla, Waymo)
🌍Topographic mapping from aircraft
cm-level precision over km distances
🌫Atmospheric sensing — wind, clouds, pollution

Chapter 02

Fibre Optics

① Total Internal Reflection (TIR)

When light travels from a denser medium (high refractive index n₁) to a rarer medium (low n₂), it bends away from the normal (Snell's Law). As the angle of incidence increases, the refracted ray bends more and more.

At a specific angle called the critical angle, the refracted ray travels along the interface (90° to normal). Beyond this angle — all light is reflected back into the denser medium. No light escapes. This is Total Internal Reflection.

Optical fibres exploit TIR to trap light inside the glass core and guide it over long distances.

// Animation: TIR — drag angle slider to see partial → critical → total reflection
Angle of incidence: 30°
🔴Only in denser → rarer medium
🔁100% of light reflected — no energy lost
🔮Basis of all optical fibre communication
💎Also explains sparkle of diamonds!

② Critical Angle

The critical angle (θ_c) is the minimum angle of incidence (measured from the normal, inside the denser medium) at which Total Internal Reflection occurs.

Derived from Snell's Law: n₁·sin(θ₁) = n₂·sin(θ₂). At the critical angle, θ₂ = 90°, so sin(90°) = 1:

n₁·sin(θ_c) = n₂·sin(90°) = n₂ ⟹ sin(θ_c) = n₂/n₁ ⟹ θ_c = sin⁻¹(n₂/n₁)

For glass (n₁ = 1.5) and air (n₂ = 1.0): θ_c = sin⁻¹(1/1.5) ≈ 41.8°
For a fibre core (n₁ = 1.48) and cladding (n₂ = 1.46): θ_c ≈ 80.6°

📐θ_c = sin⁻¹(n₂/n₁)
🔺If angle > θ_c → TIR occurs
Higher n₁/n₂ ratio → smaller θ_c → easier TIR
🔢Glass/air θ_c ≈ 41.8°

③ Acceptance Angle

Not all light entering a fibre will undergo TIR — only light entering within a cone of acceptance will be guided. The acceptance angle (θ_a) is the maximum angle to the fibre axis at which light can enter and still undergo TIR inside.

Light entering at an angle greater than θ_a will hit the core-cladding boundary at too shallow an angle and escape — it won't be guided.

sin(θ_a) = √(n₁² − n₂²) / n₀ For air (n₀ = 1): sin(θ_a) = √(n₁² − n₂²) θ_a = sin⁻¹(√(n₁² − n₂²))
// Diagram: Acceptance cone at fibre entrance
📡Defines the input "cone" that gets guided
🔺Light outside this cone escapes the core
🔗sin(θ_a) = NA (Numerical Aperture)
📏Wider acceptance → easier to couple light in

④ Numerical Aperture (NA) — Full Derivation

The Numerical Aperture (NA) is the most important parameter of an optical fibre — it measures the fibre's ability to collect and guide light. It equals sin of the acceptance angle.

Step-by-step derivation for Step Index Fibre:

At the fibre entrance (in medium n₀), Snell's Law gives:
n₀ · sin(θ_a) = n₁ · sin(θ_r) …(1)

Inside the core, at the core-cladding boundary, for TIR we need the angle to be ≥ critical angle:
The ray hits the boundary at angle φ = (90° − θ_r)
For TIR: φ ≥ θ_c → (90° − θ_r) ≥ θ_c → θ_r ≤ (90° − θ_c)

At the limiting case (maximum acceptance): φ = θ_c
So: n₁ · sin(θ_c) = n₂ …(2) (from critical angle definition)

From (2): sin(θ_c) = n₂/n₁ → cos(θ_c) = √(1 − n₂²/n₁²)

At maximum acceptance: θ_r = 90° − θ_c
So: sin(θ_r) = sin(90° − θ_c) = cos(θ_c) = √(1 − n₂²/n₁²) = √(n₁² − n₂²)/n₁

Substituting back into (1):
n₀ · sin(θ_a) = n₁ · √(n₁² − n₂²)/n₁ = √(n₁² − n₂²)

∴ NA = n₀ · sin(θ_a) = √(n₁² − n₂²) [for n₀ = 1 (air)] Where: n₁ = refractive index of core (higher) n₂ = refractive index of cladding (lower) θ_a = acceptance angle Also: NA = n₁ · √(2Δ) where Δ = (n₁−n₂)/n₁ (fractional refractive index diff)

Physical meaning: Higher NA → larger acceptance cone → easier to couple light → but more dispersion. Typical single-mode fibre: NA ≈ 0.1 to 0.2. Multimode: NA ≈ 0.2 to 0.5.

// Diagram: NA derivation geometry

⑤ Step Index vs Graded Index Fibre

Optical fibres differ in how the refractive index varies across the cross-section of the core:

// Diagram: Refractive index profiles & ray paths comparison
Parameter Step Index (Multimode) Graded Index (Multimode) Step Index (Single Mode)
RI ProfileUniform core, sharp boundaryGradually decreasing from axisUniform but very narrow core
Ray PathZigzag (bounces sharply)Sinusoidal (curves smoothly)Straight (only one mode)
Core Diameter50–200 μm50–100 μm8–10 μm
BandwidthLow (~20 MHz·km)Medium (~500 MHz·km)Very High (>10 GHz·km)
Modal DispersionHigh (different paths = diff. times)Low (speed compensates path)Zero (single mode)
AttenuationHighMediumLow
CostCheapestMediumMost expensive
ApplicationsShort distance LANCampus networksLong-haul telecom, internet backbone
NAHigh (0.3–0.5)Lower, varies with radiusLow (0.1–0.2)
📈Step: RI jumps abruptly at core edge
📉Graded: RI decreases gradually outward — reduces dispersion
🌐Internet uses single-mode step-index
🔬Graded index: outer rays travel faster, inner slower — all arrive together!

⑥ Attenuation in Optical Fibres

As light travels through an optical fibre, its power decreases with distance. This loss is called attenuation. It's measured in decibels per kilometre (dB/km).

Attenuation (dB/km) = (10/L) · log₁₀(P_in / P_out) where L = fibre length in km

Main causes of attenuation:

🔵 Rayleigh Scattering — Light scatters off microscopic density fluctuations in the glass. Dominant at short wavelengths. Follows λ⁻⁴ law — shorter λ = more scattering.

🔴 Absorption — Glass absorbs some photons due to impurities (OH⁻ ions, metal ions) or intrinsic glass absorption. Pure silica has very low absorption.

🟡 Micro/Macro-bending losses — Any bend in the fibre changes the angle of incidence at the core-cladding boundary. If the angle drops below critical angle, light escapes.

📡 The minimum attenuation window for silica fibre is at 1550 nm (~0.2 dB/km) — which is why all modern long-haul internet uses 1550 nm wavelength!

Attenuation vs Wavelength (silica fibre): 850 nm : ~2.5 dB/km (multimode window) 1310 nm : ~0.35 dB/km (zero-dispersion point) 1550 nm : ~0.2 dB/km (minimum attenuation — used by internet!)
// Animation: Signal fading with distance along fibre
📡1550 nm used globally for low-loss comms
📉0.2 dB/km → after 100 km, only 1% power left
🔬Rayleigh scattering dominant for λ < 1000 nm
🔁Repeaters/amplifiers placed every ~80 km