Charged-Particle Motion in a Uniform Magnetic Field – Comprehensive Notes

Chapter 1 – Uniform Circular Motion of a Charged Particle in a Magnetic Field

  • When a charged particle with velocity v\vec v enters a region of uniform magnetic field B\vec B such that vB\vec v \perp \vec B:

    • Magnetic force: FB=qv×B\vec F_B = q\,\vec v \times \vec B

    • Magnitude: FB=qvBsinθF_B = qvB \sin\theta

      • θ=90sinθ=1FB=qvB\theta = 90^\circ \Rightarrow \sin\theta = 1 \Rightarrow F_B = qvB (maximum force)

      • θ=0 or 180FB=0\theta = 0^\circ \text{ or } 180^\circ \Rightarrow F_B = 0 (no deflection; particle moves undeviated)

    • Direction by right-hand (palm) rule; for negative charge reverse the direction.

Centripetal Force Condition
  • Magnetic force provides the required centripetal force for circular motion: qvB=mv2rqvB = \frac{mv^2}{r}

    • Rearranged for radius:
      r=mvqBr = \frac{mv}{qB}

    • Substitute momentum p=mvp = mv to obtain an alternative form:
      r=pqBr = \frac{p}{qB}

Time Period (Time of Flight for One Revolution)
  • Distance traveled in one full circle: 2πr2\pi r

  • Time period T=distancespeed=2πrvT = \dfrac{\text{distance}}{\text{speed}} = \dfrac{2\pi r}{v}

  • Insert r=mvqBr = \dfrac{mv}{qB}:
    T=2π(mv/qB)v=T=2πmqBT = \frac{2\pi (mv/qB)}{v} = \boxed{T = \frac{2\pi m}{qB}}

Frequency
  • Definition: number of revolutions per second f=1Tf = \dfrac{1}{T}

  • Using the expression for TT:
    f=f=qB2πmf = \boxed{f = \frac{qB}{2\pi m}}

Angular Frequency / Angular Velocity ω\omega
  • Two equivalent relationships used in exams:

    • ω=2πf\omega = 2\pi f

    • ω=2πT\omega = \dfrac{2\pi}{T}

  • Substitute either ff or TT to get:
    ω=qBm\boxed{\omega = \frac{qB}{m}}

  • Key observation: ω\omega, ff, and TT depend only on the charge-to-mass ratio qm\frac{q}{m} and the magnetic field BB, not on the particle’s speed (provided motion is perpendicular to BB).


Chapter 2 – Charges at Rest or Moving Parallel/Antiparallel to B\vec B

  • Charge at rest (v=0v = 0): FB=0F_B = 0 → No acceleration; particle continues with zero velocity.

  • Charge moving parallel or antiparallel to B\vec B (θ=0,180\theta = 0^\circ, 180^\circ): FB=0F_B = 0 → Particle travels straight, undisturbed.


Chapter 3 – Proton vs. Alpha-Particle Properties

  • Proton (symbol pp)

    • Mass: mp=mm_p = m (reference symbol used in the lecture)

    • Charge: qp=qq_p = q

  • Alpha particle (α\alpha) = helium nucleus (4He2+^{4}\text{He}^{2+})

    • Composition: 2 protons + 2 neutrons

    • Mass: mα4mm_\alpha \approx 4m (neutron and proton masses almost equal)

    • Charge: qα=2qq_\alpha = 2q (only the two protons contribute; neutrons are neutral)


Chapter 4 – Sample Problem: Equal-Radius Paths for Proton and Alpha Particle

  • Situation:

    • Uniform B\vec B field (same region & magnitude for both particles)

    • Both enter with velocities perpendicular to B\vec B (ensures circular motion)

    • Radii of the two circular paths are given to be equal: r<em>p=r</em>αr<em>p = r</em>\alpha

Using the Radius–Momentum Relation

r=pqBr = \frac{p}{qB}

  • Set the radii equal and cancel the common BB:
    p<em>pq</em>pB=p<em>αq</em>αB<br>    p<em>pp</em>α=q<em>pq</em>α\frac{p<em>p}{q</em>pB} = \frac{p<em>\alpha}{q</em>\alpha B}<br>\;\Longrightarrow\; \frac{p<em>p}{p</em>\alpha} = \frac{q<em>p}{q</em>\alpha}

  • Insert charges:
    q<em>p=q,  q</em>α=2qp<em>pp</em>α=q2q=12q<em>p = q, \; q</em>\alpha = 2q \Rightarrow \frac{p<em>p}{p</em>\alpha} = \frac{q}{2q} = \boxed{\tfrac{1}{2}}

  • Common exam pitfall (highlighted in the lecture): do not divide by the mass ratio; the formula already involves momentum, not directly the mass.


Chapter 5 – Summary of Key Equations

  • Magnetic force (magnitude): F=qvBsinθF = qvB\sin\theta

  • Centripetal condition for circular motion ((\theta = 90^\circ)):
    qvB=mv2rqvB = \dfrac{mv^2}{r}

  • Radius: r=mvqB=pqBr = \dfrac{mv}{qB} = \dfrac{p}{qB}

  • Time period: T=2πmqBT = \dfrac{2\pi m}{qB}

  • Frequency: f=qB2πmf = \dfrac{qB}{2\pi m}

  • Angular frequency (cyclotron frequency): ω=qBm\omega = \dfrac{qB}{m}


Chapter 6 – Practical & Theoretical Implications

  • Because TT, ff, and ω\omega depend only on qm\frac{q}{m} and BB, all particles with the same charge-to-mass ratio execute circular motion with the same frequency—basis of the cyclotron accelerator.

  • Knowing any one variable (radius, time period, frequency, or angular frequency) lets you derive the others using the boxed formulas.

  • Conceptual checkpoints tested in boards & entrance exams:

    1. Zero magnetic force for vB\vec v \parallel \vec B.

    2. Maximum magnetic force for vB\vec v \perp \vec B.

    3. Derivation of rr, TT, ff, ω\omega from qvB=mv2rqvB = \dfrac{mv^2}{r}.

    4. Comparative questions (e.g.

    • proton vs. alpha particle radii, momenta, frequencies).

    1. Right-hand palm rule direction questions, especially sign reversal for negative charges.

Chapter 1 – How a Charged Particle Moves in a Magnetic Field
  • When a charged particle (like a tiny electron or proton) with speed v enters a uniform magnetic field B (an area with an invisible magnetic push/pull) so that its path is straight across the field lines (vis perpendicular to B):

    • Magnetic force (_F_B): This is the push or pull the magnetic field puts on the moving particle.

      • Its strength (how big the push/pull is): FB=qvBsinθF_B = qvB\sin\theta

      • When the particle moves straight across the field (θ=90\theta = 90^\circ), the force is strongest: FB=qvBF_B = qvB

      • If the particle moves along the field lines (θ=0\theta = 0^\circ or 180180^\circ), there's no force: FB=0F_B = 0 (it just keeps going straight).

    • Direction of force: Use the right-hand (palm) rule. If the particle has a negative charge (like an electron), flip the direction you found.

Why it Moves in a Circle (Centripetal Force)
  • The magnetic force acts like a string, constantly pulling the particle towards the center, making it move in a perfect circle. This "pull-to-center" force is called centripetal force.

    • The magnetic force (qvBqvB) provides the needed centripetal force (mv2r\frac{mv^2}{r}): qvB=mv2rqvB = \frac{mv^2}{r}

  • We can use this to find the radius (r) of the circle the particle makes:

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

  • Since momentum (p) is mass (m) times velocity (v) (p=mvp = mv), we can also write the radius as:

r=pqBr = \frac{p}{qB}

Time for One Full Circle (Time Period)
  • The distance the particle travels in one full circle is the circumference (2πr2\pi r).

  • The time it takes to complete one circle (Time period T) is:

T=distancespeed=2πrvT = \frac{\text{distance}}{\text{speed}} = \frac{2\pi r}{v}

  • If we put in the formula for r:

T=2π(mv/qB)v=T=2πmqBT = \frac{2\pi (mv/qB)}{v} = \boxed{T = \frac{2\pi m}{qB}}

How Many Circles Per Second (Frequency)
  • Frequency (f) is how many full circles the particle makes in one second. It's the opposite of the time period: f=1Tf = \frac{1}{T}

  • Using the formula for T:

f=f=qB2πmf = \boxed{f = \frac{qB}{2\pi m}}

How Fast it Spins (Angular Frequency / Angular Velocity ω\omega)
  • Angular frequency (ω\omega) tells us how fast the particle is spinning in its circle.

    • It's related to frequency and time period by: ω=2πf\omega = 2\pi f or ω=2πT\omega = \frac{2\pi}{T}

  • Using the formula for f or T:

ω=qBm\boxed{\omega = \frac{qB}{m}}

  • Key thing to notice: ω\omega, f, and T depend only on the particle's charge-to-mass ratio (qm\frac{q}{m}) and the magnetic field (BB). They don't depend on how fast the particle is actually moving (its speed v), as long as it's moving straight across the magnetic field.


Chapter 2 – When the Magnetic Field Does Nothing
  • If the charged particle is not moving (v=0v = 0): There's no magnetic force (FB=0F_B = 0). So, it just stays still.

  • If the charged particle moves exactly along the magnetic field lines (either with them or directly against them, θ=0,180\theta = 0^\circ, 180^\circ): There's no magnetic force (FB=0F_B = 0). The particle just keeps moving in a straight line, unaffected.


Chapter 3 – Understanding Protons and Alpha Particles
  • Proton (symbol pp):

    • Mass: Let's call its mass m.

    • Charge: Let's call its charge q (it's a positive charge).

  • Alpha particle (α\alpha) (this is the core of a Helium atom, 4He2+^{4}\text{He}^{2+}):

    • What it's made of: 2 protons + 2 neutrons.

    • Mass: Since neutrons and protons have almost the same mass, an alpha particle is roughly 4 times heavier than a proton (mα4mm_\alpha \approx 4m).

    • Charge: It has a charge of +2 because of its two protons (neutrons have no charge) (qα=2qq_\alpha = 2q).


Chapter 4 – Solving a Problem: Proton vs. Alpha Particle Paths with Same Radius
  • The situation: Imagine a uniform magnetic field (B\vec B) that's the same everywhere. A proton and an alpha particle both enter this field, moving straight across the field lines, and they end up making circles of the exact same size (r<em>p=r</em>αr<em>p = r</em>\alpha).

Using the Radius-Momentum Formula
  • Our formula for radius is: r=pqBr = \frac{p}{qB}

  • Since the radii are equal and the magnetic field B is the same for both, we can set them equal and cancel out B:

p<em>pq</em>pB=p<em>αq</em>αB\frac{p<em>p}{q</em>pB} = \frac{p<em>\alpha}{q</em>\alpha B}

  • This simplifies to: p<em>pp</em>α=q<em>pq</em>α\frac{p<em>p}{p</em>\alpha} = \frac{q<em>p}{q</em>\alpha}

  • Now, put in their charges (proton charge q<em>p=qq<em>p = q, alpha particle charge q</em>α=2qq</em>\alpha = 2q):

p<em>pp</em>α=q2q=12\frac{p<em>p}{p</em>\alpha} = \frac{q}{2q} = \boxed{\tfrac{1}{2}}

  • Important tip: This means the proton's momentum (p<em>pp<em>p) must be half of the alpha particle's momentum (p</em>αp</em>\alpha) for them to have the same radius. Don't get confused and divide by mass ratios directly here; the formula already uses momentum.


Chapter 5 – Quick Look at the Main Formulas
  • Magnetic force (strength): F=qvBsinθF = qvB\sin\theta

  • For circular motion (force is perpendicular): qvB=mv2rqvB = \dfrac{mv^2}{r}

  • Radius of the circle: r=mvqB=pqBr = \dfrac{mv}{qB} = \dfrac{p}{qB}

  • Time for one circle: T=2πmqBT = \dfrac{2\pi m}{qB}

  • Revolutions per second: f=qB2πmf = \dfrac{qB}{2\pi m}

  • How fast it spins: ω=qBm\omega = \dfrac{qB}{m}


Chapter 6 – Why This Is Important
  • Because T, f, and ω\omega depend only on the charge-to-mass ratio (qm\frac{q}{m}) and the magnetic field (BB), any particles with the same qm\frac{q}{m} will spin in circles at the same frequency. This idea is used in machines like the cyclotron accelerator, which speeds up particles.

  • If you know just one of these values (like the radius, time period, frequency, or angular frequency), you can use the formulas to calculate all the others.

  • Things to remember for tests:

    1. When is there no magnetic force on a charged particle? (When it moves parallel to the field).

    2. When is the magnetic force strongest? (When it moves perpendicular to the field).

    3. How to get the formulas for r, T, f, and ω\omega starting from the main force equation (qvB=mv2rqvB = \dfrac{mv^2}{r}).

    4. Questions comparing different particles (like asking about the radii, momenta, or frequencies of a proton vs. an alpha particle).

    5. How to use the right-hand palm rule to find the direction of the force, and remember to flip it for negative charges.