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Chapter 4: Moving Charges and Magnetism

A current-carrying wire and a magnet exert force on each other — this is the discovery of Oersted (1820) that united electricity and magnetism into a single subject, electromagnetism. This chapter develops:

  1. The magnetic force F⃗=qv⃗×B⃗\vec{F} = q\vec{v}\times\vec{B} acting on moving charges.
  2. The sources of magnetic fields — currents — via the Biot–Savart law and Ampère's law.
  3. Devices built on these principles: the cyclotron, solenoid, moving-coil galvanometer, and conversions to ammeter/voltmeter.

The mathematics is more vector-heavy than electrostatics: dot products and especially cross products are everywhere.

Concept Map

  • 4.1 Magnetic field — Oersted's experiment
  • 4.2 Magnetic force on a moving charge — Lorentz force
  • 4.3 Motion in a magnetic field — circular and helical
  • 4.4 Cyclotron
  • 4.5 Magnetic force on a current-carrying conductor
  • 4.6 Biot–Savart law and applications
  • 4.7 Ampère's circuital law: wire, solenoid, toroid
  • 4.8 Force between parallel currents; definition of ampere
  • 4.9 Torque on a current loop; moving-coil galvanometer
  • 4.10 Galvanometer →\to ammeter and voltmeter

4.1 Magnetic Field — Oersted's Experiment

Observation

A compass needle placed near a current-carrying wire deflects, showing that the wire creates a magnetic field. Reversing the current reverses the deflection. Thus a magnetic field can be produced by moving charges (currents) as well as by permanent magnets.

Magnetic Field B⃗\vec{B}

The magnetic field B⃗\vec{B} is a vector field. It is sometimes called the magnetic flux density.

SI unit. Tesla (T\text{T}): 1 T=1 N/(A m)=1 Wb/m21\text{ T} = 1\text{ N}/(\text{A m}) = 1\text{ Wb/m}^2. The CGS unit is the gauss (1 G=10−4 T1\text{ G} = 10^{-4}\text{ T}).

Typical values: Earth's surface ∼5×10−5 T\sim 5\times 10^{-5}\text{ T}; small bar magnet ∼10−2 T\sim 10^{-2}\text{ T}; MRI machine ∼1–3 T\sim 1\text{–}3\text{ T}.

Right-Hand Rule for Wire

For a straight wire, B⃗\vec{B} encircles the wire; curl your right hand with thumb along the current — your fingers curl in the direction of B⃗\vec{B}.


4.2 Magnetic Force on a Moving Charge — Lorentz Force

Definition

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

 F⃗B=qv⃗×B⃗ .\boxed{\,\vec{F}_B = q\vec{v}\times\vec{B}\,}.

Magnitude: F=qvBsin⁡θF = qvB\sin\theta where θ\theta is the angle between v⃗\vec{v} and B⃗\vec{B}.

Direction. Perpendicular to both v⃗\vec{v} and B⃗\vec{B} — right-hand rule.

Properties

  1. Force is zero when v⃗∥B⃗\vec{v}\parallel\vec{B} (θ=0\theta=0 or π\pi).
  2. Force is maximum (qvBqvB) when v⃗⊥B⃗\vec{v}\perp\vec{B}.
  3. The magnetic force is always perpendicular to v⃗\vec{v}, so it does no work: F⃗⋅v⃗=0\vec{F}\cdot\vec{v}=0. Kinetic energy of the charge is conserved.

Lorentz Force (combined with electric field)

If both E⃗\vec{E} and B⃗\vec{B} are present:

F⃗=q(E⃗+v⃗×B⃗).\vec{F} = q(\vec{E} + \vec{v}\times\vec{B}).

Worked Example

An electron (q=−1.6×10−19 Cq = -1.6\times 10^{-19}\text{ C}) moves at v⃗=2×106 i^ m/s\vec{v} = 2\times 10^6\,\hat{i}\text{ m/s} in B⃗=0.5 j^ T\vec{B} = 0.5\,\hat{j}\text{ T}. Find the force.

v⃗×B⃗=2×106⋅0.5 k^=106 k^\vec{v}\times\vec{B} = 2\times 10^6\cdot 0.5\,\hat{k} = 10^6\,\hat{k}. F⃗=qv⃗×B⃗=−(1.6×10−19)(106)k^=−1.6×10−13 k^ N\vec{F} = q\vec{v}\times\vec{B} = -(1.6\times 10^{-19})(10^6)\hat{k} = -1.6\times 10^{-13}\,\hat{k}\text{ N}.

Pitfalls

  • The magnetic force changes the direction of v⃗\vec{v}, not its magnitude.
  • Sign of charge: for an electron, F⃗\vec{F} is in the opposite direction to v⃗×B⃗\vec{v}\times\vec{B}.
  • Don't confuse F⃗=qv⃗×B⃗\vec{F} = q\vec{v}\times\vec{B} (force on a charge) with F⃗=IL⃗×B⃗\vec{F} = I\vec{L}\times\vec{B} (force on a current).

4.3 Motion in a Magnetic Field

(a) Charge Moving Perpendicular to B⃗\vec{B}

If v⃗⊥B⃗\vec{v}\perp\vec{B}, the magnetic force always remains perpendicular to v⃗\vec{v} — it acts as a centripetal force. The charge moves in a circle.

Step 1. ∣qvB∣=mv2/r\vert qvB\vert = mv^2/r.

Step 2. Radius:

 r=mvqB .\boxed{\,r = \frac{mv}{qB}\,}.

Step 3. Angular speed: ω=v/r=qB/m\omega = v/r = qB/m. Period:

 T=2πmqB ,ν=qB2πm.\boxed{\,T = \frac{2\pi m}{qB}\,}, \qquad \nu = \frac{qB}{2\pi m}.

TT is independent of vv and rr — the basis of the cyclotron.

(b) Helical Motion

If v⃗\vec{v} has a component along B⃗\vec{B}, decompose: v∥v_\parallel (unaffected) and v⊥v_\perp (gives circular motion). Result: a helix with:

  • Radius r=mv⊥/(qB)r = mv_\perp/(qB).
  • Pitch (distance per turn along axis) p=v∥T=2πmv∥/(qB)p = v_\parallel T = 2\pi m v_\parallel/(qB).

Worked Example

A proton (m=1.67×10−27m = 1.67\times 10^{-27} kg) enters B⃗=0.1 T\vec{B} = 0.1\text{ T} at v=106 m/sv = 10^6\text{ m/s} perpendicular to B⃗\vec{B}.

r=mv/(qB)=(1.67×10−27)(106)/((1.6×10−19)(0.1))=0.104 mr = mv/(qB) = (1.67\times 10^{-27})(10^6)/((1.6\times 10^{-19})(0.1)) = 0.104\text{ m}. T=2πr/v=6.55×10−7 sT = 2\pi r/v = 6.55\times 10^{-7}\text{ s} (ν≈1.53 MHz\nu \approx 1.53\text{ MHz}).

Pitfalls

  • Cyclotron period is independent of vv only in the non-relativistic regime. At very high vv, mm grows and the period drifts.
  • For an electron the circle is in the opposite sense compared to a proton in the same B⃗\vec{B}.

4.4 Cyclotron

Principle

The cyclotron exploits the fact that the period of circular motion is independent of vv. Two semicircular "dees" sit in a uniform magnetic field. An alternating voltage between them, with frequency matching νc=qB/(2πm)\nu_c = qB/(2\pi m), accelerates the particle each time it crosses the gap — the radius grows but the timing stays in sync.

Resonance Condition

 νac=νc=qB2πm .\boxed{\,\nu_{\text{ac}} = \nu_c = \frac{qB}{2\pi m}\,}.

Maximum Kinetic Energy

When the particle reaches the maximum radius RR:

vmax⁡=qBRm,Kmax⁡=12mvmax⁡2=q2B2R22m.v_{\max} = \frac{qBR}{m}, \qquad K_{\max} = \frac{1}{2}mv_{\max}^2 = \frac{q^2B^2R^2}{2m}.

Limitations

  1. Relativistic mass increase — at high vv, mm rises, νc\nu_c drops, particle goes out of sync.
  2. Cannot accelerate uncharged particles (no Lorentz force).
  3. Cannot accelerate electrons efficiently — they go relativistic too quickly.
  4. Limited to positive ions of moderate energy (∼\sim tens of MeV).

Improvements: synchrocyclotron (variable frequency), synchrotron (variable BB).

Worked Example

Cyclotron with B=1 TB = 1\text{ T} and R=0.5 mR = 0.5\text{ m}, accelerating protons.

Kmax⁡=(1.6×10−19)2(1)2(0.5)2/(2⋅1.67×10−27)=1.92×10−12 J=12 MeVK_{\max} = (1.6\times 10^{-19})^2(1)^2(0.5)^2/(2\cdot 1.67\times 10^{-27}) = 1.92\times 10^{-12}\text{ J} = 12\text{ MeV}.

Pitfalls

  • The dees themselves do not accelerate the particle — they shield it from the AC field; acceleration only occurs in the gap.
  • The frequency depends on q/mq/m ratio; protons and deuterons need different cyclotron frequencies.

4.5 Magnetic Force on a Current-Carrying Wire

Derivation

A wire of length LL, cross-section AA, current II in field B⃗\vec{B} contains nALn A L free electrons drifting at v⃗d\vec{v}_d. Total force:

F⃗=(nAL)⋅(−e)v⃗d×B⃗.\vec{F} = (nAL)\cdot (-e)\vec{v}_d\times\vec{B}.

But I=nAevdI = nAev_d and the current direction is opposite to v⃗d\vec{v}_d (electron flow), so IL⃗=−nAevdL⃗=−nAev⃗dLI\vec{L} = -nAe v_d \vec{L} = -nAe\vec{v}_d L... working out carefully:

 F⃗=IL⃗×B⃗ ,\boxed{\,\vec{F} = I\vec{L}\times\vec{B}\,},

where L⃗\vec{L} is the length vector in the direction of conventional current.

For a curved wire of arbitrary shape:

F⃗=I∫dl⃗×B⃗.\vec{F} = I\int d\vec{l}\times\vec{B}.

In a uniform B⃗\vec{B}, the integral ∫dl⃗\int d\vec{l} depends only on the endpoints — a closed loop in uniform B⃗\vec{B} experiences zero net force (but possibly a torque).

Worked Example

A horizontal wire of length 0.5 m0.5\text{ m} carries I=4 AI = 4\text{ A} northward. B⃗=0.2 T\vec{B} = 0.2\text{ T} vertically downward. Force on the wire:

F=ILBsin⁡90°=4⋅0.5⋅0.2=0.4 NF = ILB\sin 90° = 4\cdot 0.5\cdot 0.2 = 0.4\text{ N}, directed eastward (right-hand rule).

Pitfalls

  • Closed loop in uniform B⃗\vec{B}: F⃗net=0\vec{F}_{\text{net}} = 0.
  • Force depends on the wire's orientation, not where it physically is in space (as long as B⃗\vec{B} is uniform).

4.6 Biot–Savart Law

Statement

A small element dl⃗d\vec{l} of a wire carrying current II creates, at a point PP at displacement r⃗\vec{r}, a magnetic field

 dB⃗=μ04π I dl⃗×r^r2 ,\boxed{\,d\vec{B} = \frac{\mu_0}{4\pi}\,\frac{I\,d\vec{l}\times\hat{r}}{r^2}\,},

where μ0=4π×10−7 T m/A\mu_0 = 4\pi\times 10^{-7}\text{ T m/A} is the permeability of free space, and r^\hat{r} is from dl⃗d\vec{l} to PP.

Magnitude: dB=μ04πI dlsin⁡θr2dB = \dfrac{\mu_0}{4\pi}\dfrac{I\,dl\sin\theta}{r^2}.

Comparison with Coulomb's Law

PropertyCoulombBiot–Savart
SourcedqdqI dl⃗I\,d\vec{l}
Field typeE⃗\vec{E}B⃗\vec{B}
Constant1/(4πε0)1/(4\pi\varepsilon_0)μ0/(4π)\mu_0/(4\pi)
DirectionAlong r^\hat{r}Perpendicular to both dl⃗d\vec{l} and r^\hat{r}
Falloff1/r21/r^21/r21/r^2

Application (a) — Straight Wire (Finite)

Long straight wire of length spanning angles θ1\theta_1 to θ2\theta_2 as seen from PP (perpendicular distance aa).

Step 1. For an element dldl at angle θ\theta, r=a/sin⁡θr = a/\sin\theta, dl=a dθ/sin⁡2θdl = a\,d\theta/\sin^2\theta (using l=−acot⁡θl = -a\cot\theta).

Step 2. All dB⃗d\vec{B} point in the same direction (out/into page).

Step 3.

B=∫μ0I4πsin⁡θ dθa=μ0I4πa[cos⁡θ1−cos⁡θ2]B = \int \frac{\mu_0 I}{4\pi}\frac{\sin\theta\,d\theta}{a} = \frac{\mu_0 I}{4\pi a}\bigl[\cos\theta_1-\cos\theta_2\bigr]

(with appropriate sign convention; an alternative common form is B=μ0I4πa(sin⁡ϕ1+sin⁡ϕ2)B = \dfrac{\mu_0 I}{4\pi a}(\sin\phi_1 + \sin\phi_2) where ϕ\phi measured from perpendicular).

Special case — Infinite wire (θ1=0,θ2=π\theta_1=0, \theta_2=\pi):

 B=μ0I2πa .\boxed{\,B = \frac{\mu_0 I}{2\pi a}\,}.

Semi-infinite wire (from −∞-\infty to the foot of perpendicular):

B=μ0I4πa.B = \frac{\mu_0 I}{4\pi a}.

Application (b) — Circular Loop (Centre)

Loop of radius RR carrying II.

Step 1. For every element dl⃗d\vec{l}, dl⃗⊥r^d\vec{l}\perp\hat{r}, so sin⁡θ=1\sin\theta = 1. Also r=Rr = R.

Step 2. All elements produce dBdB in the same direction along the axis at the centre.

Step 3.

B=∫μ0I dl4πR2=μ0I4πR2⋅2πR=μ0I2R.B = \int\frac{\mu_0 I\,dl}{4\pi R^2} = \frac{\mu_0 I}{4\pi R^2}\cdot 2\pi R = \frac{\mu_0 I}{2R}.  Bcentre=μ0I2R .\boxed{\,B_{\text{centre}} = \frac{\mu_0 I}{2R}\,}.

For NN turns: B=μ0NI/(2R)B = \mu_0 N I/(2R).

Application (c) — Circular Loop (Axis)

Point on axis at distance zz from centre.

Step 1. Each element gives dB=μ0I dl/(4π(R2+z2))dB = \mu_0 I\,dl/(4\pi (R^2+z^2)) (since dl⃗⊥r^d\vec{l}\perp\hat{r}).

Step 2. Components perpendicular to axis cancel; axial components add. Axial fraction: cos⁡α=R/R2+z2\cos\alpha = R/\sqrt{R^2+z^2}.

Step 3.

Bz=∫μ0I dl4π(R2+z2)⋅RR2+z2=μ0IR4π(R2+z2)3/2⋅2πR.B_z = \int\frac{\mu_0 I\,dl}{4\pi(R^2+z^2)}\cdot\frac{R}{\sqrt{R^2+z^2}} = \frac{\mu_0 I R}{4\pi(R^2+z^2)^{3/2}}\cdot 2\pi R.  Bz=μ0IR22(R2+z2)3/2 .\boxed{\,B_z = \frac{\mu_0 I R^2}{2(R^2+z^2)^{3/2}}\,}.

For z≫Rz\gg R: Bz≈μ0IR2/(2z3)=μ0(2m)/(4πz3)B_z \approx \mu_0 I R^2/(2z^3) = \mu_0(2 m)/(4\pi z^3) where m=IπR2m = I\pi R^2 is the magnetic moment — same 1/r31/r^3 dependence as an electric dipole on axis.

Pitfalls

  • Biot–Savart is the magnetic analog of Coulomb's law — for currents, not charges.
  • Always identify the direction of dl⃗×r^d\vec{l}\times\hat{r} before applying magnitude formulas.
  • For curved wires, use symmetry — most elements give components that cancel.

4.7 Ampère's Circuital Law

Statement

The line integral of B⃗\vec{B} around any closed loop equals μ0\mu_0 times the net current enclosed by the loop:

 ∮B⃗⋅dl⃗=μ0Ienc .\boxed{\,\oint \vec{B}\cdot d\vec{l} = \mu_0 I_{\text{enc}}\,}.

Sign convention: IencI_{\text{enc}} is positive when current flows in the direction given by the right-hand rule from the orientation of the loop.

Like Gauss's law for E⃗\vec{E}, Ampère's law is always true, but useful only when symmetry lets us pull BB out of the integral.

Application (a) — Infinite Straight Wire

Circular Amperian loop of radius rr coaxial with the wire. By symmetry, B⃗\vec{B} is tangent and constant in magnitude.

∮B dl=B⋅2πr=μ0I\oint B\,dl = B\cdot 2\pi r = \mu_0 I, so

B=μ0I2πr.B = \frac{\mu_0 I}{2\pi r}.

(Same as Biot–Savart — but with much less work.)

Application (b) — Solenoid

A long solenoid: closely wound, nn turns per unit length, current II.

Inside (away from ends), B⃗\vec{B} is uniform along the axis; outside, B→0B\to 0 (for an ideal long solenoid).

Amperian loop: a rectangle of length LL, one side parallel to axis inside the solenoid, the opposite side far outside, two short sides perpendicular to axis.

  • Inside leg: ∫B⃗⋅dl⃗=BL\int \vec{B}\cdot d\vec{l} = BL.
  • Outside leg: ≈0\approx 0.
  • Short sides: B⃗⊥dl⃗\vec{B}\perp d\vec{l}, contribution zero.

∮=BL\oint = BL. Enclosed current: nLInLI.

BL=μ0nLI⇒ Binside=μ0nI .BL = \mu_0 n L I \Rightarrow \boxed{\,B_{\text{inside}} = \mu_0 n I\,}.

For a solenoid of finite length, near the ends BB drops to half: Bend=μ0nI/2B_{\text{end}} = \mu_0 n I/2.

Application (c) — Toroid

A toroid is a solenoid bent into a doughnut. NN total turns, mean radius rr. Amperian loop: a circle of radius rr inside the toroid.

∮B dl=B⋅2πr=μ0NI\oint B\,dl = B\cdot 2\pi r = \mu_0 N I:

 B=μ0NI2πr .\boxed{\,B = \frac{\mu_0 N I}{2\pi r}\,}.

Outside the toroid: B=0B = 0 (Amperian loops outside enclose zero net current).

Worked Example

A solenoid has 10001000 turns over 50 cm50\text{ cm} and carries 2 A2\text{ A}.

n=1000/0.5=2000 /mn = 1000/0.5 = 2000\text{ /m}. B=(4π×10−7)(2000)(2)=5×10−3 TB = (4\pi\times 10^{-7})(2000)(2) = 5\times 10^{-3}\text{ T}.

Pitfalls

  • Ampère's law works only for steady currents (in this chapter — Maxwell's correction comes later).
  • Symmetry is essential; randomly drawn loops produce useless equations.
  • The integral is over the loop, not the current.

4.8 Force Between Parallel Currents; Definition of the Ampere

Setup

Two long parallel wires, separation dd, currents I1,I2I_1, I_2.

Step 1. Field due to wire 1 at the location of wire 2: B1=μ0I1/(2πd)B_1 = \mu_0 I_1/(2\pi d).

Step 2. Force per unit length on wire 2: F/L=I2B1=μ0I1I22πdF/L = I_2 B_1 = \dfrac{\mu_0 I_1 I_2}{2\pi d}.

Step 3.

 FL=μ0I1I22πd .\boxed{\,\frac{F}{L} = \frac{\mu_0 I_1 I_2}{2\pi d}\,}.

Direction:

  • Currents in same direction: wires attract.
  • Currents in opposite directions: wires repel.

Definition of the Ampere

The historical SI definition (pre-2019): one ampere is the steady current which, when flowing in two parallel infinite wires 1 m1\text{ m} apart in vacuum, produces a force per unit length of 2×10−7 N/m2\times 10^{-7}\text{ N/m} between them.

(Since 2019, the ampere is defined in terms of the elementary charge ee; but the parallel-wire formula remains the working test.)

Worked Example

Two parallel wires, 0.5 m0.5\text{ m} apart, both carrying 10 A10\text{ A} in the same direction. Force per meter:

F/L=(4π×10−7)(10)(10)2π(0.5)=4×10−5 N/m, attractive.F/L = \frac{(4\pi\times 10^{-7})(10)(10)}{2\pi(0.5)} = 4\times 10^{-5}\text{ N/m, attractive}.

Pitfalls

  • "Same direction →\to attract" — counter-intuitive if you only know charges. The field/force geometry differs from Coulomb.
  • The formula is for infinite parallel wires; for finite segments it's an approximation.

4.9 Torque on a Current Loop; Moving-Coil Galvanometer

Torque on a Rectangular Loop

Loop of sides aa (horizontal) and bb (vertical), current II, in uniform B⃗\vec{B} horizontal. The loop's normal n^\hat{n} makes angle θ\theta with B⃗\vec{B}.

Two horizontal sides experience opposite forces along the loop axis — no torque (or cancellation).

Two vertical sides (length bb) carry currents perpendicular to B⃗\vec{B}. Each experiences force F=IbBF = IbB, equal and opposite, forming a couple.

Perpendicular distance between the forces: asin⁡θa\sin\theta.

τ=IbB⋅asin⁡θ=IABsin⁡θ,\tau = IbB\cdot a\sin\theta = IAB\sin\theta,

where A=abA = ab is the loop area.

For NN turns: τ=NIABsin⁡θ\tau = NIAB\sin\theta.

Magnetic Dipole Moment

Define m⃗=NIA⃗\vec{m} = NI\vec{A} (vector area, by right-hand rule); SI unit: A m2\text{A m}^2. Then

 τ⃗=m⃗×B⃗ ,U=−m⃗⋅B⃗.\boxed{\,\vec{\tau} = \vec{m}\times\vec{B}\,}, \qquad U = -\vec{m}\cdot\vec{B}.

(Direct analog of electric dipole: p⃗↔m⃗\vec{p}\leftrightarrow\vec{m}, E⃗↔B⃗\vec{E}\leftrightarrow\vec{B}.)

Moving-Coil Galvanometer

A coil of NN turns, area AA, suspended in a radial magnetic field (produced by curved pole pieces). When current II flows:

  • Deflecting torque: τdef=NIAB\tau_{\text{def}} = NIAB (because θ=90°\theta = 90° always — that's the point of the radial field).
  • Restoring torque: τrest=kϕ\tau_{\text{rest}} = k\phi (a torsion spring with constant kk, ϕ\phi is the deflection).

At equilibrium:

NIAB=kϕ⇒ ϕ=NABk I .NIAB = k\phi \Rightarrow \boxed{\,\phi = \frac{NAB}{k}\,I\,}.

Linear scale: deflection ∝\propto current.

Sensitivity

  • Current sensitivity: ϕ/I=NAB/k\phi/I = NAB/k.
  • Voltage sensitivity: ϕ/V=NAB/(kRg)\phi/V = NAB/(kR_g) where RgR_g is the galvanometer's own resistance.

To increase current sensitivity: increase NN, AA, BB; decrease kk.

But increasing NN also increases RgR_g, so voltage sensitivity may not improve.

Pitfalls

  • Galvanometer's pole pieces are curved precisely to keep θ=90°\theta = 90° — this is what makes the scale linear.
  • "Sensitivity" and "accuracy" are not the same; a sensitive instrument can be precise but biased.

4.10 Conversion of a Galvanometer

To an Ammeter

An ammeter must measure large currents and have low resistance (so it doesn't disturb the circuit). Add a small shunt SS in parallel with the galvanometer.

Step 1. Let full-scale current of galvanometer be IgI_g (with RgR_g). To read up to II, shunt must carry I−IgI - I_g.

Step 2. Same voltage across GG and SS:

IgRg=(I−Ig)S⇒ S=IgRgI−Ig .I_g R_g = (I - I_g)S \Rightarrow \boxed{\,S = \frac{I_g R_g}{I - I_g}\,}.

Step 3. Effective resistance of ammeter:

RA=RgSRg+S<S.R_A = \frac{R_g S}{R_g + S} < S.

For I≫IgI\gg I_g, S≪RgS\ll R_g, so RAR_A is very small — ideal.

To a Voltmeter

A voltmeter must measure large voltages without drawing current — high resistance. Add a large series resistance RR.

Step 1. For full-scale voltage VV:

V=Ig(Rg+R)⇒ R=VIg−Rg .V = I_g(R_g + R) \Rightarrow \boxed{\,R = \frac{V}{I_g} - R_g\,}.

Step 2. Effective resistance: RV=R+Rg≫RgR_V = R + R_g \gg R_g — ideal voltmeter draws minimal current.

Worked Example

A galvanometer with Rg=50 ΩR_g = 50\,\Omega, Ig=1 mAI_g = 1\text{ mA}:

  • To read up to 1 A1\text{ A} as an ammeter: S=(10−3)(50)/(1−10−3)≈0.05 ΩS = (10^{-3})(50)/(1 - 10^{-3}) \approx 0.05\,\Omega.
  • To read up to 10 V10\text{ V} as a voltmeter: R=10/10−3−50=9950 ΩR = 10/10^{-3} - 50 = 9950\,\Omega.

Pitfalls

  • An ammeter goes in series in the circuit; a voltmeter goes in parallel.
  • Putting a voltmeter in series with a load gives essentially zero current — students often make this mistake.
  • Ammeters are dangerous to apply directly across a battery — low resistance means huge currents.

Solved Problems

Problem 1 (Easy)

A wire carries 5 A5\text{ A} in a horizontal direction. The horizontal component of Earth's magnetic field is 4×10−5 T4\times 10^{-5}\text{ T}. The force on a 1 m1\text{ m} length of the wire (perpendicular to B⃗\vec{B}):

F=ILB=5⋅1⋅4×10−5=2×10−4 N.F = ILB = 5\cdot 1\cdot 4\times 10^{-5} = 2\times 10^{-4}\text{ N}.

Problem 2 (Easy)

A proton enters a B⃗=0.2 T\vec{B} = 0.2\text{ T} field at v=2×107 m/sv = 2\times 10^7\text{ m/s} perpendicular to B⃗\vec{B}. Find the radius.

r=mvqB=(1.67×10−27)(2×107)(1.6×10−19)(0.2)=1.04 m.r = \frac{mv}{qB} = \frac{(1.67\times 10^{-27})(2\times 10^7)}{(1.6\times 10^{-19})(0.2)} = 1.04\text{ m}.

Problem 3 (Medium)

A circular coil of radius 0.1 m0.1\text{ m}, 100100 turns, carries 2 A2\text{ A}. Find B⃗\vec{B} at its centre and at 0.1 m0.1\text{ m} on the axis.

Centre: B=μ0NI/(2R)=(4π×10−7)(100)(2)/(2⋅0.1)=1.26×10−3 TB = \mu_0 N I/(2R) = (4\pi\times 10^{-7})(100)(2)/(2\cdot 0.1) = 1.26\times 10^{-3}\text{ T}.

On axis (z=0.1z = 0.1): B=μ0NIR2/(2(R2+z2)3/2)=B = \mu_0 N I R^2/(2(R^2+z^2)^{3/2}) = with R2+z2=0.02R^2+z^2 = 0.02, (R2+z2)3/2=2.83×10−3(R^2+z^2)^{3/2} = 2.83\times 10^{-3}. B=(4π×10−7)(100)(2)(0.01)/(2⋅2.83×10−3)=4.44×10−4 TB = (4\pi\times 10^{-7})(100)(2)(0.01)/(2\cdot 2.83\times 10^{-3}) = 4.44\times 10^{-4}\text{ T}.

Problem 4 (Medium)

A solenoid of length 0.5 m0.5\text{ m} and 500500 turns carries current II. Determine II such that BB inside is 0.01 T0.01\text{ T}.

B=μ0nI⇒I=B/(μ0n)=0.01/(4π×10−7⋅1000)=7.96 A.B = \mu_0 n I \Rightarrow I = B/(\mu_0 n) = 0.01/(4\pi\times 10^{-7}\cdot 1000) = 7.96\text{ A}.

Problem 5 (Medium) — Parallel Wires

Two long parallel wires, 5 cm5\text{ cm} apart, carry 4 A4\text{ A} and 6 A6\text{ A} in opposite directions. Find the force per meter.

F/L=μ0I1I22πd=(4π×10−7)(4)(6)2π(0.05)=9.6×10−5 N/m, repulsive.F/L = \frac{\mu_0 I_1 I_2}{2\pi d} = \frac{(4\pi\times 10^{-7})(4)(6)}{2\pi(0.05)} = 9.6\times 10^{-5}\text{ N/m, repulsive}.

Problem 6 (Hard) — Cyclotron Design

A cyclotron of dee radius 0.4 m0.4\text{ m} accelerates protons to 10 MeV10\text{ MeV}. Find the magnetic field needed and the required AC frequency.

K=q2B2R2/(2m)K = q^2B^2R^2/(2m). Solving:

B=1R2mK/q2=10.42(1.67×10−27)(10⋅106⋅1.6×10−19)/(1.6×10−19)2.B = \frac{1}{R}\sqrt{2mK/q^2} = \frac{1}{0.4}\sqrt{2(1.67\times 10^{-27})(10\cdot 10^6\cdot 1.6\times 10^{-19})/(1.6\times 10^{-19})^2}.

2mK=2⋅1.67×10−27⋅1.6×10−12=5.34×10−392mK = 2\cdot 1.67\times 10^{-27}\cdot 1.6\times 10^{-12} = 5.34\times 10^{-39}. 5.34×10−39/(2.56×10−38)=0.2086=0.457 ... in units T m\sqrt{5.34\times 10^{-39}/(2.56\times 10^{-38})} = \sqrt{0.2086} = 0.457\text{ ... in units T m}. B=0.457/0.4=1.14 TB = 0.457/0.4 = 1.14\text{ T}.

Frequency: ν=qB/(2πm)=(1.6×10−19⋅1.14)/(2π⋅1.67×10−27)=1.74×107 Hz=17.4 MHz\nu = qB/(2\pi m) = (1.6\times 10^{-19}\cdot 1.14)/(2\pi\cdot 1.67\times 10^{-27}) = 1.74\times 10^7\text{ Hz} = 17.4\text{ MHz}.

Problem 7 (Hard) — Galvanometer Conversion

A galvanometer (Rg=100 ΩR_g = 100\,\Omega, Ig=10 μAI_g = 10\,\mu\text{A}) is to be converted (a) to an ammeter of range 0–1 A0\text{–}1\text{ A}, and (b) to a voltmeter of range 0–100 V0\text{–}100\text{ V}.

(a) S=IgRg/(I−Ig)=10−5⋅100/(1−10−5)≈10−3 Ω=1 mΩS = I_g R_g/(I - I_g) = 10^{-5}\cdot 100/(1 - 10^{-5}) \approx 10^{-3}\,\Omega = 1\text{ m}\Omega.

(b) R=V/Ig−Rg=100/10−5−100=107−100≈10 MΩR = V/I_g - R_g = 100/10^{-5} - 100 = 10^7 - 100 \approx 10\text{ M}\Omega.


JEE/NEET Edge Cases

  1. Velocity selector: Crossed E⃗\vec{E} and B⃗\vec{B} select particles with v=E/Bv = E/B. Used in mass spectrometers.

  2. Cyclotron loses sync for high-energy particles due to relativistic mass increase; synchrocyclotrons modulate frequency.

  3. Force on a closed loop in uniform B⃗\vec{B} is zero, but torque generally non-zero.

  4. Net force on a current loop in a non-uniform field: Use F⃗=∇(m⃗⋅B⃗)\vec{F} = \nabla(\vec{m}\cdot\vec{B}). This is how a magnet attracts a current loop.

  5. Helical pitch ratio: for a charge entering at angle θ\theta to B⃗\vec{B}, pitch/circumference =v∥/v⊥=cot⁡θ= v_\parallel/v_\perp = \cot\theta.

  6. Solenoid end vs middle: Bend=Bmid/2B_{\text{end}} = B_{\text{mid}}/2 for a long solenoid.

  7. Current loop near a long wire: the loop experiences a net force (one side closer to the wire than the other).

  8. Toroid outside is zero: but only for an ideal toroid; real-world toroids leak a little.

  9. Galvanometer sensitivity vs robustness: increasing NN and AA makes coil heavier; spring constant kk has practical lower bound.

  10. Ammeter has lowest resistance, voltmeter has highest — swap them and you'll either short the battery or read essentially nothing.

  11. Magnetic field of a finite straight wire at perpendicular foot: B=(μ0I/4πa)(sin⁡ϕ1+sin⁡ϕ2)B = (\mu_0 I/4\pi a)(\sin\phi_1+\sin\phi_2) where ϕi\phi_i are angles to the ends from the perpendicular. Don't forget this — the infinite formula doesn't always apply.


Quick Recap

  • F⃗=q(E⃗+v⃗×B⃗)\vec{F} = q(\vec{E} + \vec{v}\times\vec{B}); magnetic force does no work.
  • Circle in B⃗\vec{B}: r=mv/qBr = mv/qB; T=2πm/qBT = 2\pi m/qB.
  • Cyclotron: ν=qB/(2πm)\nu = qB/(2\pi m); Kmax⁡=q2B2R2/(2m)K_{\max} = q^2B^2R^2/(2m).
  • Wire force: F⃗=IL⃗×B⃗\vec{F} = I\vec{L}\times\vec{B}.
  • Biot–Savart: dB⃗=(μ0/4π)(Idl⃗×r^)/r2d\vec{B} = (\mu_0/4\pi)(Id\vec{l}\times\hat{r})/r^2.
  • Wire: B=μ0I/(2πa)B = \mu_0 I/(2\pi a). Loop centre: μ0I/(2R)\mu_0 I/(2R). Solenoid: μ0nI\mu_0 n I. Toroid: μ0NI/(2πr)\mu_0 N I/(2\pi r).
  • Parallel wires: F/L=μ0I1I2/(2πd)F/L = \mu_0 I_1 I_2/(2\pi d); same direction →\to attract.
  • Loop torque: τ⃗=m⃗×B⃗\vec{\tau} = \vec{m}\times\vec{B}; m⃗=NIA⃗\vec{m} = NI\vec{A}.
  • Galvanometer: ϕ=NABI/k\phi = NABI/k.
  • Ammeter shunt: S=IgRg/(I−Ig)S = I_gR_g/(I-I_g); Voltmeter series: R=V/Ig−RgR = V/I_g - R_g.

Formula Sheet

QuantityFormulaNotes
Lorentz forceF⃗=q(E⃗+v⃗×B⃗)\vec{F} = q(\vec{E}+\vec{v}\times\vec{B})
Magnetic forceF=qvBsin⁡θF = qvB\sin\thetaNo work
Circular motionr=mv/qBr = mv/qB
PeriodT=2πm/qBT = 2\pi m/qBIndependent of vv
Cyclotron freqν=qB/(2πm)\nu = qB/(2\pi m)
Cyclotron KEKmax⁡=q2B2R2/(2m)K_{\max} = q^2B^2R^2/(2m)
Helix pitchp=2πmv∥/(qB)p = 2\pi m v_\parallel/(qB)
Force on wireF⃗=IL⃗×B⃗\vec{F} = I\vec{L}\times\vec{B}
Biot–SavartdB⃗=μ04πIdl⃗×r^r2d\vec{B} = \dfrac{\mu_0}{4\pi}\dfrac{Id\vec{l}\times\hat{r}}{r^2}μ0=4π×10−7\mu_0 = 4\pi\times 10^{-7}
Inf. straight wireB=μ0I/(2πa)B = \mu_0 I/(2\pi a)
Finite wireB=(μ0I/4πa)(sin⁡ϕ1+sin⁡ϕ2)B = (\mu_0 I/4\pi a)(\sin\phi_1+\sin\phi_2)ϕ\phi from perpendicular
Loop centreB=μ0NI/(2R)B = \mu_0 N I/(2R)
Loop axisB=μ0IR2/[2(R2+z2)3/2]B = \mu_0 IR^2/[2(R^2+z^2)^{3/2}]
Ampère's law∮B⃗⋅dl⃗=μ0Ienc\oint\vec{B}\cdot d\vec{l}=\mu_0 I_{\text{enc}}
Solenoid insideB=μ0nIB = \mu_0 n In=N/Ln=N/L
Solenoid endB=μ0nI/2B = \mu_0 n I/2
ToroidB=μ0NI/(2πr)B = \mu_0 N I/(2\pi r)Inside
Parallel wiresF/L=μ0I1I2/(2πd)F/L = \mu_0 I_1I_2/(2\pi d)Same dir: attract
Magnetic momentm⃗=NIA⃗\vec{m} = NI\vec{A}A m²
Loop torqueτ⃗=m⃗×B⃗\vec{\tau} = \vec{m}\times\vec{B}
Loop PEU=−m⃗⋅B⃗U = -\vec{m}\cdot\vec{B}
Galvanometerϕ=NABI/k\phi = NABI/k
Current sens.NAB/kNAB/kϕ/I\phi/I
Voltage sens.NAB/(kRg)NAB/(kR_g)ϕ/V\phi/V
Ammeter shuntS=IgRg/(I−Ig)S = I_gR_g/(I-I_g)Parallel
Voltmeter seriesR=V/Ig−RgR = V/I_g - R_gSeries

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