President Giuse

Physics 23 Study Guide

Giancoli Physics — Full Course (Lectures 1A through 10B)

Chapters 16–25  |  Electrostatics · Circuits · Magnetism · EM Induction · Waves · Optics · Instruments

📋 Table of Contents — Click to expand/collapse

Lecture 1A — Electric Charge & Coulomb's Law

Date: January 6, 2026  |  Sections: 16.1–16.7

§16.1–16.3 — Static Electricity, Conductors, Induction

Electric charge comes in two kinds: positive (protons) and negative (electrons). Like charges repel, unlike attract. Charge is conserved (total charge in a closed system is constant) and quantized in units of e = 1.602 × 10⁻¹⁹ C.

Conductors (metals) — electrons move freely.
Insulators (rubber, glass) — electrons are tightly bound.
Semiconductors (Si, Ge) — intermediate.

Charging Methods

  • Friction: rubbing transfers electrons (e.g., balloon on hair)
  • Conduction (contact): charge flows from charged to neutral object
  • Induction: bring charged object near a conductor → free charges redistribute. Ground the conductor → opposite-sign charges flow to ground → remove ground → object is left with net charge of opposite sign to inducer.

An electroscope detects charge: gold leaves diverge when like charges are induced on them.

§16.4 — Coulomb's Law

The force between two point charges Q₁ and Q₂ separated by distance r:

Coulomb's Law (Eq. 16-1, 16-2) F = k · |Q₁Q₂| / r²    where k = 8.988 × 10⁹ N·m²/C²

Equivalently, k = 1/(4πε₀) where ε₀ = 8.85 × 10⁻¹² C²/(N·m²) is the permittivity of free space.

Alternate form F = (1/4πε₀) · Q₁Q₂ / r²
Vector form: Force is along the line joining the charges. Repulsive if same sign, attractive if opposite. Treat magnitudes in the formula and assign direction by inspection.
Compared with gravity: Same 1/r² form, but Coulomb's force is ~10³⁹ times stronger between two electrons than their gravitational attraction.

§16.5 — Multi-Charge Systems (Superposition)

The total force on a charge from multiple other charges is the vector sum of the individual Coulomb forces:

Principle of Superposition Fnet = Σ Fi = F₁ + F₂ + F₃ + …

Strategy: compute each pairwise force magnitude with Coulomb's law, decompose into x and y components, sum components, then recombine.

+Q₁ +Q₂ +q F₁ F₂ Fnet
Superposition: net force on charge q is the vector sum of Coulomb forces from Q₁ and Q₂.

§16.6 — The Electric Field

The electric field at a point is the force per unit positive test charge placed there:

Electric Field Definition (Eq. 16-3) E = F / q    [units: N/C = V/m]

For a point charge Q at distance r:

Field of Point Charge (Eq. 16-4) E = kQ / r²    (radially outward if Q>0, inward if Q<0)
Why use E? The field is a property of space, set up by source charges, independent of any test charge. Once E is known, the force on any charge q placed there is just F = qE.

§16.7 — Field from Continuous Charge Distributions

For a continuous distribution, divide into infinitesimal charge elements dQ and integrate (or sum):

Field from Continuous Distribution E = ∫ k · dQ / r² · r̂

Common results to recognize (derived in lecture / textbook):

SourceField magnitudeNotes
Point chargeE = kQ/r²Radial
Infinite line (linear density λ)E = 2kλ/r = λ/(2πε₀r)Perpendicular to line
Infinite plane (surface density σ)E = σ/(2ε₀)Uniform, ⊥ plane
Conducting plate (σ on surface)E = σ/ε₀Just outside conductor
Ring (charge Q, radius R) on axisE = kQx/(x²+R²)3/2x = distance along axis

Lecture 1B — Field Lines, Conductors, Gauss's Law

Date: January 8, 2026  |  Sections: 16.8–16.9, 16.12

§16.8 — Electric Field Lines

Field lines are a visual tool: tangent to E, density proportional to |E|.

  • Originate on positive charges, terminate on negative (or at infinity)
  • Number of lines from a charge ∝ magnitude of charge
  • Field lines never cross (E has unique direction at each point)
  • For a uniform field (e.g., between parallel plates): lines are parallel and evenly spaced
+
Electric dipole field lines: from + to −, denser where the field is stronger.

§16.9 — Electric Field and Conductors

In electrostatic equilibrium (no current flowing), free charges have rearranged so that:

  • E = 0 everywhere inside a conductor. Otherwise charges would still be moving.
  • Net charge resides on the surface.
  • E is perpendicular to the surface just outside (any tangential component would push charges along surface).
  • E just outside surface: E = σ/ε₀ where σ = local surface charge density.
Faraday cage: A hollow conductor shields its interior from external static fields. Used in electronics enclosures, MRI rooms, and (approximately) car bodies during lightning strikes.

§16.12 — Gauss's Law

Electric flux through a surface is the "flow" of E through it:

Electric Flux (Eq. 16-7) ΦE = Σ E·ΔA = Σ E ΔA cos θ

Gauss's Law: the total flux through any closed surface equals the enclosed charge divided by ε₀:

Gauss's Law (Eq. 16-9) ΦE = ∮ E·dA = Qencl / ε₀
Symmetry strategy: Choose a Gaussian surface where E is either constant and ⊥ to the surface (so EΔA cos 0 = EA) or parallel to it (flux = 0). Common choices: sphere (point/spherical charge), cylinder (line/cylindrical charge), pillbox (plane/sheet charge).

Worked Examples (must-know results)

ConfigurationGaussian surfaceResult
Point charge QSphere of radius rE = kQ/r² (recovers Coulomb)
Spherical shell, charge QSphereE = 0 inside; E = kQ/r² outside
Infinite line, λCylinder of radius r, length ℓE = λ/(2πε₀r)
Infinite plane, σPillboxE = σ/(2ε₀)
Conductor surface, σPillbox half-insideE = σ/ε₀ (outside only)
Key insight: Gauss's Law is always true, but only useful for computing E when the geometry has high symmetry.

Lecture 2A — Electric Potential

Date: January 13, 2026  |  Sections: 17.1–17.5

§17.1 — Electric Potential Energy & Potential

Like gravity, the electric force is conservative. The electric potential energy change between points a and b:

Change in PE (uniform field) ΔU = Ub − Ua = −Wfield = −qEd cos θ

The electric potential V is potential energy per unit charge:

Potential Difference (Eq. 17-2a) Vba = Vb − Va = ΔU/q    [units: 1 volt = 1 J/C]
Sign convention: A positive charge naturally moves from high V to low V (releasing PE). A negative charge naturally moves from low V to high V.
Energy gained by charge q falling through V W = qV    (1 eV = energy gained by e⁻ across 1 V = 1.6×10⁻¹⁹ J)

§17.2 — Relation Between V and E

For a uniform field between parallel plates separated by distance d:

V and E in uniform field (Eq. 17-4a) Vba = −E·d    or equivalently    E = V/d

In general: E points "downhill" — from high to low potential. Electric field strength can also be expressed in V/m, equivalent to N/C.

§17.3 — Equipotential Lines & Surfaces

An equipotential is a surface where V is constant — no work is done moving a charge along it.

  • Equipotentials are always perpendicular to E field lines
  • The surface of any conductor in equilibrium is an equipotential
  • Closely spaced equipotentials → strong field; widely spaced → weak field

§17.4 — Electric Potential Due to a Point Charge

Choosing V = 0 at infinity:

Potential of Point Charge (Eq. 17-5) V = kQ/r

Note: V is a scalar, sign included (positive Q → positive V; negative Q → negative V). Falls off as 1/r (slower than E ∝ 1/r²).

§17.5 — Potential from Multiple Charges & Distributions

Superposition for V is easier than for E because V is a scalar — no vector decomposition needed:

Superposition of potentials Vtotal = Σ Vi = Σ kQi/ri

For continuous distributions: V = ∫ k dQ / r.

Potential Energy of a Pair of Charges

U = kQ₁Q₂/r    (positive if same sign, negative if opposite)

For multiple charges, sum over all unique pairs.

Lecture 2B — Capacitance & Stored Energy

Date: January 15, 2026  |  Sections: 17.7–17.9

§17.7 — Capacitance

A capacitor stores charge — typically two conductors separated by an insulator. When connected to a voltage V, it stores charge Q ∝ V:

Capacitance Definition (Eq. 17-7) Q = CV    or    C = Q/V    [units: 1 farad = 1 C/V]

Parallel-Plate Capacitor

Two plates of area A separated by distance d, vacuum between:

Parallel-Plate Capacitance (Eq. 17-8) C = ε₀ · A/d

Larger area or smaller separation → more capacitance. Typical capacitors: pF to mF range.

+Q −Q d E
Parallel-plate capacitor: uniform E between plates, magnitude E = V/d = σ/ε₀.

§17.8 — Dielectrics

Inserting an insulating material (a dielectric) between capacitor plates increases C by a factor K (the dielectric constant):

Capacitance with Dielectric C = K ε₀ A/d = ε A/d    where ε = K ε₀ is the permittivity
MaterialKDielectric strength (V/m)
Vacuum1.0000
Air (1 atm)1.00063 × 10⁶
Paper3.715 × 10⁶
Mica7150 × 10⁶
Water80

Mechanism: the dielectric polarizes — dipoles align with E, partly canceling it inside the dielectric → smaller V for same Q → larger C.

§17.9 — Energy Stored in a Capacitor

Charging from 0 to Q requires work against the building voltage:

Energy in Capacitor (Eq. 17-10) U = ½QV = ½CV² = Q²/(2C)

Energy Density of an Electric Field

For a parallel-plate capacitor, U/Volume gives the energy density of the field itself — a result that turns out to be general:

Electric Energy Density u = ½ ε₀ E²    [J/m³]
This will reappear: EM waves carry energy with density uE = ½ε₀E². The magnetic analog is uB = B²/(2μ₀) (Lecture 7A).

Lecture 3A — Current, Resistance, DC Circuits

Date: January 20, 2026  |  Sections: 18.1–18.4, 18.8, 19.1

§18.1–18.2 — The Battery & Electric Current

A battery uses chemical energy to maintain a potential difference between its terminals — an "electrical pump" pushing positive charge from low to high potential internally.

Electric Current (Eq. 18-1) I = ΔQ / Δt    [units: 1 ampere = 1 C/s]

Conventional current is in the direction positive charge would flow — opposite to actual electron flow in metals.

§18.3 — Ohm's Law & Resistance

For many materials at fixed temperature, current is proportional to voltage applied:

Ohm's Law (Eq. 18-2) V = IR    [units: 1 ohm = 1 V/A]

Ohmic materials follow this linear V–I relationship; non-ohmic devices (diodes, transistors) do not.

§18.4 — Resistivity

For a uniform wire of length ℓ and cross-section A:

Resistance (Eq. 18-3) R = ρ · ℓ / A

where ρ is the resistivity [Ω·m]. Resistivity depends on temperature:

Temperature dependence (Eq. 18-4) ρT = ρ₀[1 + α(T − T₀)]
Materialρ at 20°C (Ω·m)α (1/°C)
Copper1.68 × 10⁻⁸0.0068
Aluminum2.65 × 10⁻⁸0.00429
Tungsten5.6 × 10⁻⁸0.0045
Carbon3.5 × 10⁻⁵−0.0005
Glass10⁹–10¹²

§18.8 — Microscopic View of Current; Drift Velocity

Free electrons move randomly at very high speeds (~10⁶ m/s thermal), but with an applied field, drift slowly in the field's direction:

Current and Drift Velocity (Eq. 18-10) I = n e A vd

where n = number density of charge carriers, e = electron charge, A = cross-section, vd = drift speed.

Surprisingly slow: Drift speed in a typical wire is ~10⁻⁵ m/s. The signal (E field changes) propagates at near c, but individual electrons crawl.

§19.1 — EMF & Terminal Voltage

The EMF (ε, "electromotive force") is the voltage a source provides when no current flows. Real batteries have internal resistance r, so terminal voltage is less when current flows:

Terminal Voltage (Eq. 19-1) Vab = ε − Ir

For a circuit with external load R: I = ε / (R + r). When R ≫ r: terminal voltage ≈ ε.

Lecture 3B — Combining Resistors & Capacitors; Kirchhoff's Rules

Date: January 22, 2026  |  Sections: 19.2–19.5

§19.2 — Resistors in Series & Parallel

Series (same I) Req = R₁ + R₂ + R₃ + …
Parallel (same V) 1/Req = 1/R₁ + 1/R₂ + 1/R₃ + …
  • Series: same current through each; voltages add. Equivalent R is larger than any individual.
  • Parallel: same voltage across each; currents add. Equivalent R is smaller than any individual.

§19.3 — Kirchhoff's Rules

Junction Rule (Conservation of Charge): The sum of currents entering any junction equals the sum leaving.
ΣIin = ΣIout
Loop Rule (Conservation of Energy): The sum of potential changes around any closed loop is zero.
ΣΔV = 0

Sign Conventions for Loop Rule

  • Crossing a battery from − to + (in direction of EMF): +ε
  • Crossing a battery from + to −: −ε
  • Crossing a resistor in the direction of assumed current flow: −IR
  • Crossing a resistor opposite to assumed current flow: +IR
Strategy: (1) Label all currents with arrows (guess direction; if wrong, you'll get a negative I). (2) Apply junction rule to reduce unknowns. (3) Apply loop rule to remaining loops to get enough equations. (4) Solve the linear system.

§19.4 — EMFs in Series & Parallel; Charging a Battery

  • Series, same direction: εtot = ε₁ + ε₂; rtot = r₁ + r₂. Adds voltage.
  • Series, opposing: εtot = |ε₁ − ε₂|. (E.g., charger driving current backward through a battery to charge it.)
  • Parallel, identical batteries: Same voltage as one battery, but can supply more current (and last longer).

§19.5 — Capacitors in Series & Parallel

Note the formulas are opposite from resistors:

Series capacitors (same Q) 1/Ceq = 1/C₁ + 1/C₂ + …
Parallel capacitors (same V) Ceq = C₁ + C₂ + …
Why opposite? Series capacitors have the same charge (charge can't go through the gap, so what builds on one plate also builds on the next). Same V across each requires careful thought — voltages add, like resistors in series. Parallel: each has the source voltage, charges add.

Lecture 4A — Midterm #1

Date: January 27, 2026  |  Covers: Chapters 16, 17, 18.1–18.4 & 18.8, 19.1–19.5

What's on Midterm #1

  • Coulomb's law & multi-charge force calculations
  • Electric field, field lines, conductors in equilibrium
  • Gauss's law & symmetric distributions
  • Electric potential, equipotentials, V from point/distributions
  • Capacitors (parallel-plate, dielectrics, energy)
  • Current, Ohm's law, resistivity, EMF & terminal voltage
  • Resistor & capacitor combinations, Kirchhoff's rules
Focus areas: Practice multi-charge superposition (vectors!), Gauss's law symmetry choices, and Kirchhoff multi-loop circuits — these are the most common stumbling points.

Lecture 4B — RC Circuits, Power, Alternating Current

Date: January 29, 2026  |  Sections: 19.6, 18.5–18.7

§19.6 — RC Circuits

A capacitor in series with a resistor and battery. Charging:

RC Charging (Eq. 19-7) Q(t) = Qmax(1 − e−t/τ)    where τ = RC,   Qmax = Cε
RC Discharging (Eq. 19-8) Q(t) = Q₀ · e−t/τ    (battery removed, capacitor drains through R)
Current during charging I(t) = (ε/R) · e−t/τ
Q t Qmax Q = Qmax(1 − e⁻ᵗ/τ) τ=RC 0.63·Qmax
Capacitor charging through R. At t = τ = RC, Q reaches 63% of max.
Time constant: τ = RC. Larger R or larger C → slower charging/discharging. Compare to τ = L/R for RL circuits (Lecture 7A).

§18.5 — Electric Power

Power Dissipated (Eq. 18-5, 18-6) P = IV = I²R = V²/R    [units: 1 watt = 1 J/s]

Energy delivered: U = Pt. Electric companies bill in kilowatt-hours (1 kWh = 3.6 × 10⁶ J).

§18.6 — Power in Household Circuits

Household appliances are rated in watts at the household voltage (120 V US, 240 V EU). Current drawn: I = P/V.

  • 1500 W hair dryer at 120 V → 12.5 A — near limit of 15 A circuit breaker
  • Too many devices → I exceeds breaker rating → circuit trips
  • Fuses do the same job (single-use, melt to break circuit)

§18.7 — Alternating Current

AC voltage and current oscillate sinusoidally:

AC Voltage and Current (Eq. 18-7, 18-8) V = V₀ sin(2πft),    I = I₀ sin(2πft)

where f = 60 Hz (US) or 50 Hz (EU).

RMS (Root-Mean-Square) Values

Average of V or I is zero, so we use rms (which gives the same average power as DC):

RMS Voltage (Eq. 18-9) Vrms = V₀/√2
RMS Current Irms = I₀/√2
Average AC power (Eq. 18-10) P̄ = Irms · Vrms = ½ I₀ V₀ = Irms² R
"120 V" outlet: means Vrms = 120 V, so peak V₀ = 120·√2 ≈ 170 V.

Lecture 5A — Electric Hazards, Meters, Superconductivity

Date: February 3, 2026  |  Sections: 19.7–19.8, 18.10

§19.7 — Electric Hazards

Danger comes primarily from current, not voltage. Effects on humans:

Current (60 Hz AC, hand-to-hand)Effect
1 mAThreshold of perception
5 mAMaximum harmless current
10–20 mA"Can't let go" — muscles contract
50 mAPain, possible fainting
100–300 mAVentricular fibrillation — can be fatal
> 1 ASevere burns; possible cardiac arrest

Body resistance: dry skin ~10⁵ Ω, wet skin/internal ~10³ Ω. At 120 V on wet skin: I ≈ 120 mA → potentially lethal.

Three-prong plugs & GFCIs: The ground (third) prong gives fault current a path to ground instead of through you. A GFCI (ground-fault circuit interrupter) trips in <1 ms when it detects an imbalance ≥ 5 mA between hot and neutral lines. Required by code in bathrooms/kitchens.

§19.8 — Ammeters & Voltmeters

Both built around a galvanometer (sensitive current meter, full-scale ~50 μA, internal R~30 Ω):

  • Ammeter: Galvanometer with a small shunt Rshunt in parallel. Connected in series in the circuit. Want low total R so it doesn't perturb the circuit.
  • Voltmeter: Galvanometer with a large Rser in series. Connected in parallel across the element. Want high total R so it draws negligible current.
Common mistake: Connecting an ammeter in parallel (it has near-zero resistance → short circuit → blown fuse or worse). Always check before connecting.

§18.10 — Superconductivity

Below a critical temperature Tc, certain materials drop to zero resistance. Currents persist for years without dissipation.

  • Discovered 1911 (Onnes, Hg at 4.2 K)
  • "High-Tc" cuprates (1986+, Tc up to ~135 K) work above liquid nitrogen (77 K)
  • Applications: MRI magnets, particle accelerators (LHC), maglev trains, SQUIDs
  • Type II superconductors expel B (Meissner effect) up to a critical field Hc

Lecture 5B — Magnetism, Magnetic Force, Cyclotron Motion

Date: February 5, 2026  |  Sections: 20.1–20.6

§20.1–20.2 — Magnets & the Earth's Magnetic Field

Every magnet has two poles, North and South. Like poles repel, unlike attract. Unlike electric charges, no isolated magnetic monopole has ever been found; cutting a magnet in half gives two complete magnets.

Earth's geographic North is actually a magnetic south pole (so a compass N-pole points there). Field strength at surface ≈ 0.5 × 10⁻⁴ T.

§20.3 — Force on a Current-Carrying Wire

Force on Current-Carrying Wire (Eq. 20-1, 20-2) F = IℓB sin θ    (θ = angle between I and B)

Direction: right-hand rule #1 — point fingers in direction of I, curl toward B; thumb gives F. (Equivalently F = I×B.)

The tesla is defined by this equation: 1 T = 1 N/(A·m).

§20.4 — Force on a Moving Charge

Lorentz Force (Eq. 20-3, 20-4) F = qvB sin θ    (with E too: F = qE + qv×B)

Right-hand rule: fingers point along v, curl into B, thumb gives F (for positive q; reverse for negative).

Magnetic forces do no work: F is always perpendicular to v, so F·v = 0. Magnetic fields can change direction of motion, never speed.

§20.5 — Charged Particles in a Magnetic Field; Cyclotron Motion

A charged particle moving perpendicular to B traces a circle (or helix if v has a parallel component). Setting magnetic force = centripetal force:

Cyclotron Radius (Eq. 20-5) qvB = mv²/r  →  r = mv/(qB)
Cyclotron Frequency f = qB/(2πm)    (independent of v and r — the basis of cyclotrons)
+q v F B (out of page) r = mv/(qB)
Charged particle in uniform B (out of page) traces circular path of radius r = mv/(qB).

§20.6 — Magnetic Field of a Long Straight Wire

B from Long Wire (Eq. 20-6) B = μ₀I / (2πr)

Field circles the wire. Direction: right-hand rule #2 — thumb along I, fingers curl in direction of B.

μ₀ = 4π × 10⁻⁷ T·m/A is the permeability of free space.

Force Between Two Parallel Wires (will revisit in 6A)

Two parallel wires carrying currents I₁ and I₂ separated by distance d:

F/ℓ = μ₀ I₁ I₂ / (2π d)

Same direction → attract; opposite directions → repel. (This is how the ampere was historically defined.)

Lecture 6A — Hall Effect, Torque on Current Loops

Date: February 10, 2026  |  Sections: 20.9–20.11

§20.9 — The Hall Effect

When a current-carrying conductor sits in a B-field perpendicular to I, charge carriers are deflected to one edge — building up a transverse Hall voltage:

Hall Voltage (Eq. 20-7) VH = EH · w = vd B w

where w = width perpendicular to both I and B. Equivalently VH = IB / (n e t) where t = thickness, n = carrier density.

What it tells us:
  • Sign of VH reveals sign of charge carriers (e.g., proves electrons in metals are negative; reveals "holes" in some semiconductors).
  • Magnitude measures B (Hall probes used to measure magnetic fields), or carrier density n (semiconductor characterization).

§20.10 — Torque on a Current Loop & Magnetic Dipole Moment

A rectangular loop of N turns, area A, carrying current I in a field B experiences a torque:

Torque on Current Loop (Eq. 20-10) τ = NIAB sin θ

where θ is the angle between B and the area vector (normal to loop). Maximum when loop's plane is parallel to B (θ = 90°); zero when plane is perpendicular to B (θ = 0°).

Magnetic Dipole Moment (Eq. 20-11) μ = NIA    (vector along loop normal, by right-hand rule)
Torque in vector form τ = μ × B;   magnitude τ = μB sin θ
Energy of Magnetic Dipole in B U = −μ·B = −μB cos θ   (minimum when aligned)

§20.11 — Applications: Galvanometers, Motors, Speakers

  • Galvanometer: Loop in radial B; restoring spring → deflection ∝ I.
  • DC Motor: Loop in B + commutator (split-ring) flips current each half-turn → continuous rotation.
  • Loudspeaker: Voice-coil in radial B; AC signal → axial force on coil → cone vibrates → sound.

Lecture 6B — Solenoids, Ampère's Law, EM Induction

Date: February 12, 2026  |  Sections: 20.7–20.8, 21.1–21.2

§20.7 — Solenoids & Toroids

A solenoid is a long, tightly-wound coil. Inside (away from ends) the field is nearly uniform and parallel to the axis:

B inside a Solenoid (Eq. 20-8) B = μ₀ n I    where n = N/ℓ (turns per unit length)

Outside an ideal solenoid: B ≈ 0. With an iron core: replace μ₀ with μ = Kmμ₀ (Km can be 10²–10⁴) — the basis of electromagnets.

§20.8 — Ampère's Law

The magnetic version of Gauss's law for symmetric current distributions:

Ampère's Law (Eq. 20-9) Σ B Δℓ = μ₀ Iencl

The line integral of B around a closed Amperian loop equals μ₀ × the current through any surface bounded by the loop.

Worked Examples

SourceAmperian loopResult
Long straight wire, ICircle of radius r around wireB = μ₀I/(2πr)
Solenoid, n turns/m, IRectangle straddling wallB = μ₀nI
Toroid, N turns, ICircle inside torusB = μ₀NI/(2πr)
Maxwell's extension: Ampère's law as written is incomplete — Maxwell added the displacement-current term μ₀ε₀(dΦE/dt) (see Lecture 7B). The full law is one of the four Maxwell equations and predicts EM waves.

§21.1 — Induced EMF

Faraday's seminal experiments (1831) showed that a changing magnetic environment near a coil induces an EMF — a current flows even with no battery in the circuit. Three ways to produce induced EMF:

  • Move a magnet relative to a coil
  • Change the current (and hence the field) in a nearby coil
  • Change the area or orientation of a coil in a steady field

What matters is the rate of change of magnetic flux:

Magnetic Flux (Eq. 21-1) ΦB = B A = BA cos θ    [units: 1 weber = 1 T·m²]

§21.2 — Faraday's Law & Lenz's Law

Faraday's Law of Induction (Eq. 21-2) ε = −N · ΔΦB / Δt

where N is the number of turns. The minus sign carries Lenz's rule:

Lenz's Law: The induced current flows in the direction whose magnetic field opposes the change in flux that produced it. (A consequence of energy conservation — otherwise you'd get free energy.)

Lenz's Law in Practice

ActionFlux changeInduced current direction
N-pole of magnet approaching coilΦB increasing into coilCreates B out of coil → repels magnet
N-pole withdrawingΦB decreasingCreates B into coil → attracts magnet
Loop area shrinking in BΦB decreasingCurrent to maintain flux (same direction as B)
Connecting to next week: Lecture 7A starts with motional EMF — a special case of Faraday's law where the flux changes because the loop area changes. Inductors, transformers, and AC generators all build on this foundation.

Lecture 7A — EM Induction, Inductance, RL Circuits, Transformers

Date: February 17, 2026  |  Sections: 21.3–21.7, 21.9–21.12

§21.3 — EMF Induced in a Moving Conductor (Motional EMF)

When a conducting rod of length moves with velocity v perpendicular to a magnetic field B, free electrons in the rod experience a magnetic force F = qvB, driving them toward one end. This separation of charge creates a potential difference — an induced EMF.

Motional EMF (Eq. 21-3) ε = Bℓv

This is valid when B, , and v are mutually perpendicular. If not perpendicular, use only the perpendicular components.

Derivation via force: A charge q in the rod feels force F = qvB along the rod. Work done moving charge from one end to the other: W = qvBℓ. Since EMF = W/q: ε = Bℓv.
B (out) v ε = Bℓv F on e⁻
Moving rod on U-shaped conductor in magnetic field B (out of page). Rod moves right with speed v, inducing EMF ε = Bℓv.
Key insight: A changing magnetic flux (due to the changing area of the loop as the rod moves) also gives ε = BΔA/Δt = B(ℓv·Δt)/Δt = Bℓv — consistent with Faraday's Law.

Applications

  • Electromagnetic blood-flow meter: vessel diameter ℓ, field B, measured EMF → v = ε/(Bℓ)
  • Airplane wing EMF: ε = Bℓv ≈ 1 V (negligible in practice)

§21.4 — Changing Magnetic Flux Produces an Electric Field

A changing magnetic field produces an electric field — not just in conductors, but in any region of space. This is one of Maxwell's key insights (Faraday's Law generalized).

Effective E-field in moving conductor E = vB

This follows from F = qvB and E = F/q.

§21.5 — Electric Generators

A generator converts mechanical energy → electrical energy. A coil of N turns and area A rotates at angular velocity ω in field B. By Faraday's law the induced EMF is:

AC Generator Output (Eq. 21-5) ε = NBAω sin(ωt) = ε₀ sin(ωt)    where ε₀ = NBAω

The output is sinusoidal (alternating). The RMS output is:

Vrms = NBAω / √2 = ε₀ / √2
AC Generator schematic: N Armature coil (N turns, area A) | / ───────┤ ┌────┐ ← rotates in B field Axle ──┤ │coil│ | └────┘ S | | Slip rings → output ε = ε₀ sin(ωt)

Generator Equation Derivation

At angle θ from vertical, velocity component perpendicular to B: v⊥ = v sin θ = (ωh/2) sin θ. Contribution from both arms: ε = 2NBlv⊥ = 2NBl·(ωh/2) sin θ = NBAω sin(ωt).

DC vs. AC generators: AC generators use continuous slip rings → sinusoidal output. DC generators use split-ring commutators → rectified (pulsating) DC.

§21.6 — Back EMF and Counter Torque; Eddy Currents

Back EMF in Motors

As a motor's armature spins, it acts like a generator and produces a back EMFback) opposing the applied voltage. Net current in the motor:

Motor current (Kirchhoff's rule) I = (Vapplied − εback) / R

At start-up: εback = 0, so current is large (I = V/R). At full speed: εback ≈ V, current is small.

Motor burnout: If a motor jams (stops spinning), εback = 0 and current surges to V/R, potentially melting windings. This is why appliances burn out when overloaded.

Counter Torque in Generators

When a generator supplies current, Lenz's law produces a counter torque opposing rotation. More load → more counter torque → more mechanical energy input required. Energy is conserved.

Eddy Currents

Eddy currents are induced currents that circulate within bulk conductors in changing magnetic fields. They cause:

  • Magnetic braking (smooth, contactless braking on trains)
  • Heating losses in transformer cores (minimized by lamination)
  • Metal detection (walk-through detectors pulse current → eddy currents in metal → detected)

§21.7 — Transformers and Transmission of Power

A transformer changes AC voltage using mutual inductance. Primary coil (NP turns, voltage VP) is linked to secondary coil (NS turns, voltage VS) through a laminated iron core.

Transformer Voltage Ratio (Eq. 21-6) VS / VP = NS / NP
Transformer Current Ratio (Eq. 21-7) IS / IP = NP / NS
Power conservation (ideal transformer) Pin = Pout  →  IPVP = ISVS
Transformer (step-up shown): Primary (NP=4) Iron Core Secondary (NS=12) |||| ┌──────┐ |||||||||||| VP ─┤ ├─────────┤ ████ ├─────────┤ ├─ VS |||| └──────┘ |||||||||||| VS/VP = NS/NP = 12/4 = 3 → VS = 3·VP (step-up)

Types of Transformers

TypeNS vs NPVoltageCurrentExample
Step-upNS > NPVS > VPIS < IPPower plant output
Step-downNS < NPVS < VPIS > IPHome supply, phone charger

Power Transmission

Power loss in transmission lines: Ploss = I²R. Transmitting at high voltage → low current → minimal loss.

Power loss in transmission lines Ploss = I²R = (Ptransmitted/V)2 · R
Example: 120 kW at 240 V → I = 500 A → Ploss = (500)²(0.4) = 100 kW (83% lost!). At 24,000 V → I = 5 A → Ploss = 10 W (<0.01% lost).

Typical transmission: 240 kV → step down to 7200 V (substation) → step down to 120/240 V (home).

§21.9 — Applications of Induction

  • Microphone: Sound vibrates a coil near a magnet → induced EMF = audio signal
  • Seismograph: Relative motion of magnet and coil during earthquakes → induced EMF
  • GFCI: Detects current imbalance (≥5 mA) in hot vs. neutral lines → trips in <1 ms, protecting from electrocution
  • Inductive charging: Primary coil in charger base, secondary in device — like a transformer without an iron core

§21.10 — Inductance

Mutual Inductance

When current in coil 1 changes, it induces an EMF in nearby coil 2:

Mutual Inductance (Eq. 21-8) ε₂ = −M · (ΔI₁/Δt)    where M = mutual inductance [henrys, H]

Self-Inductance

A changing current in a coil induces an EMF in that same coil opposing the change (self-inductance L):

Self-Inductance (Eq. 21-9) ε = −L · (ΔI/Δt)    [L in henrys, H]

Inductance of a Solenoid

Solenoid inductance (Eq. 21-13) L = μ₀N²A / ℓ    (N turns, length ℓ, cross-section area A, air-filled)

where μ₀ = 4π × 10⁻⁷ T·m/A. For iron core: replace μ₀ with μ = Kmμ₀ where Km ≈ hundreds to thousands.

Units: 1 Henry (H) = 1 V·s/A. An inductor symbol on circuit diagrams: ⌇⌇⌇⌇ (coil).

§21.11 — Energy Stored in a Magnetic Field

An inductor carrying current I stores energy in its magnetic field:

Energy in inductor (Eq. 21-10) U = ½LI²

For a solenoid, using L = μ₀N²A/ℓ and B = μ₀NI/ℓ:

Magnetic energy density (Eq. 21-10) u = B² / (2μ₀)    [J/m³]
Analogy with capacitor: Capacitor stores U = ½CV² in electric field (density u = ½ε₀E²). Inductor stores U = ½LI² in magnetic field (density u = B²/2μ₀). Both formulas are general — valid anywhere those fields exist.

§21.12 — LR Circuit

When a battery V₀ is connected to an inductor L and resistor R in series, current builds exponentially:

Current build-up in RL circuit (Eq. 21-12) I(t) = (V₀/R)(1 − e−t/τ)    where τ = L/R (time constant)
Current decay (battery disconnected) I(t) = Imax · e−t/τ
I t Imax=V₀/R Growth: I=(V₀/R)(1−e⁻ᵗ/τ) τ=L/R 0.63·Imax
RL circuit current growth. At t = τ = L/R, current reaches 63% of maximum.
Time constant: τ = L/R
At t = τ: I = 0.63 Imax
At t = 5τ: I ≈ 0.993 Imax (essentially full)
Comparison to RC:
RC circuit: τ = RC
LR circuit: τ = L/R
Both show exponential behavior

AC Circuits — Reactance (§21.13)

For AC sources with current I = I₀ cos(2πft):

ElementVoltage–CurrentReactance/ResistancePhase
Resistor RV = IRR (ohms)In phase
Inductor LV = IXLXL = 2πfL = ωLV leads I by 90°
Capacitor CV = IXCXC = 1/(2πfC)I leads V by 90°

LRC Series Circuit (§21.14)

Impedance Z = √(R² + (XL − XC)²)
Ohm's Law for AC Vrms = Irms · Z
Phase angle tan φ = (XL − XC) / R

Lecture 7B — LC Circuits, Maxwell's Equations, EM Waves

Date: February 19, 2026  |  Sections: 21.13–21.15, 22.1–22.2

§21.15 — Resonance in AC Circuits; LC Oscillations

In an LRC series circuit, current is maximum when the impedance Z is minimum. This occurs when XL = XC, i.e., at the resonant frequency:

Resonant Frequency (Eq. 21-19) f₀ = 1 / (2π√(LC))    or equivalently    ω₀ = 1/√(LC)

At resonance, Z = R (purely resistive), and Irms = Vrms/R (maximum).

LC Oscillations (ideal: R ≈ 0)

Energy oscillates between the capacitor (electric field) and the inductor (magnetic field), analogous to a mechanical pendulum:

Oscillation frequency f = 1 / (2π√(LC))
Energy conservation Utotal = ½LI² + Q²/(2C) = const.
C L ½CV² ↔ ½LI² f = 1/(2π√LC) Q(t) = Q₀cos(ωt)
LC circuit oscillations: charge and current oscillate at f₀ = 1/(2π√LC).
Analogy to pendulum: Capacitor charge Q ↔ displacement x; Inductor current I ↔ velocity v; L ↔ mass m; 1/C ↔ spring constant k. Frequency: f = (1/2π)√(1/LC) ↔ f = (1/2π)√(k/m).

Radio Tuning Application

A variable capacitor C is adjusted so that f₀ = 1/(2π√(LC)) matches the station frequency. Only that frequency produces significant current in the receiver circuit.

§22.1 — Maxwell's Equations

Maxwell unified all of electromagnetism into four equations. These are the foundation of classical electrodynamics and are consistent with special relativity.

Maxwell's Equation 1 — Gauss's Law (Electric) ΣE⊥ΔA = Qencl / ε₀    "Electric field lines originate on positive charges"
Maxwell's Equation 2 — Gauss's Law (Magnetic) ΣB⊥ΔA = 0    "Magnetic field lines always form closed loops — no magnetic monopoles"
Maxwell's Equation 3 — Faraday's Law ΣE‖Δℓ = −ΔΦB/Δt    "A changing magnetic field produces an electric field"
Maxwell's Equation 4 — Ampère's Law (Extended) ΣB‖Δℓ = μ₀I + μ₀ε₀(ΔΦE/Δt)    "A current OR changing electric field produces a magnetic field"
Maxwell's key addition: The term μ₀ε₀(ΔΦE/Δt) in Equation 4 is the "displacement current" — Maxwell's hypothesis that a changing electric field acts like a current and produces a magnetic field. This symmetry predicts electromagnetic waves.
EquationNamed forPhysical meaning
1. Electric Gauss's LawGauss / CoulombElectric charges are sources of E field
2. Magnetic Gauss's LawGaussNo magnetic monopoles; B field lines close
3. Faraday's LawFaradayChanging B → electric field
4. Ampère–Maxwell LawAmpère / MaxwellCurrent or changing E → magnetic field

§22.2 — Production of Electromagnetic Waves

Maxwell reasoned: if changing B → E (Faraday), and changing E → B (his extension of Ampère), then these fields can mutually sustain each other and propagate through space as a wave — even in vacuum.

How EM Waves are Produced

Oscillating charges on an antenna (driven by an AC source) create oscillating E and B fields. These fields "detach" from the antenna and propagate outward as electromagnetic waves.

Key properties of EM waves:
  • E and B are perpendicular to each other and to the direction of propagation (transverse wave)
  • E and B are in phase (reach maxima simultaneously)
  • Amplitude decreases as 1/r from source; intensity as 1/r²
  • Self-sustaining: no medium required — propagate in vacuum
  • Produced by accelerating electric charges
→ z E (vertical) B (horizontal, into/out of page) → propagation
EM wave: E (red) and B (blue) oscillate perpendicular to each other and to the direction of travel.
Ratio of E to B in EM wave E/B = c    (speed of light)

Lecture 8A — Midterm #2

Date: February 24, 2026  |  Covers: 19.6, 18.5–18.7, 19.7–19.8, 18.10, 20.1–20.11, 21.1–21.15, 22.1–22.2

What's on Midterm #2

  • RC circuits, electric power, AC and rms values
  • Electric hazards, ammeter/voltmeter design, superconductivity
  • Magnetic force on currents and moving charges; cyclotron motion
  • B-field of long wire, force between parallel wires
  • Hall effect, torque on current loops, magnetic dipole moment
  • Solenoids, Ampère's law
  • EM induction: Faraday's & Lenz's laws, motional EMF
  • Generators, transformers, inductance, RL circuits, transmission
  • LC oscillation, resonance, Maxwell's equations, EM waves
Focus areas: Right-hand rules (force on charge, B-field of wire, magnetic dipole), Faraday/Lenz sign conventions, transformer ratios, and resonance frequency f₀ = 1/(2π√LC).

Lecture 8B — Maxwell's Equations & Electromagnetic Waves (Full)

Date: February 26, 2026  |  Sections: 22.1–22.5

§22.3 — Light as an EM Wave; The EM Spectrum

Maxwell calculated the speed of EM waves from his equations and found it exactly matched the measured speed of light. Therefore light is an electromagnetic wave.

Speed of Light (Eq. 22-2, 22-3) c = 1/√(ε₀μ₀) = E/B = 3.00 × 10⁸ m/s

where ε₀ = 8.85 × 10⁻¹² C²/(N·m²) and μ₀ = 4π × 10⁻⁷ N/A².

Wave equation (Eq. 22-4) c = f · λ    (applies to all EM waves in vacuum)

The Electromagnetic Spectrum

TypeWavelengthFrequencyUses/Source
Radio waves10³ m – 0.1 m10⁴ – 10⁹ HzAM/FM radio, TV
Microwaves0.1 m – 1 mm10⁹ – 3×10¹¹ HzRadar, microwave ovens, WiFi
Infrared (IR)1 mm – 700 nm3×10¹¹ – 4×10¹⁴ HzHeat, remote controls, IR cameras
Visible light700 nm – 400 nm4–7.5 × 10¹⁴ HzVision (red → violet)
Ultraviolet (UV)400 nm – 10 nm7.5×10¹⁴ – 10¹⁶ HzSun, sterilization
X-rays10 nm – 0.01 nm10¹⁶ – 10¹⁸ HzMedical imaging, crystallography
Gamma rays< 0.01 nm> 10¹⁸ HzNuclear decay, cancer therapy
Visible light: wavelengths 400 nm (violet) to 700 nm (red). Frequencies ≈ 4.3 × 10¹⁴ Hz (red) to 7.5 × 10¹⁴ Hz (violet).

§22.4 — Measuring the Speed of Light

Historical methods: Rømer (1676, Jupiter's moons), Michelson (rotating mirror, 1926). Modern value:

c = 2.9979 × 10⁸ m/s ≈ 3.00 × 10⁸ m/s (exact by definition since 1983)

In a medium with index of refraction n:   v = c/n < c

§22.5 — Energy and Intensity of EM Waves

EM waves carry energy. The energy density in fields E and B:

Electric field energy density uE = ½ε₀E²
Magnetic field energy density uB = B²/(2μ₀)

Since E = cB and c = 1/√(ε₀μ₀), the two contributions are equal: uE = uB.

Total EM energy density u = ε₀E² = B²/μ₀ = ε₀E·cB

Intensity (Irradiance)

Intensity = power per unit area (W/m²). For a plane EM wave with peak fields E₀ and B₀:

Intensity of EM wave (Eq. 22-7) I = Savg = ½c·ε₀·E₀² = (E₀B₀)/(2μ₀) = c·ε₀·Erms²
RMS fields Erms = E₀/√2,    Brms = B₀/√2
Poynting vector S: The instantaneous power per area carried by an EM wave is S = cε₀E² = (EB)/μ₀. The time-averaged value is I = Savg = ½cε₀E₀².

Radiation Pressure

Pressure (fully absorbed) P = I/c
Pressure (fully reflected) P = 2I/c

Radiation pressure is tiny but measurable (demonstrated by Crookes radiometer, solar sails concept).

Inverse Square Law

I = Psource / (4πr²)    (for isotropic source)

E and B amplitudes fall as 1/r; intensity falls as 1/r².

Lecture 9A — Wave Optics: Interference & Diffraction; Refraction

Date: March 3, 2026  |  Sections: 24.1–24.7, 23.1–23.2, 23.4–23.6

§24.1 — Waves vs. Rays; Huygens' Principle

Huygens' Principle: Every point on a wavefront acts as a source of secondary spherical wavelets. The new wavefront is the envelope of these wavelets after a time Δt.

This explains reflection and refraction using wave theory. It also explains why light bends around corners (diffraction) — prominent when λ is comparable to slit/obstacle size.

When to use wave optics: When slit/obstacle size ≈ λ (diffraction is important).
When to use ray optics: When slit/obstacle ≫ λ (geometric optics is a good approximation).

§24.2 — Young's Double-Slit Experiment

Two narrow slits separated by distance d are illuminated by coherent light (wavelength λ). Waves from the two slits interfere, producing alternating bright and dark fringes on a screen at distance L.

Constructive interference (bright fringes) d sin θ = mλ    m = 0, ±1, ±2, …
Destructive interference (dark fringes) d sin θ = (m + ½)λ    m = 0, ±1, ±2, …
Fringe spacing on screen (small angle: sin θ ≈ tan θ = y/L) ym = mλL/d    (position of m-th bright fringe)    Fringe spacing: Δy = λL/d
d m=0 m=1 → light L (screen distance)
Young's double-slit. Bright fringes where path difference = mλ. Fringe spacing Δy = λL/d.
Phase difference: Path difference δ = d sin θ. Constructive: δ = mλ (integer wavelengths). Destructive: δ = (m+½)λ (half-integer wavelengths). Two sources must be coherent (same frequency, constant phase relationship).

Index of Refraction and Wavelength in a Medium

Wavelength in medium with index n λn = λ / n    (frequency unchanged: f = c/λ = v/λn)

§24.4 — Diffraction Grating

A diffraction grating has many closely spaced slits (N slits, spacing d). The condition for bright maxima is the same as double-slit, but the peaks are much sharper and brighter:

Diffraction Grating — Principal Maxima d sin θ = mλ    m = 0, ±1, ±2, …    (m = order)

where d = 1/(number of lines per meter) = grating spacing.

Advantages over double-slit: Many slits → very sharp, bright maxima (narrow peaks). Used in spectrometers to measure wavelengths with high precision. White light → each wavelength appears at a different angle.

Resolving Power

R = λ/Δλ = mN    (m = order, N = total number of slits)

§24.5 — Single-Slit Diffraction

Even a single slit of width a produces a diffraction pattern. Minima occur where:

Single-Slit — Dark Fringes (minima) a sin θ = mλ    m = ±1, ±2, ±3, …    (NOT m = 0)
Note: m = 0 is the central maximum (not a minimum!). Minima at m = ±1, ±2, … The central maximum has double the width of the other maxima.

Central maximum width: Δy = 2λL/a. Narrower slit → wider diffraction pattern (inverse relationship).

a Central max m=1 m=-1 ← dark (m=1) ← dark (m=-1) a sinθ = mλ (minima)
Single-slit diffraction intensity pattern. Minima at a sinθ = mλ (m ≠ 0).

§24.6 — Diffraction and the Double-Slit

The actual double-slit pattern is the product of the two-slit interference pattern and the single-slit diffraction envelope. Some interference maxima may be "missing" if they coincide with single-slit minima.

Missing order when:   mdouble-slit = m' · (d/a)   where m' is a single-slit minimum order

§24.7 — Thin-Film Interference

When light reflects from a thin film (e.g., soap bubble, oil slick), rays reflecting from the top and bottom surfaces may interfere. The path difference is 2t (twice the film thickness for normal incidence).

Phase Shift on Reflection

Phase shift rule: When light reflects from a surface where it goes from lower to higher n, it undergoes a 180° phase shift (equivalent to λ/2 path difference). No phase shift when going from higher to lower n.
ConditionBright (constructive)Dark (destructive)
0 or 2 phase shifts (both or neither surfaces shift)2t = mλn2t = (m+½)λn
1 phase shift (one surface shifts)2t = (m+½)λn2t = mλn

where λn = λ/n is the wavelength inside the film (n = index of film).

Thin-film: path difference in film 2t = mλ/n    or    2nt = mλ    (bright, with one phase shift)
Examples:
  • Soap film (n ≈ 1.33) in air: one phase shift (at top surface only) → 2nt = (m+½)λ for bright
  • Oil (n = 1.5) on water (n = 1.33): both surfaces shift → 2nt = mλ for bright
  • Anti-reflection coating: one phase shift, thickness = λ/(4n) → destructive reflection

Newton's Rings

Circular thin-film interference rings formed between a convex lens and a flat glass surface. Central spot is dark (one phase shift, t→0).

§23.1 — The Ray Model of Light

Light travels in straight-line paths called rays when λ ≪ size of obstacles. This is the basis of geometric optics. Ray model successfully explains reflection, refraction, and image formation.

§23.2 — Reflection; Plane Mirror Images

Law of Reflection θr = θi    (angle of reflection = angle of incidence, measured from normal)

Plane mirror: Virtual, upright image. Image distance = object distance (di = do behind mirror). Image same size as object. Mirror need only be half person's height for full-body view.

Real image: Light rays actually converge at image point. Can be projected on screen.
Virtual image: Rays only appear to diverge from image point (don't pass through it). Cannot be projected.

§23.4 — Refraction; Snell's Law

When light crosses a boundary between media with different indices of refraction, it bends. Snell's Law:

Snell's Law of Refraction n₁ sin θ₁ = n₂ sin θ₂

n = index of refraction = c/v. Light bends toward the normal when entering a denser medium (n₂ > n₁), away from normal when entering less dense.

MediumIndex nSpeed v = c/n
Vacuum1.0003.00 × 10⁸ m/s
Air1.0003 ≈ 1.00≈ c
Water1.332.26 × 10⁸ m/s
Glass (crown)1.521.97 × 10⁸ m/s
Diamond2.421.24 × 10⁸ m/s
n₁ (air) n₂ (glass, n₂>n₁) θ₁ θ₂
Snell's Law: n₁ sin θ₁ = n₂ sin θ₂. Light bends toward normal entering denser medium.

§23.5 — Total Internal Reflection (TIR)

When light travels from denser (n₁) to less dense (n₂) medium, and θ₁ exceeds the critical angle θc, light is totally reflected (no refracted ray):

Critical Angle for TIR (n₁ > n₂) sin θc = n₂ / n₁    (if n₂ = air ≈ 1: sin θc = 1/n₁)
Applications of TIR:
  • Optical fibers: Light trapped by TIR at glass–air boundary; used in communications and medical scopes
  • Prism binoculars: 45°-45°-90° prisms (n ≈ 1.5, θc = 41.8°) fold light path
  • Diamonds: Very high n (2.42), small θc (24.4°) → lots of internal reflections → brilliance

§23.6 — Visible Spectrum and Dispersion

Glass has different n for different wavelengths: n is slightly larger for violet (shorter λ) than red (longer λ). This dispersion causes a prism to split white light into a spectrum. Rainbows are caused by dispersion in water droplets.

Lecture 9B — Geometric Optics: Mirrors & Lenses

Date: March 5, 2026  |  Sections: 23.3, 23.7–23.10

§23.3 — Formation of Images by Spherical Mirrors

Focal Length of a Spherical Mirror

For a concave spherical mirror with radius of curvature r, parallel rays converge at the focal point F. The focal length:

Focal length of spherical mirror (Eq. 23-1) f = r / 2

Valid for paraxial rays (small angles only). Concave mirror: f > 0. Convex mirror: f < 0.

Mirror Equation

Mirror Equation (Eq. 23-2) 1/do + 1/di = 1/f = 2/r
Lateral Magnification (Eq. 23-3) m = hi/ho = −di/do

Sign Conventions for Mirrors

QuantityPositive (+)Negative (−)
doObject in front of mirrorObject behind mirror (virtual object)
diImage in front of mirror (real)Image behind mirror (virtual)
fConcave mirrorConvex mirror
mImage uprightImage inverted

Ray Diagram Rules for Mirrors

Three principal rays from object point O': Ray 1: Parallel to axis → reflects through F (concave) or away from F (convex) Ray 2: Through F → reflects parallel to axis Ray 3: Through center of curvature C → reflects back on itself Image I' forms where reflected rays intersect (real) or appear to intersect behind mirror (virtual)

Cases for Concave Mirrors

Object locationImage typeImage locationOrientationSize
do > 2f (beyond C)Realf < di < 2fInvertedReduced
do = 2f (at C)Realdi = 2fInvertedSame size
f < do < 2fRealdi > 2fInvertedEnlarged
do = fdi = ∞
do < f (inside F)VirtualBehind mirrorUprightEnlarged
Convex mirror: Always forms virtual, upright, reduced image regardless of object position. Wide field of view → used as security/rearview mirrors. f is negative.

§23.7 — Thin Lenses

A lens refracts light at two surfaces. A converging lens (thicker at center) has positive focal length; a diverging lens (thinner at center) has negative focal length.

Converging (+ lens) F Diverging (− lens) F (virtual)
Converging lens focuses parallel rays at real focal point F. Diverging lens causes rays to spread from virtual F.

Lens Types

ShapeNamef
Biconvex, plano-convex, converging meniscusConvergingf > 0
Biconcave, plano-concave, diverging meniscusDivergingf < 0

§23.8 — The Thin Lens Equation

Thin Lens Equation (same form as mirror equation) 1/do + 1/di = 1/f
Lateral Magnification m = hi/ho = −di/do

Sign Conventions for Thin Lenses

QuantityPositive (+)Negative (−)
doObject on incoming light sideVirtual object
diImage on outgoing side (real)Image on same side as object (virtual)
fConverging lensDiverging lens
mImage uprightImage inverted

Lens Power (Diopters)

P = 1/f    [diopters, D; f in meters]    Example: f = 25 cm → P = +4.0 D

Ray Diagram Rules for Lenses

Three principal rays (for converging lens): Ray 1: Parallel to axis → refracts through far focal point F₂ Ray 2: Through optical center (midpoint of lens) → passes straight through Ray 3: Through near focal point F₁ → refracts parallel to axis Image forms where refracted rays intersect (real) or appear to diverge from (virtual, same side as object)

Image Cases for Converging Lens

Object locationImageOrientationSizeType
do > 2ff < di < 2fInvertedReducedReal
do = 2fdi = 2fInvertedSameReal
f < do < 2fdi > 2fInvertedEnlargedReal
do < fSame side as objectUprightEnlargedVirtual

Diverging lens: always virtual, upright, reduced image.

§23.9 — Combinations of Lenses

For two thin lenses in contact or close together:

1/ftotal = 1/f₁ + 1/f₂    or    Ptotal = P₁ + P₂

For separated lenses: treat each lens sequentially. The image from lens 1 becomes the object for lens 2.

§23.10 — Lensmaker's Equation

Lensmaker's Equation 1/f = (n−1)[1/R₁ − 1/R₂]

where R₁, R₂ are radii of curvature of lens surfaces (positive if center of curvature is on the far side).

Lecture 10A — Optical Instruments: Camera, Eye, Magnifier

Date: March 10, 2026  |  Sections: 25.1–25.4

§25.1 — Camera

A camera uses a converging lens to form a real, inverted, reduced image on film/sensor. The image distance is adjusted by moving the lens (focusing).

1/do + 1/di = 1/f    (thin lens equation applies)

f-stop (f-number)

f/# = f / D    (f = focal length, D = aperture diameter)

Common f-stops: f/1.4, f/2, f/2.8, f/4, f/5.6, f/8, f/11, f/16. Each stop halves the light area → doubles exposure time needed. Lower f/# = wider aperture = more light = shallower depth of field.

Depth of field: Range of object distances that appear in focus. Smaller aperture (larger f/#) → greater depth of field.

§25.2 — The Human Eye

The eye is a variable-power optical system. The cornea does most of the refracting (~2/3 of total power). The crystalline lens provides fine adjustment through accommodation (changing shape via ciliary muscles).

Cross-section of Human Eye: Incoming Cornea Lens Retina (sensor) light → ─────┤(n≈1.38)├────────────────────── Vitreous humor (n≈1.337) Image forms on retina (fovea = highest resolution) Signals sent via optic nerve to brain
ParameterValue
Diameter of eye≈ 2.5 cm
Near point (young adult)≈ 25 cm (closest comfortable focus)
Far point (normal eye)∞ (can focus on very distant objects)
Lens power range+18 to +24 D (accommodation range)

§25.3 — Corrective Lenses

Nearsightedness (Myopia)

Far point is closer than infinity — eye too powerful or too long. Cannot focus on distant objects. Corrected with diverging (negative) lens that moves the image of a distant object to the person's far point.

For myopia:   f = −(far point distance)    [far point in meters, f negative]

Farsightedness (Hyperopia)

Near point is farther than 25 cm — eye too weak or too short. Cannot focus on close objects. Corrected with converging (positive) lens that moves a close object's image to the person's near point.

For hyperopia:   1/f = 1/do + 1/di   where do = desired near distance, di = −(near point)

Presbyopia and Astigmatism

  • Presbyopia: Loss of accommodation with age → near point recedes → reading glasses needed
  • Astigmatism: Non-spherical cornea → different focal lengths in different planes → corrected by cylindrical lens

§25.4 — Magnifying Glass (Simple Magnifier)

A converging lens held close to the eye allows an object to be placed closer than the near point (25 cm), producing a larger apparent (angular) size.

Angular Magnification

The angular magnification M compares the angle subtended with the lens to the angle subtended by the object at the near point (25 cm) without the lens:

Magnification — object at focal point (image at ∞, most relaxed) M = N / f    where N = 25 cm (near point), f = focal length [cm]
Magnification — image at near point N (maximum magnification) M = N/f + 1 = 25/f + 1
Example: A 5 cm focal length magnifier: M = 25/5 = 5× (relaxed eye) or M = 25/5 + 1 = 6× (image at near point). For comfortable, relaxed viewing, use M = N/f.
Why it works: The lens creates a virtual, upright, enlarged image on the same side as the object. The eye sees this virtual image as if it were at infinity (or at least beyond the near point).

Lecture 10B — Optical Instruments: Microscopes, Telescopes, Aberrations

Date: March 12, 2026  |  Sections: 25.5–25.9

§25.5 — Compound Microscope

A compound microscope uses two converging lenses to achieve high magnification of nearby objects:

  • Objective lens (short f, fobj ≈ mm–cm): object placed just beyond Fobj → forms real, inverted, magnified image I'
  • Eyepiece (ocular) (acts as magnifying glass): I' serves as object just inside Feye → forms virtual, enlarged image seen by eye
Compound Microscope layout: Object Objective Intermediate Eyepiece Eye O ───────[ f_obj ]──── I' ────[ f_eye ]──→ ↑very close ↑real ↑virtual just beyond F_obj enlarged final image inverted

Total Magnification

Microscope magnification (Eq. 25-6) Mtotal = Mobj × Meye = (−di,obj / do,obj) × (N / feye)
Simplified (for standard tube length ℓ ≈ 16 cm, N = 25 cm) M ≈ (ℓ / fobj) × (N / feye) = (ℓ · N) / (fobj · feye)

where ℓ is the distance between the objective's back focal point and the front focal point of the eyepiece (the "tube length", typically ≈ 16 cm or 18 cm).

Example: fobj = 0.80 cm, feye = 2.5 cm, ℓ = 16 cm, N = 25 cm:
M = (16/0.80)(25/2.5) = 20 × 10 = 200×

Resolution of a Microscope

Minimum resolvable separation (Rayleigh criterion): δmin = 0.61λ / (n sin θ) where n sin θ is the numerical aperture (NA). Shorter wavelength → better resolution (electron microscopes use e⁻ waves with very short λ).

§25.6 — Telescopes

Telescopes magnify distant objects. Two main types:

Refracting Telescope

Two converging lenses. Objective has long focal length; eyepiece has short focal length. Object at ∞ → objective forms real image at its focal point → eyepiece acts as magnifier.

Telescope angular magnification (Eq. 25-9) M = −fobj / feye    (negative = inverted image)

The two lenses are separated by fobj + feye (sum of focal lengths) when viewing an object at infinity.

Refracting telescope (Keplerian type): Distant Objective Eyepiece Eye object ─── [ f_obj ] ──── [f_eye] ────→ ←─────────────────────────→ f_obj + f_eye (tube length) Final image at ∞ (inverted)

Reflecting Telescope

Uses a large concave mirror as the objective instead of a lens. Advantages:

  • No chromatic aberration (mirrors reflect all wavelengths equally)
  • Easier to build very large diameter mirrors than lenses
  • Parabolic mirrors eliminate spherical aberration
  • Can use CCD sensor at prime focus directly

Designs: Newtonian focus (flat secondary mirror at 45°), Cassegrain (convex secondary through hole in primary).

M = −fmirror / feye    (same formula as refracting telescope)

Terrestrial Telescopes

  • Galilean telescope: Diverging eyepiece → upright image, compact, no field lens (opera glasses)
  • Spyglass (erector type): Extra erecting lens to flip image upright
  • Binoculars: Use two Porro prisms (TIR) to fold light path and produce upright image; effectively have long fobj in compact body

Light-Gathering Power

Proportional to area of objective: ∝ D2. Larger aperture → fainter objects visible. This, not magnification, is why astronomers want big telescopes.

§25.7 — Lens Aberrations

Spherical Aberration

Rays far from the optical axis focus at a different point than paraxial rays. Corrected by: compound lens systems, aspherical lenses, stopping down aperture.

Chromatic Aberration

Since n varies with λ (dispersion), different colors focus at different points. Corrected by an achromatic doublet: a converging and diverging lens of different glass types cemented together. Mirrors have no chromatic aberration.

Other Aberrations

  • Coma: Off-axis points form comet-shaped blurs
  • Astigmatism: Off-axis rays in different planes focus at different distances
  • Field curvature: Image forms on curved surface, not flat
  • Distortion: Magnification varies with distance from axis

§25.8 — Limits of Resolution; Rayleigh Criterion

Due to diffraction, even a perfect lens cannot form a perfect point image. Two point sources can just be resolved when the central maximum of one coincides with the first minimum of the other:

Rayleigh Criterion — circular aperture θmin = 1.22 λ/D    (radians)    [D = aperture diameter, λ = wavelength]

Smaller θmin (better resolution) requires: larger D or shorter λ.

Minimum resolvable distance at range L smin = 1.22 λL/D

§25.9 — Specialty Instruments

InstrumentPrincipleKey formula
Spectrometer / spectroscopeDiffraction grating separates wavelengthsd sin θ = mλ
Interferometer (Michelson)Path difference → interference fringesΔL = mλ/2 (bright)
Fiber optic scope (endoscope)TIR keeps light in fibersin θc = n₂/n₁

Lecture 11A — Final Exam

Date: March 16, 2026  |  Cumulative: Chapters 16–25

Cumulative Topics — Final Exam

The final covers everything from the term. Use the equation reference below as your master sheet.

  • Electrostatics (Ch. 16–17): Coulomb, E-field, Gauss, V, capacitance, dielectrics, energy storage
  • Circuits (Ch. 18–19): Ohm's law, resistivity, EMF/terminal voltage, series/parallel, Kirchhoff, RC, AC, power, hazards
  • Magnetism (Ch. 20): Force on charges/wires, cyclotron motion, B from wire/loop/solenoid, Ampère, Hall, torque on loops
  • EM Induction (Ch. 21): Faraday/Lenz, motional EMF, generators, transformers, inductance, RL, LC resonance
  • EM Waves (Ch. 22): Maxwell's equations, c = 1/√(ε₀μ₀), spectrum, intensity, radiation pressure
  • Wave Optics (Ch. 24): Huygens, double-slit, gratings, single-slit, thin films
  • Geometric Optics (Ch. 23): Reflection, Snell, TIR, mirrors, lenses, lensmaker's equation
  • Optical Instruments (Ch. 25): Camera, eye, magnifier, microscope, telescope, Rayleigh criterion
Strategy: Re-work the assigned problems from each chapter; many final questions are minor variations. Make sure you can recite (a) the four Maxwell equations, (b) right-hand rules for B and induced current, (c) sign conventions for the lens/mirror equation. These are the most common quick-recall items.

Quick Reference — All Key Equations

Complete formula sheet for exams

Chapter 16 — Electric Charge & Field

Coulomb's LawF = kQ₁Q₂/r²
Coulomb constantk = 1/(4πε₀) = 8.99×10⁹ N·m²/C²
Electric field (definition)E = F/q
Field of point chargeE = kQ/r²
Field of infinite lineE = λ/(2πε₀r)
Field of infinite planeE = σ/(2ε₀)
Field at conductor surfaceE = σ/ε₀
Gauss's Law∮ E·dA = Qencl/ε₀

Chapter 17 — Potential & Capacitance

Potential differenceVba = ΔU/q
V in uniform fieldV = −E·d
V of point chargeV = kQ/r
PE of two chargesU = kQ₁Q₂/r
Electron-volt1 eV = 1.6×10⁻¹⁹ J
Capacitance definitionC = Q/V
Parallel-plate capacitorC = ε₀A/d
With dielectricC = K ε₀ A/d
Energy in capacitorU = ½CV² = Q²/(2C)
Electric energy densityu = ½ε₀E²

Chapter 18–19 — Current & DC Circuits

CurrentI = ΔQ/Δt
Ohm's lawV = IR
Resistance from resistivityR = ρℓ/A
Resistivity vs. tempρ = ρ₀[1+α(T−T₀)]
Microscopic currentI = neAvd
Power dissipatedP = IV = I²R = V²/R
RMS valuesVrms = V₀/√2, Irms = I₀/√2
Avg AC powerP̄ = IrmsVrms
Terminal voltageVab = ε − Ir
Resistors in seriesReq = ΣRi
Resistors in parallel1/Req = Σ1/Ri
Capacitors in series1/Ceq = Σ1/Ci
Capacitors in parallelCeq = ΣCi
RC chargingQ = Qmax(1 − e−t/RC)
RC dischargingQ = Q₀ e−t/RC
RC time constantτ = RC

Chapter 20 — Magnetism

Force on currentF = IℓB sin θ
Force on moving chargeF = qvB sin θ
Cyclotron radiusr = mv/(qB)
Cyclotron frequencyf = qB/(2πm)
B of long straight wireB = μ₀I/(2πr)
B inside solenoidB = μ₀nI
B of toroidB = μ₀NI/(2πr)
Force between // wiresF/ℓ = μ₀I₁I₂/(2πd)
Hall voltageVH = vdBw
Torque on loopτ = NIAB sin θ
Magnetic dipole momentμ = NIA
Energy of dipoleU = −μB cos θ
Ampère's Law∮ B·dℓ = μ₀ Iencl

Chapter 21 — EM Induction & Circuits

Faraday's Lawε = −NΔΦB/Δt
Motional EMFε = Bℓv
Magnetic FluxΦB = BA cos θ
Generator EMFε = NBAω sin(ωt)
Transformer voltageVS/VP = NS/NP
Transformer currentIS/IP = NP/NS
Self-inductance EMFε = −L(ΔI/Δt)
Solenoid inductanceL = μ₀N²A/ℓ
Energy in inductorU = ½LI²
Magnetic energy densityu = B²/(2μ₀)
RL current (rise)I = (V/R)(1 − e−t/τ)
RL time constantτ = L/R
Inductive reactanceXL = 2πfL = ωL
Capacitive reactanceXC = 1/(2πfC)
LRC impedanceZ = √(R² + (XL−XC)²)
LC resonance frequencyf₀ = 1/(2π√(LC))

Chapter 22 — Electromagnetic Waves

Speed of lightc = 1/√(ε₀μ₀) = 3.00×10⁸ m/s
E and B relationE/B = c
Wave equationc = fλ
EM energy densityu = ε₀E² = B²/μ₀
EM wave intensityI = ½cε₀E₀²
Radiation pressure (absorbed)P = I/c
Radiation pressure (reflected)P = 2I/c
Inverse square lawI = Psrc/(4πr²)

Chapter 23 — Geometric Optics

Law of reflectionθr = θi
Snell's Lawn₁ sin θ₁ = n₂ sin θ₂
Index of refractionn = c/v
Critical angle (TIR)sin θc = n₂/n₁
Mirror focal lengthf = r/2
Mirror/Lens equation1/do + 1/di = 1/f
Magnificationm = −di/do
Lens powerP = 1/f [diopters]
Lensmaker's equation1/f = (n−1)(1/R₁ − 1/R₂)

Chapter 24 — Wave Nature of Light

Double-slit bright fringesd sin θ = mλ
Double-slit dark fringesd sin θ = (m+½)λ
Fringe positionym = mλL/d
Diffraction grating maximad sin θ = mλ
Single-slit minimaa sin θ = mλ (m≠0)
Wavelength in mediumλn = λ/n
Thin-film (1 phase shift, bright)2nt = (m+½)λ
Thin-film (0 or 2 shifts, bright)2nt = mλ

Chapter 25 — Optical Instruments

Simple magnifier (relaxed)M = N/f = 25 cm/f
Simple magnifier (max)M = N/f + 1
Microscope magnificationM = (ℓ/fobj)(N/feye)
Telescope magnificationM = −fobj/feye
Rayleigh criterionθmin = 1.22λ/D
Camera f-numberf/# = f/D

Maxwell's Equations (Summary)

1. Gauss's Law — Electric∮ E·dA = Qencl/ε₀    (charges are sources of E)
2. Gauss's Law — Magnetic∮ B·dA = 0    (no magnetic monopoles)
3. Faraday's Law∮ E·dl = −dΦB/dt    (changing B → E)
4. Ampère–Maxwell Law∮ B·dl = μ₀I + μ₀ε₀(dΦE/dt)    (I or changing E → B)

Important Constants

ConstantSymbolValue
Speed of lightc3.00 × 10⁸ m/s
Permittivity of free spaceε₀8.85 × 10⁻¹² C²/(N·m²)
Permeability of free spaceμ₀4π × 10⁻⁷ T·m/A = 1.257 × 10⁻⁶ T·m/A
Near point (standard)N25 cm = 0.25 m
Euler's numbere2.718…