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The Timpson Lyceum · University Physics II (2026) – Electricity & Magnetism

Magnetic Field and Magnetic Forces – Lecture 9 (University Physics II)

Overview

Everything up to this point has concerned electric fields and their effect on charges. This lecture opens the second half of the course by introducing the magnetic field B⃗\vec{B} — a field that acts only on moving charges, and whose force is perpendicular to both the velocity and the field itself. Two facts are taken as experimental givens rather than derived: magnetic monopoles do not exist, and a moving charge in a magnetic field feels a force F⃗=qv⃗×B⃗\vec{F} = q\vec{v} \times \vec{B}. From those two starting points follow Gauss's law for magnetism (the second of Maxwell's equations), the circular and helical paths charged particles trace out in a uniform field, the velocity selector and the measurement of the electron's mass, and finally the force and torque on current-carrying wires and loops. The recurring difficulty is geometric: magnetism is irreducibly three-dimensional, and the right-hand rule has to be applied deliberately rather than intuitively.

Key Concepts

Magnets, poles, and monopoles

The magnetic force on a moving charge

F⃗=q v⃗×B⃗\vec{F} = q\,\vec{v} \times \vec{B} F=∣q∣ vBsin⁡θF = |q|\,v B \sin\theta

where θ\theta is the angle between v⃗\vec{v} and B⃗\vec{B}. When v⃗∥B⃗\vec{v} \parallel \vec{B}, sin⁡θ=0\sin\theta = 0 and there is no force at all. The force is maximum when they are perpendicular.

Magnetic flux and Gauss's law for magnetism

ΦB=BAcos⁡ϕ\Phi_B = B A \cos\phi

where ϕ\phi is the angle between B⃗\vec{B} and the area vector (the normal to the surface). Flux is maximum when the area vector is parallel to B⃗\vec{B} and zero when it is perpendicular. For a non-uniform field or curved surface, integrate over patches: ΦB=∫B⃗⋅dA⃗\Phi_B = \int \vec{B} \cdot d\vec{A}. For a closed surface, the outward normal is taken as positive by convention.

∮B⃗⋅dA⃗=0\oint \vec{B} \cdot d\vec{A} = 0

This is the second of Maxwell's four equations, and it is a direct statement that magnetic monopoles do not exist.

Motion of a charged particle in a uniform field

R=mv∣q∣BR = \frac{mv}{|q|B}

A stronger field or a larger charge tightens the circle; a larger mass or a larger speed widens it.

ω=∣q∣BmT=2πω=2πm∣q∣B\begin{aligned} \omega &= \frac{|q|B}{m} \\ T &= \frac{2\pi}{\omega} = \frac{2\pi m}{|q|B} \end{aligned}

Remarkably, neither depends on the speed or the radius. Two identical particles launched at very different speeds in the same field complete their (very different-sized) circles in exactly the same time. This is the principle behind the cyclotron, which flips the polarity of its accelerating gaps at that fixed frequency.

Applications: velocity selector and the mass of the electron

v=EBv = \frac{E}{B}

travel straight through. Slower particles are deflected by the stronger electric force; faster ones by the stronger magnetic force.

F⃗=q(E⃗+v⃗×B⃗)\vec{F} = q\left(\vec{E} + \vec{v} \times \vec{B}\right)

Maxwell's equations describe how the fields behave; the Lorentz force law is the separate ingredient that tells how those fields act on matter. Together with Newtonian mechanics, they form the complete framework of classical electromagnetism.

Magnetic forces on currents

dF⃗=I dl⃗×B⃗d\vec{F} = I\,d\vec{l} \times \vec{B}

For a straight wire of length LL in a uniform field, this becomes F⃗=IL⃗×B⃗\vec{F} = I\vec{L} \times \vec{B}, with magnitude ILBsin⁡θILB\sin\theta. A wire carrying no current feels no force, and a wire parallel to B⃗\vec{B} feels no force. Note that current itself is never treated as a vector — it is a global property of the wire — so the direction is carried by dl⃗d\vec{l}.

τ=2(b2)(IaB)sin⁡ϕ=IABsin⁡ϕ\tau = 2\left(\frac{b}{2}\right)(IaB)\sin\phi = IAB\sin\phi

where A=abA = ab is the loop area and ϕ\phi is the angle between the area vector and B⃗\vec{B} — the same angle used for flux, which is why torque and flux tie together naturally.

τ⃗=μ⃗×B⃗U=−μ⃗⋅B⃗=−μBcos⁡ϕ\begin{aligned} \vec{\tau} &= \vec{\mu} \times \vec{B} \\ U &= -\vec{\mu} \cdot \vec{B} = -\mu B \cos\phi \end{aligned}

The potential energy follows from integrating the work done by the torque, W=∫τ dϕW = \int \tau\, d\phi, and requiring that it equal the change in UU.

Worked Example

A proton (q=1.6×10−19 Cq = 1.6 \times 10^{-19}\,\text{C}, m=1.67×10−27 kgm = 1.67 \times 10^{-27}\,\text{kg}) moves in a uniform field B=0.5 TB = 0.5\ \text{T} pointing along the xx-axis. Its initial velocity is vx=1.5×105 m/sv_x = 1.5 \times 10^5\ \text{m/s} and vy=2.0×105 m/sv_y = 2.0 \times 10^5\ \text{m/s}, with vz=0v_z = 0. Find the initial force, the initial acceleration, the radius of the helix, the period, and the pitch.

Only the component of velocity perpendicular to B⃗\vec{B} contributes to the force. Here B⃗\vec{B} lies along xx, so vxv_x produces nothing and only vyv_y matters; by the right-hand rule the force points along −z-z:

F=∣q∣ v⊥B=(1.6×10−19 C)(2.0×105 m/s)(0.5 T)=1.6×10−14 N\begin{aligned} F &= |q|\,v_\perp B \\ &= (1.6 \times 10^{-19}\,\text{C})(2.0 \times 10^5\,\text{m/s})(0.5\,\text{T}) = 1.6 \times 10^{-14}\,\text{N} \end{aligned}

The acceleration follows from Newton's second law:

a=Fm=1.6×10−14 N1.67×10−27 kg=9.5×1012 m/s2\begin{aligned} a &= \frac{F}{m} \\ &= \frac{1.6 \times 10^{-14}\,\text{N}}{1.67 \times 10^{-27}\,\text{kg}} = 9.5 \times 10^{12}\ \text{m/s}^2 \end{aligned}

The radius uses the perpendicular velocity only, since that is the part executing circular motion:

R=mv⊥∣q∣B=(1.67×10−27 kg)(2.0×105 m/s)(1.6×10−19 C)(0.5 T)=4.2×10−3 m\begin{aligned} R &= \frac{m v_\perp}{|q|B} \\ &= \frac{(1.67 \times 10^{-27}\,\text{kg})(2.0 \times 10^5\,\text{m/s})}{(1.6 \times 10^{-19}\,\text{C})(0.5\,\text{T})} = 4.2 \times 10^{-3}\ \text{m} \end{aligned}

The period depends only on mass, charge, and field — not on the speed or the radius:

T=2πm∣q∣B=2π(1.67×10−27 kg)(1.6×10−19 C)(0.5 T)=1.3×10−7 s\begin{aligned} T &= \frac{2\pi m}{|q|B} \\ &= \frac{2\pi (1.67 \times 10^{-27}\,\text{kg})}{(1.6 \times 10^{-19}\,\text{C})(0.5\,\text{T})} = 1.3 \times 10^{-7}\ \text{s} \end{aligned}

Finally, the pitch is how far the parallel motion advances in one full revolution:

p=v∥T=(1.5×105 m/s)(1.3×10−7 s)=2.0×10−2 m\begin{aligned} p &= v_\parallel T \\ &= (1.5 \times 10^5\,\text{m/s})(1.3 \times 10^{-7}\,\text{s}) = 2.0 \times 10^{-2}\ \text{m} \end{aligned}

The proton therefore spirals along the field in a helix of radius about 4.2 mm, completing over seven million turns per second while advancing 2 cm per turn — and its speed never changes, since the magnetic force does no work.

Summary