Lesson 3.7 · 3. Electromagnetism

Modern Optics

The previous two lessons covered the classical foundations of optics: wave phenomena (interference, diffraction, coherence) and geometric ray tracing (reflection, refraction, lenses). In this lesson, we enter the modern era. Starting in the 1960s with the invention of the laser, optics underwent a revolution that continues today. Lasers, fiber optics, nonlinear optics, and quantum optics have transformed not only physics but also telecommunications, medicine, manufacturing, and fundamental research. Many of these advances connect directly to the quantum mechanics and electromagnetism developed earlier in this course.

Lasers

The word LASER stands for Light Amplification by Stimulated Emission of Radiation. To understand how a laser works, we need three ingredients from quantum mechanics.

Stimulated Emission

Three processes of light-matter interaction

Einstein identified three fundamental processes by which light interacts with atoms:

1. Absorption: An atom in a lower energy state $|1\rangle$ absorbs a photon of energy $h\nu = E_2 - E_1$ and transitions to the upper state $|2\rangle$. Rate: $R_{\text{abs}} = B_{12} \rho(\nu) N_1$.

2. Spontaneous emission: An atom in state $|2\rangle$ spontaneously emits a photon and drops to $|1\rangle$. The emitted photon has random direction and phase. Rate: $R_{\text{sp}} = A_{21} N_2$.

3. Stimulated emission: An incoming photon causes an atom in state $|2\rangle$ to emit a second, identical photon (same frequency, direction, phase, and polarization) while dropping to $|1\rangle$. Rate: $R_{\text{st}} = B_{21} \rho(\nu) N_2$.

The Einstein $A$ and $B$ coefficients are related: $A_{21}/B_{21} = 8\pi h\nu^3/c^3$ and $B_{12} = B_{21}$ (for equal degeneracies).

Stimulated emission is the key process. It produces a copy of the incoming photon, creating two photons where there was one. If these two photons each stimulate another emission, we get four, then eight, and so on: exponential amplification of light. But there is a catch.

Population Inversion

Why we need population inversion

In thermal equilibrium, lower energy states are always more populated than higher ones (Boltzmann distribution: $N_2/N_1 = e^{-h\nu/k_BT} < 1$). This means absorption dominates over stimulated emission: a beam of light passing through the medium is attenuated, not amplified.

For amplification, we need $N_2 > N_1$: a population inversion. This is a fundamentally non-equilibrium condition that must be maintained by an external energy source (the pump). Population inversion cannot be achieved in a simple two-level system (pumping both excites and de-excites), which is why practical lasers use three-level or four-level schemes.

In a four-level laser (the most common design), the pump excites atoms from the ground state (level 0) to a high-energy state (level 3). Atoms rapidly decay non-radiatively to the upper laser level (level 2). The laser transition occurs from level 2 to level 1, and level 1 rapidly empties back to the ground state. Because level 1 is nearly empty, population inversion between levels 2 and 1 is easily achieved.

The Laser Cavity

To turn an amplifier into an oscillator, we place the gain medium inside an optical cavity (also called a resonator): two mirrors facing each other, one highly reflective and one partially transmitting.

R = 100% R = 98% Gain Medium Output Pump energy Cavity length L
Schematic of a laser cavity: a gain medium between two mirrors. Light bounces back and forth, being amplified on each pass. The partially transmitting mirror allows a fraction of the light to escape as the output beam. External pumping maintains the population inversion.

Cavity Modes

The cavity supports standing waves. The condition for a standing wave between two flat mirrors separated by distance $L$ is:

$$L = q \frac{\lambda}{2}, \qquad q = 1, 2, 3, \ldots$$

where $q$ is a (very large) integer. The corresponding frequencies are the longitudinal modes:

$$\nu_q = q \frac{c}{2L}$$

The spacing between adjacent modes is the free spectral range:

$$\Delta\nu_{\text{FSR}} = \frac{c}{2L}$$

For a typical cavity length $L = 30$ cm, $\Delta\nu_{\text{FSR}} = 500$ MHz. The laser oscillates at the longitudinal modes that fall within the gain bandwidth of the medium. A helium-neon laser at 632.8 nm typically operates on 2-5 longitudinal modes simultaneously.

Lasing threshold

Laser action begins when the round-trip gain exceeds the round-trip loss. If the gain per pass is $G$, and the mirror reflectivities are $R_1$ and $R_2$, the threshold condition is:

$$G^2 R_1 R_2 \geq 1$$

or equivalently, the gain must compensate for mirror transmission, scattering, absorption, and diffraction losses. Below threshold, the device produces only spontaneous emission (like an LED). Above threshold, stimulated emission dominates and the output is coherent laser light.

What makes laser light special?

Laser light has four distinctive properties: (1) Directionality (a narrow, well-collimated beam), because only photons aligned with the cavity axis are amplified. (2) Monochromaticity (a very narrow spectral linewidth), because only specific cavity modes oscillate. (3) Coherence (both temporal and spatial), because all photons are copies of each other via stimulated emission. (4) High intensity, because all the power is concentrated in a narrow beam and narrow spectrum. No other light source combines all four properties.

Fiber Optics

An optical fiber is a thin, flexible strand of glass or plastic that guides light over long distances by total internal reflection. Fiber optics is the backbone of modern telecommunications: virtually all internet traffic travels through optical fibers.

Total Internal Reflection in Fibers

A typical fiber consists of a core (refractive index $n_1$) surrounded by a cladding (refractive index $n_2 < n_1$). Light entering the core at a sufficiently shallow angle (relative to the core-cladding interface) undergoes total internal reflection and is trapped inside the core.

The numerical aperture of the fiber determines the maximum acceptance angle:

$$\text{NA} = \sin\theta_{\max} = \sqrt{n_1^2 - n_2^2}$$

For a typical telecom fiber, $n_1 = 1.4475$ and $n_2 = 1.4440$, giving NA $\approx 0.10$ and $\theta_{\max} \approx 5.7°$.

Fiber Modes

Single-mode Fiber core cladding Multi-mode Fiber mode 1 mode 2 mode 3 Multi-mode fiber: different modes travel different path lengths (modal dispersion)
Top: a single-mode fiber guides only one spatial mode, preserving pulse shape over long distances. Bottom: a multi-mode fiber supports many modes traveling at different effective speeds, causing pulse broadening (modal dispersion).

Single-mode vs. multi-mode fibers

The number of modes a fiber supports depends on the V-parameter:

$$V = \frac{2\pi a}{\lambda} \text{NA} = \frac{2\pi a}{\lambda}\sqrt{n_1^2 - n_2^2}$$

where $a$ is the core radius. When $V < 2.405$, only one mode propagates: this is a single-mode fiber. For $V \gg 1$, many modes exist: this is a multi-mode fiber.

Single-mode fibers (core diameter $\sim 9$ $\mu$m for telecom wavelengths) are preferred for long-distance communication because they avoid modal dispersion (different modes travel at different speeds, broadening pulses). Multi-mode fibers (core diameter $\sim 50$-$62.5$ $\mu$m) are used for short links where ease of coupling matters more than bandwidth.

Attenuation and Dispersion

Modern silica fibers achieve remarkably low attenuation: about $0.2$ dB/km at $\lambda = 1550$ nm (the telecom C-band). This means that after 100 km, only 1% of the original power remains, but optical amplifiers (erbium-doped fiber amplifiers, or EDFAs) can boost the signal without converting it to electrical form.

Even in single-mode fibers, chromatic dispersion broadens pulses because different wavelengths travel at slightly different speeds. The dispersion is characterized by the parameter $D$ (in ps/(nm$\cdot$km)). Telecom systems manage dispersion using dispersion-compensating fibers or dispersion-shifted fibers designed so that $D = 0$ near 1550 nm.

Nonlinear Optics

At low intensities, the response of a material to light is linear: the polarization $\mathbf{P}$ is proportional to the electric field $\mathbf{E}$. But at high intensities (easily achieved with lasers), nonlinear terms become significant.

Nonlinear polarization

The polarization of a medium can be expanded in powers of the electric field:

$$P = \varepsilon_0\left(\chi^{(1)} E + \chi^{(2)} E^2 + \chi^{(3)} E^3 + \cdots\right)$$

The linear term $\chi^{(1)}$ gives ordinary refraction and absorption. The second-order term $\chi^{(2)}$ (present only in non-centrosymmetric materials) gives rise to second harmonic generation, sum/difference frequency generation, and parametric amplification. The third-order term $\chi^{(3)}$ (present in all materials) gives the Kerr effect, self-phase modulation, and four-wave mixing.

Second Harmonic Generation (SHG)

When an intense beam at frequency $\omega$ passes through a crystal with $\chi^{(2)} \neq 0$, the $E^2$ term generates a polarization component at frequency $2\omega$. This oscillating polarization radiates light at twice the input frequency (half the wavelength). For example, a 1064 nm infrared Nd:YAG laser beam can be converted to green 532 nm light by passing it through a potassium titanyl phosphate (KTP) crystal.

Efficient SHG requires phase matching: the generated second-harmonic wave must travel at the same speed as the nonlinear polarization that drives it. This condition is:

$$n(2\omega) = n(\omega)$$

which is generally not satisfied because of dispersion. Phase matching is achieved by exploiting the birefringence of the crystal: choosing a propagation direction where the ordinary wave at $\omega$ has the same index as the extraordinary wave at $2\omega$.

The Kerr Effect and Self-Phase Modulation

The third-order susceptibility $\chi^{(3)}$ causes the refractive index to depend on intensity:

$$n = n_0 + n_2 I$$

where $n_2$ is the nonlinear refractive index (typically $\sim 10^{-20}$ m$^2$/W for glass). This optical Kerr effect has several consequences:

  • Self-focusing: A beam with a Gaussian intensity profile experiences a higher refractive index at its center than at its edges, creating a self-induced lens that focuses the beam.
  • Self-phase modulation (SPM): A pulse traveling through a Kerr medium accumulates an intensity-dependent phase, broadening its spectrum.
  • Optical solitons: In optical fibers, the interplay between SPM (which broadens the spectrum) and anomalous dispersion (which compresses the pulse) can create solitons, pulses that propagate without changing shape. Solitons are governed by the nonlinear Schrodinger equation, connecting optics to the mathematics of integrable systems.

Quantum Optics Preview

Classical electromagnetism treats light as a continuous wave. Quantum mechanics (Lessons 6-11) tells us that light is made of discrete photons. Quantum optics is the field where these two descriptions meet, and where the quantum nature of light produces effects that have no classical analog.

Photon Statistics

Three types of light

The statistical properties of light reveal its quantum nature:

Coherent light (laser output) has photon numbers following a Poisson distribution: $P(n) = e^{-\bar{n}} \bar{n}^n / n!$, with variance equal to the mean ($\Delta n^2 = \bar{n}$). This is as "classical" as quantum light can be.

Thermal light (incandescent sources) follows a Bose-Einstein distribution: $P(n) = \bar{n}^n / (1+\bar{n})^{n+1}$, with super-Poissonian statistics ($\Delta n^2 = \bar{n} + \bar{n}^2 > \bar{n}$). The photons tend to arrive in bunches.

Quantum light (single-photon sources, squeezed states) can have sub-Poissonian statistics ($\Delta n^2 < \bar{n}$). This is impossible classically and is a signature of genuinely quantum behavior.

Squeezed States

The electromagnetic field has two quadratures (like the position and momentum of a harmonic oscillator), satisfying an uncertainty relation:

$$\Delta X_1 \cdot \Delta X_2 \geq \frac{1}{4}$$

A coherent state (laser light) saturates this bound with equal uncertainties in both quadratures. A squeezed state reduces the uncertainty in one quadrature below the coherent-state level, at the cost of increased uncertainty in the other:

$$\Delta X_1 = \frac{1}{2}e^{-r}, \qquad \Delta X_2 = \frac{1}{2}e^{r}$$

where $r$ is the squeezing parameter. Squeezed states are produced using parametric down-conversion (a $\chi^{(2)}$ process) and are used in gravitational wave detectors (LIGO uses squeezed light to improve sensitivity below the quantum shot noise limit) and in quantum information protocols.

Quantum Optics and Entanglement

Parametric down-conversion, where a single photon splits into two lower-energy photons, naturally produces entangled photon pairs (Lesson 9). These pairs have correlated polarizations, frequencies, and emission times. They are the workhorse of experimental quantum information science: Bell inequality tests, quantum key distribution, quantum teleportation, and boson sampling all rely on entangled photon pairs produced by nonlinear optical crystals.

Ultrafast Optics

One of the most remarkable capabilities of modern lasers is the generation of extremely short pulses. A mode-locked laser produces pulses as short as a few femtoseconds ($1$ fs $= 10^{-15}$ s).

Mode Locking

How mode locking works

A laser cavity supports many longitudinal modes separated by $\Delta\nu = c/(2L)$. Normally these modes oscillate independently with random phases. Mode locking forces all the modes to oscillate with a fixed phase relationship. When $N$ modes of equal amplitude are locked in phase, they interfere constructively once per round trip, producing a periodic train of short pulses.

The pulse duration is approximately the inverse of the total bandwidth:

$$\Delta t \approx \frac{1}{N \Delta\nu} = \frac{2L}{Nc}$$

A titanium-sapphire (Ti:sapphire) laser with a bandwidth of $\sim 100$ nm centered at $800$ nm can produce pulses as short as $\sim 5$ fs, containing only about two optical cycles.

Mode locking can be achieved by placing a modulator inside the cavity that periodically attenuates the light (active mode locking) or by using a saturable absorber that transmits high-intensity peaks and absorbs low-intensity continuous-wave light (passive mode locking). Kerr-lens mode locking, which exploits self-focusing in the gain medium, is the most common technique for generating the shortest pulses.

Applications of Ultrafast Pulses

Femtosecond pulses have opened entirely new frontiers:

  • Femtochemistry: Ahmed Zewail (Nobel Prize 1999) used femtosecond pulses to observe chemical bonds breaking and forming in real time, capturing the "transition state" of chemical reactions.
  • Attosecond science: Through high-harmonic generation (a highly nonlinear process), femtosecond laser pulses produce attosecond ($10^{-18}$ s) pulses of extreme ultraviolet light, enabling observation of electron dynamics within atoms (Nobel Prize in Physics 2023).
  • Optical frequency combs: The spectrum of a mode-locked laser consists of a comb of precisely equally spaced frequencies. This frequency comb can serve as an "optical ruler" for measuring frequencies with extraordinary precision (Nobel Prize 2005, John Hall and Theodor Hansch). Frequency combs are now used in precision spectroscopy, atomic clocks, exoplanet detection, and tests of fundamental physics.
  • Laser machining and surgery: Ultrashort pulses can ablate material with minimal heat damage to surrounding tissue, enabling precise eye surgery (LASIK) and micromachining of delicate structures.

How short can a light pulse be?

The shortest possible pulse at a given center wavelength is a single-cycle pulse: one complete oscillation of the electric field. At $\lambda = 800$ nm, the optical period is $T = \lambda/c \approx 2.7$ fs. Pulses shorter than one optical cycle do not exist at that wavelength (the concept of "wavelength" ceases to be meaningful). However, by moving to shorter wavelengths (XUV, X-rays), or by using attosecond pulses generated through high-harmonic generation, even shorter durations have been achieved, down to $\sim 40$ attoseconds.

Laser Types and Applications

Different applications demand different laser characteristics. Here is a summary of common laser types:

Laser Type Wavelength Key Properties Applications
He-Ne 632.8 nm Low power, excellent beam quality Alignment, interferometry, teaching
Nd:YAG 1064 nm High power, pulsed or CW Machining, surgery, SHG to 532 nm
Ti:sapphire 700-1000 nm Broadband, ultrafast Femtosecond spectroscopy, frequency combs
CO$_2$ 10.6 $\mu$m High power, infrared Cutting, welding, surgery
Semiconductor Various (400-1600 nm) Compact, efficient, direct modulation Telecom, optical storage, laser pointers
Fiber laser ~1060 nm High power, excellent beam quality Industrial cutting, defense

Lasers and Fundamental Physics

Lasers are not just practical tools; they are essential for testing fundamental physics. Laser interferometry detects gravitational waves (LIGO/Virgo, Lesson 33). Laser cooling traps atoms near absolute zero (Lesson 7), enabling Bose-Einstein condensation and atomic clocks. Frequency combs test whether fundamental constants vary over time. High-intensity lasers probe quantum electrodynamics in extreme fields (Schwinger limit). The laser is arguably the most versatile scientific instrument ever invented.

Key Takeaways
  • Lasers work by stimulated emission in a population-inverted medium inside an optical cavity, producing light that is directional, monochromatic, coherent, and intense.
  • Optical fibers guide light by total internal reflection; single-mode fibers avoid modal dispersion and are the backbone of global telecommunications.
  • Nonlinear optics (second harmonic generation, Kerr effect, four-wave mixing) emerges at high intensities and enables frequency conversion, soliton propagation, and ultrafast pulse generation.
  • Quantum optics reveals the photon nature of light through photon statistics (Poissonian, super-Poissonian, sub-Poissonian) and squeezed states that beat the standard quantum limit.
  • Mode-locked lasers produce femtosecond pulses, enabling real-time observation of molecular dynamics and generating frequency combs for precision metrology.
  • Modern optics connects to nearly every area of physics covered in this course: quantum mechanics, electromagnetism, relativity, and even gravitational wave detection.