SL & HL Fields BETA D.3

Motion in Electromagnetic Fields

This topic explores how charged particles and current-carrying conductors behave when subjected to electric and magnetic fields. By analyzing the forces exerted, we can predict trajectories, select particle velocities, and understand the fundamental attraction or repulsion between parallel currents.

Part of IB Physics (2025-2030 syllabus) — Standard and Higher Level.

Key points

  • A uniform electric field exerts a constant force F=qEF = qE on a charge, directed along the field lines for a positive charge and opposite to them for a negative charge, resulting in a parabolic trajectory if the charge enters perpendicular to the field.
  • A magnetic field exerts a velocity-dependent force F=qvBsinθF = qvB\sin\theta perpendicular to both the velocity and the field, causing a charged particle to undergo uniform circular motion when entering perpendicularly.
  • Because the magnetic force is always perpendicular to the direction of motion, a magnetic field does zero work on a free charged particle, changing only its direction and not its kinetic energy.
  • The period of a charged particle's circular motion in a uniform magnetic field, T=2πmqBT = \frac{2\pi m}{qB}, is independent of the particle's speed and orbital radius, which is the principle behind cyclotron accelerators.
  • In combined fields, a velocity selector balances the electric force FE=qEF_E = qE and the magnetic force FB=qvBF_B = qvB to allow only particles of a specific speed v=EBv = \frac{E}{B} to pass through undeflected.
  • The force on a conductor of length LL carrying a current II in a magnetic field BB is given by F=BILsinθF = BIL\sin\theta, oriented according to Fleming's left-hand rule.
  • Parallel wires carrying currents in the same direction attract each other, while those with opposite currents repel each other, due to the magnetic fields they set up around themselves.

Subtopic by subtopic

Charged particles in a uniform electric field

Between two oppositely charged parallel plates the electric field is uniform: the field lines are evenly spaced, parallel, and run from the positive plate to the negative plate. A charge qq in this region experiences a constant force, directed along the field for a positive charge and opposite to it for a negative charge, given by:

F=qEF = qE

A constant force means a constant acceleration a=qEma = \frac{qE}{m}, so the motion is exactly analogous to projectile motion under gravity.

  • A charge released from rest accelerates in a straight line along the field.
  • A charge entering perpendicular to the field keeps a constant velocity component across the plates while accelerating along the field, tracing a parabolic path.

For example, the electron beam in an oscilloscope is steered up and down by a pair of deflection plates in exactly this way.

You should be able to split the motion into independent components, apply the kinematic (suvat) equations along the field direction, and calculate the work done W=qEdW = qEd as the charge moves a distance dd along the field, which equals its gain in kinetic energy.

Charged particles in a uniform magnetic field

A magnetic field pushes on a moving charge with force F=qvBsinθF = qvB\sin\theta, where θ\theta is the angle between the velocity and the field. The force is perpendicular to both the velocity and the field, with a direction given by hand rules (reversed for a negative charge).

When a charged particle enters a uniform magnetic field perpendicularly, the magnetic force acts as a centripetal force: because it is always perpendicular to the velocity, its magnitude stays constant at F=qvBF = qvB while its direction changes continuously, which is exactly the condition for uniform circular motion:

qvB=mv2rqvB = \frac{mv^2}{r}

From this we derive the orbital radius r=mvqBr = \frac{mv}{qB} and the period of rotation T=2πrv=2πmqBT = \frac{2\pi r}{v} = \frac{2\pi m}{qB}. Crucially, the period is completely independent of the particle's speed and radius, which is the fundamental physics principle behind cyclotron accelerators.

Since the force never has a component along the motion, the field does no work: the speed and kinetic energy are unchanged and only the direction turns. A proton and an electron entering the same field curve in opposite senses, and the much lighter electron follows a far tighter circle.

You must be able to find the force direction, calculate rr and TT, and sketch circular arcs of constant radius.

Force on a moving charge (combined electric and magnetic fields)

When a region contains both an electric field and a magnetic field, a moving charge feels two forces at once: the electric force qEqE, which does not depend on the motion, and the magnetic force qvBqvB (for velocity perpendicular to the field), which does.

Arranging the two fields at right angles to each other, so-called crossed fields, makes these forces point in opposite directions for a particle moving perpendicular to both. The forces balance when qE=qvBqE = qvB, which happens for one single speed:

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

Notice that this speed is independent of the particle's charge and mass. This arrangement is a velocity selector: only particles with exactly this speed travel straight through, while faster particles are deflected by the now-dominant magnetic force and slower ones by the electric force.

A velocity selector is used to prepare a beam of known speed, for example before the particles enter a separate field region where their paths are analysed. You should be able to set up the force balance, derive v=EBv = \frac{E}{B}, and predict which way an off-speed particle deflects.

Force on a current-carrying conductor

A current is a flow of charge, so a current-carrying wire placed in a magnetic field feels the combined magnetic force on all of its moving charges. For a straight conductor of length LL carrying current II at angle θ\theta to a field BB, the force is given by:

F=BILsinθF = BIL\sin\theta

The force is largest when the wire is perpendicular to the field and zero when the wire lies along the field lines. The direction is perpendicular to both the wire and the field and comes from Fleming's left-hand rule:

  • first finger along the field
  • second finger along the current
  • thumb giving the force

This motor effect is what makes a coil turn in a DC motor: the two opposite sides of the coil carry current in opposite directions, so they feel forces in opposite directions, producing a turning effect.

For example, a 0.50 m0.50\ \text{m} wire carrying 3.0 A3.0\ \text{A} perpendicular to a 0.20 T0.20\ \text{T} field experiences F=0.20×3.0×0.50=0.30 NF = 0.20 \times 3.0 \times 0.50 = 0.30\ \text{N}.

Be ready to identify θ\theta correctly and to connect this equation to the definition of magnetic flux density and the tesla.

Force between parallel current-carrying wires

Every current creates its own magnetic field, so two current-carrying wires inevitably act on each other. The force between two long parallel wires is an elegant demonstration of Newton's third law and of field interaction.

Wire 1 produces a concentric magnetic field of strength B1=μ0I12πrB_1 = \frac{\mu_0 I_1}{2\pi r} at the position of Wire 2, a distance rr away. Wire 2, carrying current I2I_2, therefore experiences a force F=B1I2LF = B_1 I_2 L along a length LL. Substituting for B1B_1 gives the force per unit length:

FL=μ0I1I22πr\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi r}

By symmetry, Wire 2 exerts an equal and opposite force on Wire 1.

  • Currents in the same direction attract: the field in the gap between the wires is weakened while the field outside is strengthened, pushing the wires together.
  • Currents in opposite directions repel.

You can see this in practice when closely spaced cables carrying large currents jump apart at switch-on.

You should be able to calculate FL\frac{F}{L} using μ0=4π×107 T m A1\mu_0 = 4\pi \times 10^{-7}\ \text{T m A}^{-1}, identify the force direction from the two current directions, and explain the attraction or repulsion using the resultant field pattern.

Formulae

F=qEF = qE

To calculate the electrostatic force acting on a charge qq in a uniform electric field EE.

F=qvBsinθF = qvB \sin\theta

To calculate the magnetic force on a charge qq moving with velocity vv at an angle θ\theta to a magnetic field of strength BB.

r=mvqBr = \frac{mv}{qB}

To find the radius of the circular path of a charged particle moving perpendicular (θ=90\theta = 90^\circ) to a uniform magnetic field.

T=2πmqBT = \frac{2\pi m}{qB}

To find the period of a charged particle's circular motion in a uniform magnetic field; the period does not depend on the particle's speed or orbital radius.

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

To find the speed of particles that pass undeflected through crossed electric and magnetic fields (a velocity selector), where the electric and magnetic forces balance.

F=BILsinθF = BIL \sin\theta

To calculate the force on a straight current-carrying wire of length LL placed in a magnetic field BB at an angle θ\theta to the field lines.

FL=μ0I1I22πr\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi r}

To determine the magnetic force per unit length acting between two long, parallel, current-carrying conductors separated by a distance rr.

Definitions

Magnetic Flux Density (BB)
A measure of the strength of a magnetic field, defined as the force per unit length acting on a conductor carrying a unit current perpendicular to the field lines, measured in Tesla (T\text{T} or N A1m1\text{N A}^{-1}\text{m}^{-1}).
Tesla (T\text{T})
The SI unit of magnetic flux density, where 1 T1\ \text{T} represents a field that exerts a force of 1 N1\ \text{N} on a 1 m1\ \text{m} wire carrying a current of 1 A1\ \text{A} perpendicular to the field.
Velocity Selector
A device consisting of crossed electric and magnetic fields that allows only charged particles of a specific speed v=EBv = \frac{E}{B} to pass through straight without deflection.
Fleming's Left-Hand Rule
A rule for finding the direction of the magnetic force on a current-carrying conductor: with the thumb, first finger and second finger of the left hand held mutually at right angles, the first finger points along the field, the second finger along the conventional current, and the thumb gives the direction of the force.

Worked examples

1

A proton (m=1.67×1027 kgm = 1.67 \times 10^{-27}\ \text{kg}, q=1.60×1019 Cq = 1.60 \times 10^{-19}\ \text{C}) enters a region of uniform magnetic field B=0.50 TB = 0.50\ \text{T} perpendicularly with a velocity of 3.0×106 m s13.0 \times 10^6\ \text{m s}^{-1}. Calculate the radius of its circular orbit and determine the time taken to complete one half-revolution.

  1. 1
    Identify that the magnetic force acts as the centripetal force: qvB=mv2rqvB = \frac{mv^2}{r}.
  2. 2
    Rearrange the formula to solve for the radius: r=mvqBr = \frac{mv}{qB}.
  3. 3
    Substitute the values into the equation: r=(1.67×1027 kg)×(3.0×106 m s1)(1.60×1019 C)×0.50 Tr = \frac{(1.67 \times 10^{-27}\ \text{kg}) \times (3.0 \times 10^6\ \text{m s}^{-1})}{(1.60 \times 10^{-19}\ \text{C}) \times 0.50\ \text{T}}.
  4. 4
    Calculate the radius: r=5.01×10218.00×10200.0626 mr = \frac{5.01 \times 10^{-21}}{8.00 \times 10^{-20}} \approx 0.0626\ \text{m} (or 6.3 cm6.3\ \text{cm} to 2 significant figures).
  5. 5
    Find the time for one half-revolution, which is half of the circular perimeter divided by speed: t=πrvt = \frac{\pi r}{v}.
  6. 6
    Calculate the time: t=π×0.0626 m3.0×106 m s16.6×108 st = \frac{\pi \times 0.0626\ \text{m}}{3.0 \times 10^6\ \text{m s}^{-1}} \approx 6.6 \times 10^{-8}\ \text{s}.

Answer: Radius r=6.3×102 mr = 6.3 \times 10^{-2}\ \text{m}, Time t=6.6×108 st = 6.6 \times 10^{-8}\ \text{s}

2

Two long parallel wires are separated by 5.0 cm5.0\ \text{cm} in a vacuum. Wire 1 carries a current of 4.0 A4.0\ \text{A} upwards. Wire 2 carries a current of 6.0 A6.0\ \text{A} downwards. Calculate the magnetic force per unit length acting on Wire 2 and state whether it is attractive or repulsive.

  1. 1
    Identify the formula for the force per unit length between parallel wires: FL=μ0I1I22πr\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi r}.
  2. 2
    Use the permeability of free space constant, μ0=4π×107 T m A1\mu_0 = 4\pi \times 10^{-7}\ \text{T m A}^{-1}.
  3. 3
    Substitute the given values: FL=(4π×107 T m A1)×4.0 A×6.0 A2π×0.050 m\frac{F}{L} = \frac{(4\pi \times 10^{-7}\ \text{T m A}^{-1}) \times 4.0\ \text{A} \times 6.0\ \text{A}}{2\pi \times 0.050\ \text{m}}.
  4. 4
    Simplify the terms: FL=2×107×24.00.050=9.6×105 N m1\frac{F}{L} = \frac{2 \times 10^{-7} \times 24.0}{0.050} = 9.6 \times 10^{-5}\ \text{N m}^{-1}.
  5. 5
    Determine the nature of the force: since the currents are flowing in opposite directions, the force is repulsive.

Answer: Force per unit length FL=9.6×105 N m1\frac{F}{L} = 9.6 \times 10^{-5}\ \text{N m}^{-1}, repulsive

3

An electron (m=9.11×1031 kgm = 9.11 \times 10^{-31}\ \text{kg}, q=1.60×1019 Cq = 1.60 \times 10^{-19}\ \text{C}) enters the uniform field between two horizontal parallel plates, travelling at 2.0×107 m s12.0 \times 10^{7}\ \text{m s}^{-1} parallel to the plates. The plates are 4.0 cm4.0\ \text{cm} long and the electric field strength between them is 1.5×104 N C11.5 \times 10^{4}\ \text{N C}^{-1}. Calculate the vertical deflection of the electron as it leaves the plates.

  1. 1
    Calculate the electric force on the electron: F=qE=(1.60×1019 C)×(1.5×104 N C1)=2.4×1015 NF = qE = (1.60 \times 10^{-19}\ \text{C}) \times (1.5 \times 10^{4}\ \text{N C}^{-1}) = 2.4 \times 10^{-15}\ \text{N}.
  2. 2
    Find the acceleration along the field direction: a=Fm=2.4×1015 N9.11×1031 kg=2.63×1015 m s2a = \frac{F}{m} = \frac{2.4 \times 10^{-15}\ \text{N}}{9.11 \times 10^{-31}\ \text{kg}} = 2.63 \times 10^{15}\ \text{m s}^{-2}.
  3. 3
    Find the time spent between the plates using the constant horizontal speed: t=Lv=0.040 m2.0×107 m s1=2.0×109 st = \frac{L}{v} = \frac{0.040\ \text{m}}{2.0 \times 10^{7}\ \text{m s}^{-1}} = 2.0 \times 10^{-9}\ \text{s}.
  4. 4
    Treat the motion like a projectile and use y=12at2y = \frac{1}{2}at^2, since the initial velocity along the field direction is zero.
  5. 5
    Substitute the values: y=12×(2.63×1015 m s2)×(2.0×109 s)2=5.3×103 my = \frac{1}{2} \times (2.63 \times 10^{15}\ \text{m s}^{-2}) \times (2.0 \times 10^{-9}\ \text{s})^2 = 5.3 \times 10^{-3}\ \text{m}.

Answer: Vertical deflection y=5.3×103 my = 5.3 \times 10^{-3}\ \text{m} (5.3 mm5.3\ \text{mm})

Common mistakes

  • ×Confusing the shapes of paths in electric versus magnetic fields: a charge entering perpendicular to a uniform electric field follows a parabolic path, whereas in a magnetic field it follows a circular path.
  • ×Assuming a stationary charge experiences a force in a magnetic field: the magnetic force formula F=qvBsinθF = qvB\sin\theta requires a non-zero velocity (v>0v > 0). If v=0v = 0, the force is zero.
  • ×Neglecting the charge's sign when applying right-hand rules: standard hand rules predict the direction of force on a positive charge. If the particle is an electron, you must reverse the final force direction.
  • ×Incorrectly measuring the angle θ\theta: always ensure θ\theta is the angle between the velocity vector (or current direction) and the magnetic field lines, not the angle with the normal.

Exam tips

  • When asked to **explain** why a magnetic field does no work on a moving charge, state that the magnetic force is always perpendicular to the instantaneous velocity vector, meaning the rate of work done (P=FvP = \vec{F} \cdot \vec{v}) is zero.
  • Convert all distances to metres (1 cm=102 m1\ \text{cm} = 10^{-2}\ \text{m}) before substituting into field equations; the wire separation rr in FL=μ0I1I22πr\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi r} is a frequent culprit for this slip.
  • When asked to **sketch** paths, ensure your circular arcs have a constant radius inside a uniform magnetic field, and the path transitions smoothly at the boundaries of the field.
  • Remember that in crossed-field systems (like a velocity selector), you can **deduce** the balance of forces by setting the electric force equal to the magnetic force (qE=qvBqE = qvB), resulting in the speed v=EBv = \frac{E}{B}.

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