Motion of charged particles in magnetic fields Knowledge-Based Study

Physics · Magnetism & Electromagnetism · Physics · Magnetic Fields & Forces

Physics topic explanations on Motion of charged particles in magnetic fields.

Study notes

  1. Lorentz Magnetic Force

    When a particle carrying an electric charge qq moves with a velocity v⃗\vec{v} through a uniform magnetic field B⃗\vec{B}, it experiences a magnetic deflecting force F⃗B\vec{F}_B given by the vector cross product:

    F⃗B=q(v⃗×B⃗)\vec{F}_B = q(\vec{v} \times \vec{B})

    The magnitude of this force is expressed as:

    FB=∣q∣vBsin⁡θF_B = |q|vB\sin\theta

    where θ\theta is the angle between the velocity vector v⃗\vec{v} and the magnetic field vector B⃗\vec{B}.

    Key Characteristics of the Force

    • Zero Force Conditions: The magnetic force is zero if the particle is at rest (v=0v = 0), if the particle is electrically neutral (q=0q = 0), or if the particle moves parallel or antiparallel to the field lines (θ=0∘\theta = 0^\circ or θ=180∘\theta = 180^\circ).
    • Maximum Force: The force reaches its maximum magnitude, FB,max=∣q∣vBF_{B,\text{max}} = |q|vB, when the velocity is perpendicular to the magnetic field (θ=90∘\theta = 90^\circ).
    • Direction and the Right-Hand Rule: For a positive charge, point the fingers of your right hand along v⃗\vec{v} and curl them toward B⃗\vec{B}; your extended thumb points in the direction of F⃗B\vec{F}_B. For a negative charge, the force acts in the directly opposite direction.

    Magnetic Force Does No Work

    Because the magnetic force is defined by a cross product, F⃗B\vec{F}_B is always perpendicular to the instantaneous velocity v⃗\vec{v} (and thus perpendicular to the displacement dr⃗d\vec{r}):

    F⃗B⋅v⃗=0\vec{F}_B \cdot \vec{v} = 0

    According to the work-energy theorem, the rate of work done (power PP) on the charged particle is:

    P=dWdt=F⃗B⋅v⃗=0P = \frac{dW}{dt} = \vec{F}_B \cdot \vec{v} = 0

    Consequently:

    • A static magnetic field does zero work on a moving charged particle.
    • The kinetic energy of the particle remains constant: ΔK=0\Delta K = 0.
    • The particle's speed remains constant, even though its velocity changes continuously in direction.
    • A magnetic field can change the direction of motion, but it cannot speed up or slow down a charged particle.

    Perpendicular Injection (θ=90∘\theta = 90^\circ)

    When a charged particle enters a uniform magnetic field with its velocity strictly perpendicular to B⃗\vec{B}, the magnetic force acts as a centripetal force of constant magnitude. This causes the particle to undergo uniform circular motion in a plane perpendicular to B⃗\vec{B}.

    Equating the magnetic force to the centripetal force:

    ∣q∣vB=mv2r|q|vB = \frac{mv^2}{r}

    Trajectory Parameters

    • Radius of the Orbit (Gyroradius):
      r=mv∣q∣B=p∣q∣Br = \frac{mv}{|q|B} = \frac{p}{|q|B}
      where p=mvp = mv is the linear momentum of the particle. Particles with larger momentum trace out larger circles, while stronger fields produce tighter loops.
    • Period of Revolution:
      The time required for one complete orbit is the circumference divided by the speed:
      T=2πrv=2πm∣q∣BT = \frac{2\pi r}{v} = \frac{2\pi m}{|q|B}
    • Cyclotron Frequency:
      The frequency and angular frequency (cyclotron frequency ω\omega) are given by:
      f=1T=∣q∣B2πm,ω=2πf=∣q∣Bmf = \frac{1}{T} = \frac{|q|B}{2\pi m}, \quad \omega = 2\pi f = \frac{|q|B}{m}

    Crucial Observation: The orbital period TT and cyclotron frequency ω\omega are completely independent of the particle's speed vv and radius rr. Faster particles travel along larger circles, completing each revolution in the exact same duration as slower particles of the same charge-to-mass ratio.

    General Motion (0∘<θ<90∘0^\circ < \theta < 90^\circ)

    If the velocity vector makes an arbitrary angle θ\theta with the magnetic field, we resolve v⃗\vec{v} into components parallel and perpendicular to B⃗\vec{B}:

    • v∥=vcos⁡θv_\parallel = v\cos\theta (parallel to B⃗\vec{B})
    • v⊥=vsin⁡θv_\perp = v\sin\theta (perpendicular to B⃗\vec{B})

    Because F⃗B\vec{F}_B has no component along B⃗\vec{B}, the parallel velocity v∥v_\parallel remains constant, producing uniform linear motion along the field lines. Meanwhile, v⊥v_\perp undergoes uniform circular motion with radius r=mv⊥∣q∣Br = \frac{m v_\perp}{|q|B}.

    The superposition of these two motions results in a helical path (helix). The distance moved along the field axis during one full period is called the pitch (pp):

    p=v∥T=(vcos⁡θ)(2πm∣q∣B)p = v_\parallel T = (v\cos\theta)\left(\frac{2\pi m}{|q|B}\right)

    Practical Applications

    • Velocity Selector: Perpendicular electric and magnetic fields (E⃗⊥B⃗\vec{E} \perp \vec{B}) allow only particles with speed v=EBv = \frac{E}{B} to pass through undeflected.
    • Mass Spectrometer: Ions separated by a velocity selector enter a uniform magnetic field. Since r=mvqBr = \frac{mv}{qB}, measuring the orbital radius reveals the precise mass-to-charge ratio (m/qm/q) of isotopes.
    • Magnetic Confinement: Non-uniform magnetic fields can trap charged particles, causing them to spiral and reflect back between high-field regions (magnetic mirrors), a principle seen in Earth's Van Allen radiation belts and fusion reactors.