← Module 6: Electromagnetism

NSWPhysicsSyllabus dot point

Inquiry Question 2: How does the motion of a charged particle in a magnetic field differ from its motion in an electric field?

Analyse the interaction between charged particles and uniform magnetic fields, including: acceleration, perpendicular to velocity F = qv x B, circular motion of a charged particle moving perpendicular to a uniform magnetic field

A focused answer to the HSC Physics Module 6 dot point on charges moving in magnetic fields. The Lorentz force qv x B, why it does no work, circular motion with radius r = mv/(qB), period T = 2 pi m / (qB), and the right-hand rule for direction.

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What this dot point is asking

NESA wants you to use the Lorentz force law F⃗=qv⃗×B⃗\vec{F} = q \vec{v} \times \vec{B}, recognise that the magnetic force is always perpendicular to the velocity (so does no work and changes only the direction of motion), and apply Newton's second law in the form qvB=mv2/rqvB = mv^2/r to extract the radius and period of circular motion. You should also use the right-hand rule fluently to find the direction of the force.

The answer

The Lorentz force

A particle of charge qq moving with velocity v⃗\vec{v} in a magnetic field B⃗\vec{B} experiences a force:

F⃗=qv⃗×B⃗\vec{F} = q \vec{v} \times \vec{B}

The magnitude is:

F=qvBsin⁑θF = q v B \sin \theta

where θ\theta is the angle between v⃗\vec{v} and B⃗\vec{B}. Key features:

  • If vβƒ—\vec{v} is parallel or antiparallel to Bβƒ—\vec{B} (ΞΈ=0\theta = 0 or 180Β°180Β°), the force is zero. The particle moves in a straight line.
  • If vβƒ—\vec{v} is perpendicular to Bβƒ—\vec{B} (ΞΈ=90Β°\theta = 90Β°), the force has its maximum magnitude F=qvBF = qvB and points perpendicular to both.
  • The direction is given by the right-hand rule (with a sign flip for negative charges).

Units: tesla (T), where 11 T =1= 1 N/(A m).

Why the magnetic force does no work

Because Fβƒ—βŠ₯vβƒ—\vec{F} \perp \vec{v}, the dot product Fβƒ—β‹…dsβƒ—=Fβƒ—β‹…v⃗ dt\vec{F} \cdot d\vec{s} = \vec{F} \cdot \vec{v} \, dt is always zero. The work done over any displacement is zero, so the kinetic energy and hence the speed are constant. The magnetic force can change a particle's direction but never its speed.

This is the deepest difference between electric and magnetic forces: an electric field can accelerate a charge (change its speed); a magnetic field can only steer it.

Circular motion in a uniform field

When a charged particle moves perpendicular to a uniform magnetic field, the constant-magnitude force perpendicular to v⃗\vec{v} provides exactly the centripetal force needed for circular motion. Setting magnetic = centripetal:

qvB=mv2rq v B = \frac{m v^2}{r}

Solving for the radius:

r=mvqB\boxed{r = \frac{m v}{q B}}

Solving for the period (using v=2Ο€r/Tv = 2 \pi r / T):

T=2Ο€rv=2Ο€mqBT = \frac{2 \pi r}{v} = \frac{2 \pi m}{q B}

The period depends only on m/qm/q and BB, not on the speed of the particle. This is the principle behind the cyclotron: particles of all speeds (below relativistic limits) orbit with the same period in a given field.

The frequency f=1/T=qB/(2Ο€m)f = 1/T = qB / (2 \pi m) is called the cyclotron frequency.

Direction: the right-hand rule

For a positive charge:

  1. Point the fingers of your right hand in the direction of v⃗\vec{v}.
  2. Curl them toward B⃗\vec{B} (through the smaller angle).
  3. Your thumb points in the direction of F⃗\vec{F}.

Equivalently (the "slap" rule): flat right hand, fingers along B⃗\vec{B}, thumb along v⃗\vec{v}, palm pushes in the direction of F⃗\vec{F}.

For a negative charge (such as an electron), the force is in the opposite direction to the rule above. Either reverse the rule by using your left hand, or apply the right-hand rule for the positive case and then flip.

The result is that positive charges and negative charges in the same field, moving the same way, orbit in opposite senses.

Worked example: mass spectrometer

A singly-ionised carbon-12 atom is accelerated from rest through 500 V, then enters a uniform magnetic field of 0.200.20 T perpendicular to its velocity. Find the radius of its circular path. (m=1.99Γ—10βˆ’26m = 1.99 \times 10^{-26} kg, q=1.60Γ—10βˆ’19q = 1.60 \times 10^{-19} C.)

Find the speed first. Energy conservation in the accelerator:

IMATH_39
IMATH_40
v=8.04Γ—109=8.97Γ—104v = \sqrt{8.04 \times 10^9} = 8.97 \times 10^4 m/s.

Radius in the magnetic field:

r=mvqB=1.99Γ—10βˆ’26Γ—8.97Γ—1041.60Γ—10βˆ’19Γ—0.20=5.6Γ—10βˆ’2r = \frac{m v}{q B} = \frac{1.99 \times 10^{-26} \times 8.97 \times 10^4}{1.60 \times 10^{-19} \times 0.20} = 5.6 \times 10^{-2} m = 5.6 cm.

This is a mass spectrometer: different isotopes (different mm) yield different radii at the detector, separating them by mass.

Try it: Lorentz force calculator for radius, period, and speed of a charge in a uniform magnetic field.

Common traps

Forgetting the sin⁑θ\sin \theta. F=qvBF = qvB is only the magnitude when vβƒ—βŠ₯Bβƒ—\vec{v} \perp \vec{B}. In other cases use F=qvBsin⁑θF = qvB \sin \theta.

Using F=qEF = qE for a magnetic-field problem. F=qEF = qE is the electric-field force. The magnetic-field force is F=qvBsin⁑θF = qvB \sin \theta. They look similar; mix them up and you lose easy marks.

Applying the right-hand rule to a negative charge without reversing. Always note whether the charge is positive or negative and flip the direction for an electron.

Saying the magnetic force changes the speed. It changes the direction only. Speed and kinetic energy are constant.

Forgetting that TT is independent of vv. The period depends only on m/(qB)m/(qB). Faster particles orbit on larger circles in the same time, not faster.

Mixing up the radius formula. r=mv/(qB)r = mv/(qB), not r=qB/(mv)r = qB/(mv) or r=mvB/qr = mvB/q.

In one sentence

A charged particle moving perpendicular to a uniform magnetic field experiences a force F=qvBF = qvB perpendicular to its velocity, which acts as a centripetal force and produces circular motion of radius r=mv/(qB)r = mv/(qB) and period T=2Ο€m/(qB)T = 2 \pi m / (qB) at constant speed.

Past exam questions, worked

Real questions from past NESA papers on this dot point, with our answer explainer.

2022 HSC5 marksA proton enters a uniform magnetic field of 0.40 T perpendicular to the field direction with a speed of 2.5 x 10^6 m/s. Calculate the radius and period of its circular motion. (m_p = 1.67 x 10^-27 kg, e = 1.60 x 10^-19 C.)
Show worked answer β†’

The magnetic force provides the centripetal force for circular motion:

qvB=mv2rqvB = \frac{m v^2}{r}

Solving for rr:

IMATH_2
r=4.18Γ—10βˆ’216.40Γ—10βˆ’20=6.5Γ—10βˆ’2r = \frac{4.18 \times 10^{-21}}{6.40 \times 10^{-20}} = 6.5 \times 10^{-2} m = 6.5 cm.

Period:

IMATH_4
T=1.05Γ—10βˆ’266.40Γ—10βˆ’20=1.6Γ—10βˆ’7T = \frac{1.05 \times 10^{-26}}{6.40 \times 10^{-20}} = 1.6 \times 10^{-7} s.

Markers reward the explicit equating of magnetic and centripetal force, both formulas r=mv/(qB)r = mv/(qB) and T=2Ο€m/(qB)T = 2 \pi m / (qB), and final answers with units.

2020 HSC3 marksExplain why a charged particle moving through a uniform magnetic field undergoes circular motion at constant speed, rather than spiralling or accelerating along the field direction.
Show worked answer β†’

The magnetic force on a moving charge is F⃗=qv⃗×B⃗\vec{F} = q \vec{v} \times \vec{B}. The cross product means F⃗\vec{F} is always perpendicular to v⃗\vec{v} and to B⃗\vec{B}.

Because F⃗\vec{F} is perpendicular to v⃗\vec{v}, the magnetic force does no work on the particle (W=F⃗⋅d⃗=0W = \vec{F} \cdot \vec{d} = 0). The kinetic energy and hence the speed of the particle remain constant.

A constant-magnitude force perpendicular to the velocity provides centripetal acceleration, which causes circular motion. If the particle has no velocity component along B⃗\vec{B}, the motion is a closed circle; if it does, the motion is a helix (which is outside the standard HSC treatment).

Markers reward the perpendicularity statement, the no-work argument for constant speed, and the centripetal-force conclusion.

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