SECTION 1
Historical Context & Motivation
For centuries, electricity and magnetism were treated as separate curiosities—static sparks and compass needles had little in common. The story of how scientists unified these forces and learned to predict the paths of charged particles is one of the most exciting narratives in physics. Understanding how charged particles move through electromagnetic fields opened the door to technologies ranging from television screens to particle accelerators, and it remains a cornerstone of modern physics.
1785 • Coulomb's Law
1831 • Faraday's Induction
1865 • Maxwell's Equations
1897 • Thomson's Cathode Ray Experiment
1932 • First Cyclotron
These breakthroughs posed a fundamental question that IB Physics topic D.3 tackles directly: given a charged particle entering a region of electric or magnetic field, what path does it follow, and why? Answering this question requires combining Newton's second law with the force laws for electric and magnetic fields.
SECTION 2
Core Principles & Definitions
Before analysing trajectories, you need to be comfortable with the forces that electromagnetic fields exert on charged particles. Two distinct force rules govern the behaviour: one for electric fields and one for magnetic fields. When both fields are present simultaneously, the total force is called the Lorentz force. Let's break down the key ideas.
Electric Force on a Charge
Magnetic Force on a Moving Charge
The Lorentz Force
Work and Energy
Right-Hand Rule
KEY TAKEAWAY
SECTION 3
Visualising Charged-Particle Trajectories
The diagram below shows three fundamental trajectory types that arise when a charged particle enters a uniform field region. In an electric field oriented perpendicular to the initial velocity, the path curves into a parabola—just like projectile motion under gravity. In a magnetic field perpendicular to the velocity, the particle follows a circle because the force is always centripetal. When the velocity has a component along the magnetic field, the result is a helical (spiral) path.
In the left panel, equally spaced horizontal field lines (pointing downward) create a constant downward force on the positive charge. Because the charge enters horizontally, it behaves exactly like a projectile: constant horizontal velocity, uniformly accelerating vertical velocity, producing a parabolic arc. In the centre panel, the magnetic field points into the page. The magnetic force is always perpendicular to the velocity, acting as a centripetal force that bends the path into a perfect circle. In the right panel, the velocity has a component parallel to B (which is unaffected) and a component perpendicular to B (which creates circular motion), combining into a helix.
SECTION 4
Mathematical Framework
The equations below form the mathematical toolkit for solving D.3 problems. They connect the forces from electric and magnetic fields to the resulting motion via Newton's second law.
ELECTRIC FORCE
F = force on the charge (N), q = charge (C), E = electric field strength (N C−1 or V m−1). The force is parallel to E for positive charges and antiparallel for negative charges.
MAGNETIC FORCE
v = speed of the charge (m s−1), B = magnetic flux density (T), θ = angle between v and B. When v ⊥ B, sin θ = 1 and the force is maximum. When v ∥ B, sin θ = 0 and there is no force.
RADIUS OF CIRCULAR ORBIT IN B
Setting the magnetic force equal to the centripetal force: qvB = mv²/r. Solving for r gives r = mv/(qB). Here m = mass (kg). A faster or heavier particle orbits in a larger circle; a stronger field or larger charge produces a tighter circle.
KINETIC ENERGY FROM ELECTRIC POTENTIAL DIFFERENCE
A charge q accelerated from rest through a potential difference V gains kinetic energy equal to qV. This is used frequently to find the speed of a particle before it enters a magnetic field region.
IB Exam Tip
SECTION 5
The Velocity Selector & Crossed Fields
One of the most elegant applications of combined electric and magnetic fields is the velocity selector (also called a Wien filter). By arranging E and B perpendicular to each other and perpendicular to the particle's velocity, the electric force and the magnetic force act in opposite directions. Only particles travelling at a specific speed pass through undeflected, because at that speed the two forces balance exactly.
The velocity selector is the foundation of the mass spectrometer. After selecting particles of a known speed, they enter a region of magnetic field only. There, each particle follows a semicircular path whose radius depends on its mass (r = mv/(qB)). By measuring the radius, scientists determine the mass of the ion, which reveals its identity. This is how chemists and physicists identify isotopes and unknown compounds.
Remember
SECTION 6
Worked Example — Proton in a Magnetic Field
A proton is accelerated from rest through a potential difference of 500 V and then enters a region of uniform magnetic field B = 0.20 T directed into the page. The proton's velocity is perpendicular to the field. Find (a) the proton's speed upon entering the field and (b) the radius of its circular path. Use mp = 1.67 × 10−27 kg, q = 1.60 × 10−19 C.
Proton Orbit Radius
- 1
Step 1 — Use energy conservation to find speed
The proton starts from rest, so all the electrical potential energy converts to kinetic energy: qV = ½mv². Rearranging for v gives v = √(2qV / m).v = √(2qV / m) - 2
Step 2 — Substitute numerical values
v = √(2 × 1.60 × 10−19 × 500 / 1.67 × 10−27) = √(1.60 × 10−16 / 1.67 × 10−27) = √(9.58 × 1010)v ≈ 3.10 × 10⁵ m s⁻¹ - 3
Step 3 — Apply the orbit radius formula
With v ⊥ B, the magnetic force provides centripetal force: qvB = mv²/r, so r = mv / (qB).r = mv / (qB) - 4
Step 4 — Substitute and calculate
r = (1.67 × 10−27 × 3.10 × 105) / (1.60 × 10−19 × 0.20) = 5.18 × 10−22 / 3.20 × 10−20r ≈ 0.016 m = 1.6 cm - 5
Step 5 — Interpret the result
The proton traces a circle with a radius of about 1.6 cm. This is a small circle, which makes sense because the magnetic field is fairly strong (0.20 T) and the proton's mass is small. Note that the speed does not change—the magnetic field only redirects the proton.
SECTION 7
Electric vs. Magnetic Fields — Key Differences
Students often confuse the effects of electric and magnetic fields on charged particles. The table below highlights the critical differences that IB examiners love to test.
| Property | Electric Field (E) | Magnetic Field (B) |
|---|---|---|
| Force direction | Parallel or antiparallel to E | Perpendicular to both v and B |
| Force on stationary charge | Yes — F = qE always applies | No — charge must be moving |
| Work done | Yes — changes kinetic energy | No — speed is constant |
| Typical trajectory | Straight line (parallel to E) or parabola (perpendicular entry) | Circle (v ⊥ B) or helix (v at angle to B) |
| Depends on charge sign? | Yes — positive and negative deflect opposite ways | Yes — opposite deflection via right-hand rule reversal |
| Depends on mass? | Acceleration a = qE/m depends on mass | Orbit radius r = mv/(qB) depends on mass |
Comparison of electric and magnetic field effects on charged particles
KEY TAKEAWAY
SECTION 8
Connections to Advanced Topics
The principles of D.3 are the building blocks for many technologies and advanced physics topics. Understanding circular motion in a magnetic field, for example, leads directly to how cyclotrons and synchrotrons accelerate particles to near the speed of light. At relativistic speeds, the mass in r = mv/(qB) must be replaced by the relativistic momentum γmv, causing the orbit radius to grow as the particle speeds up.
| D.3 Concept | Advanced Extension |
|---|---|
| r = mv/(qB) for circular orbits | Relativistic momentum: r = γmv/(qB) in synchrotrons; explains why the magnetic field must increase as particles accelerate |
| Velocity selector v = E/B | Mass spectrometry for isotope identification; used in nuclear physics and chemistry analysis |
| Helical motion in B | Charged particles spiral along Earth's magnetic field lines, creating the aurora borealis near the poles |
| Lorentz force F = qE + qv × B | Foundation of the Hall effect, electromagnetic induction (Faraday's law), and plasma confinement in fusion reactors (tokamaks) |
From D.3 basics to cutting-edge applications
If you continue to study physics at university level, you'll encounter the full vector form of the Lorentz force and solve differential equations of motion in non-uniform fields. For now, the key insight is that every electromagnetic technology—from MRI machines to particle colliders—relies on the same force laws you've studied in this lesson, just applied in more complex geometries.
SECTION 9
Practice Problems
Question 1: CONCEPTUAL
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Question 2: BASIC CALCULATION
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Question 3: INTERMEDIATE
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Question 4: APPLIED
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Question 5: CRITICAL THINKING
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SUMMARY
Lesson Summary
Summary
Charged particles in electric fields experience a force F = qE that acts along the field direction, doing work and changing kinetic energy. This produces straight-line acceleration (when v is parallel to E) or parabolic trajectories (when v is perpendicular to E). In magnetic fields, the force F = qvB sin θ is always perpendicular to the velocity, so it does no work and the particle's speed stays constant. When v is perpendicular to B, the result is uniform circular motion with radius r = mv/(qB); when v has a component along B, a helical path results.
When both fields are present, the Lorentz force F = qE + qv × B governs the motion. A key application is the velocity selector (v = E/B), which allows only particles of a specific speed to pass undeflected. Combined with a magnetic deflection stage, this forms the basis of the mass spectrometer. Remember: electric fields change speed; magnetic fields change direction. Master the right-hand rule for finding force directions and you'll be well prepared for any D.3 exam question.