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CalibratePhysics

Chapter 10

Magnetic Fields due to Electric Current

Maharashtra HSC · 13 subtopics · textbook pages 230–250

Formula SheetEvery formula this chapter can be examined on, in one table.

Constants, units and conventions

FormulaSymbols, units and conditions
μ0=4π×10−7 T m/A≈1.26×10−6 T m/A\mu_0 = 4\pi \times 10^{-7}\ \text{T m/A} \approx 1.26 \times 10^{-6}\ \text{T m/A}
  • Permeability of free space. Every result in this chapter is a free-space (vacuum) result. Working shortcut used in almost every numerical: μ04π=10−7\dfrac{\mu_0}{4\pi} = 10^{-7} T m/A, so μ02π=2×10−7\dfrac{\mu_0}{2\pi} = 2 \times 10^{-7} T m/A.
1 T=1 N A−1m−1=1 N s C−1m−1,1 T=104 gauss1\ \text{T} = 1\ \text{N A}^{-1}\text{m}^{-1} = 1\ \text{N s C}^{-1}\text{m}^{-1}, \qquad 1\ \text{T} = 10^{4}\ \text{gauss}
  • Tesla is the SI unit of magnetic field (magnetic induction) BB; dimensions [B]=[F/qv][B] = [F/qv]. Gauss is a non-SI convenience unit. Earth's surface field ≈3.6×10−5\approx 3.6 \times 10^{-5} T =0.36= 0.36 gauss; MRI magnets 1.5 T to 7 T.
  • Symbol ⊙\odot marks a field or current coming out of the plane of the paper, ⊗\otimes marks one going into it.

Magnetic force and the Lorentz force

FormulaSymbols, units and conditions
F⃗m=q(v⃗×B⃗)\vec{F}_m = q(\vec{v} \times \vec{B})
  • Magnetic force on a charge qq (in C) moving with velocity v⃗\vec{v} (m/s) in a field B⃗\vec{B} (T). For an electron, q=−eq = -e, so F⃗m=−e(v⃗×B⃗)\vec{F}_m = -e(\vec{v} \times \vec{B}).
Fm=qvBsin⁡θF_m = qvB\sin\theta
  • Magnitude, θ\theta = angle between v⃗\vec{v} and B⃗\vec{B}. Zero when θ=0∘\theta = 0^\circ or 180∘180^\circ (velocity parallel or antiparallel to B⃗\vec{B}), maximum qvBqvB when θ=90∘\theta = 90^\circ.
F⃗=q[E⃗+(v⃗×B⃗)]=F⃗e+F⃗m\vec{F} = q\left[\vec{E} + (\vec{v} \times \vec{B})\right] = \vec{F}_e + \vec{F}_m
  • Lorentz force: total force when both an electric field E⃗\vec{E} (V/m) and a magnetic field B⃗\vec{B} act on the charge.
F⃗m⋅v⃗=0⇒Wmagnetic=0\vec{F}_m \cdot \vec{v} = 0 \quad \Rightarrow \quad W_{\text{magnetic}} = 0
  • The magnetic force is always perpendicular to the velocity, so it does no work: it changes the direction of motion but never the speed or the kinetic energy.

Cyclotron motion

FormulaSymbols, units and conditions
qvB=mv2R⇒mv=p=qBRqvB = \dfrac{mv^2}{R} \quad \Rightarrow \quad mv = p = qBR
  • Cyclotron formula, for a charge moving in a plane perpendicular to a uniform B⃗\vec{B}. RR = radius of the circular path (m), pp = linear momentum (kg m/s).
R=mvqB=pqBR = \dfrac{mv}{qB} = \dfrac{p}{qB}
  • Radius of the circular path; heavier or faster particles curve less, stronger fields curve them more.
T=2πRv=2πmqBT = \dfrac{2\pi R}{v} = \dfrac{2\pi m}{qB}
  • Period of revolution. It is independent of the speed and of the radius — the fact the cyclotron is built on.
fc=1T=qB2πmf_c = \dfrac{1}{T} = \dfrac{qB}{2\pi m}
  • Cyclotron frequency (Hz). Resonance condition for the cyclotron: frequency of the applied alternating voltage fa=fcf_a = f_c.
t=T2=πmqBt = \dfrac{T}{2} = \dfrac{\pi m}{qB}
  • Time to complete one semicircle inside a dee — this is the interval after which the electric field between the dees must be reversed. Board numericals ask for exactly this quantity.
K.E.=12mv2=q2B2Rexit22m\text{K.E.} = \dfrac{1}{2}mv^2 = \dfrac{q^2B^2R_{\text{exit}}^2}{2m}
  • Final kinetic energy of the accelerated ion; RexitR_{\text{exit}} = radius of the outermost circular path (radius of a dee). Energy is proportional to Rexit2R_{\text{exit}}^2.
K.E.=2π2mf2R2\text{K.E.} = 2\pi^2 m f^2 R^2
  • Same result written using the oscillator frequency ff instead of BB (obtained by putting B=2πmf/qB = 2\pi m f/q). Use it when the question gives the dee radius and the oscillator frequency.
Δ(K.E.)=qV  per gap crossing\Delta(\text{K.E.}) = qV \ \text{ per gap crossing}
  • VV = potential difference across the gap between the dees. Typical machine values: BB up to 1.5 T, VV up to 10000 V, faf_a about 10 MHz.

Helical motion

FormulaSymbols, units and conditions
v∥=vcos⁡θ,v⊥=vsin⁡θv_\parallel = v\cos\theta, \qquad v_\perp = v\sin\theta
  • Components of velocity parallel and perpendicular to B⃗\vec{B}, with θ\theta the angle between v⃗\vec{v} and B⃗\vec{B}.
Fm on v∥=qv∥Bsin⁡0∘=0F_m \text{ on } v_\parallel = qv_\parallel B\sin 0^\circ = 0
  • The parallel component is untouched by the field, so the particle drifts steadily along B⃗\vec{B}.
r=mv⊥qB,T=2πmqB,pitch=v∥T=2πmv∥qBr = \dfrac{mv_\perp}{qB}, \qquad T = \dfrac{2\pi m}{qB}, \qquad \text{pitch} = v_\parallel T = \dfrac{2\pi m v_\parallel}{qB}
  • Radius, period and pitch of the helix. Pitch = distance advanced along B⃗\vec{B} in one full revolution.

Magnetic force on a current-carrying wire

FormulaSymbols, units and conditions
q=It=ILvdq = It = \dfrac{IL}{v_d}
  • Charge crossing a section in the time the drift velocity vdv_d carries it through a length LL of wire.
Fm=ILB(B⃗⊥wire)F_m = ILB \quad (\vec{B} \perp \text{wire})
  • Force on a straight length LL (m) of wire carrying current II (A) in a perpendicular field BB (T).
F⃗m=I L⃗×B⃗,Fm=ILBsin⁡θ\vec{F}_m = I\,\vec{L} \times \vec{B}, \qquad F_m = ILB\sin\theta
  • General straight-wire form; L⃗\vec{L} is the length vector directed along the current, θ\theta the angle between L⃗\vec{L} and B⃗\vec{B}.
dF⃗m=I dl⃗×B⃗,F⃗m=∫wireI dl⃗×B⃗d\vec{F}_m = I\,d\vec{l} \times \vec{B}, \qquad \vec{F}_m = \int_{\text{wire}} I\,d\vec{l} \times \vec{B}
  • Arbitrarily shaped wire: sum the force on each infinitesimal element.
F⃗m=I(∫dl⃗)×B⃗(B⃗ uniform)\vec{F}_m = I\left(\int d\vec{l}\right) \times \vec{B} \quad (\vec{B} \text{ uniform})
  • For a uniform field the integral reduces to the vector joining the ends of the wire.

Force on a closed circuit in a uniform field

FormulaSymbols, units and conditions
F⃗m=I(∮Cdl⃗)×B⃗=0(B⃗ uniform)\vec{F}_m = I\left(\oint_C d\vec{l}\right) \times \vec{B} = 0 \qquad (\vec{B} \text{ uniform})
  • The sum of the length vectors around a closed circuit is zero, so the net force on any closed circuit in a uniform magnetic field is zero. (A net torque may still act.)

Torque on a current loop; moving coil galvanometer

FormulaSymbols, units and conditions
τ=Il1l2Bsin⁡θ=IABsin⁡θ\tau = I l_1 l_2 B \sin\theta = IAB\sin\theta
  • Torque on a single planar loop of area A=l1l2A = l_1 l_2; θ\theta = angle between the normal n^\hat{n} to the plane of the loop and B⃗\vec{B}.
τ=NIABsin⁡θ\tau = NIAB\sin\theta
  • Flat coil of NN turns. Valid for a planar coil of any shape in a uniform field. Note the trap: if the question gives the angle α\alpha between the plane (or axis) of the coil and B⃗\vec{B}, convert first — θ=90∘−α\theta = 90^\circ - \alpha.
τmax⁡=NIAB(θ=90∘),τmin⁡=0(θ=0∘)\tau_{\max} = NIAB \quad (\theta = 90^\circ), \qquad \tau_{\min} = 0 \quad (\theta = 0^\circ)
  • Maximum torque when the plane of the coil contains B⃗\vec{B}; zero when the plane of the coil is perpendicular to B⃗\vec{B}.
τ=NIAB(radial field, galvanometer)\tau = NIAB \qquad (\text{radial field, galvanometer})
  • In a moving coil galvanometer the soft-iron core makes the field radial, so sin⁡θ=1\sin\theta = 1 always.
Kϕ=NIAB⇒ϕ=(NABK)I⇒ϕ∝IK\phi = NIAB \quad \Rightarrow \quad \phi = \left(\dfrac{NAB}{K}\right)I \quad \Rightarrow \quad \phi \propto I
  • KK = torsional constant of the spring (N m per degree or N m/rad), ϕ\phi = steady angular deflection. Rearranged for the current, I=KϕNABI = \dfrac{K\phi}{NAB}.

Magnetic dipole moment

FormulaSymbols, units and conditions
μ=m=NIA(SI unit: A m2 or J/T)\mu = m = NIA \qquad \text{(SI unit: A m}^2 \text{ or J/T)}
  • Magnetic dipole moment of a coil of NN turns, each of area AA, carrying current II. For a circular coil of radius rr, A=πr2A = \pi r^2. Direction: along n^\hat{n}, given by the right-hand thumb rule.
m⃗=IA⃗(single loop)\vec{m} = I\vec{A} \qquad \text{(single loop)}
  • A⃗\vec{A} has magnitude AA and direction normal to the plane of the loop.
τ⃗=m⃗×B⃗,τ=mBsin⁡θ\vec{\tau} = \vec{m} \times \vec{B}, \qquad \tau = mB\sin\theta
  • Torque on a magnetic dipole in a uniform field — the magnetic analogue of τ⃗=p⃗×E⃗\vec{\tau} = \vec{p} \times \vec{E} for an electric dipole.

Magnetic potential energy of a dipole

FormulaSymbols, units and conditions
U=−m⃗⋅B⃗=−mBcos⁡θU = -\vec{m} \cdot \vec{B} = -mB\cos\theta
  • Potential energy of a magnetic dipole due to its orientation in a field, analogous to U=−p⃗⋅E⃗U = -\vec{p}\cdot\vec{E}.
Umin⁡=−mB (θ=0∘),Umax⁡=+mB (θ=180∘)U_{\min} = -mB \ (\theta = 0^\circ), \qquad U_{\max} = +mB \ (\theta = 180^\circ)
  • Minimum (stable) when m⃗\vec{m} is parallel to B⃗\vec{B}; maximum (unstable) when antiparallel.

Biot-Savart law and the straight wire

FormulaSymbols, units and conditions
dB=μ04π I dl sin⁡θr2dB = \dfrac{\mu_0}{4\pi}\,\dfrac{I\,dl\,\sin\theta}{r^2}
  • Magnitude of the field at a point P produced by a current element I dl⃗I\,d\vec{l}; rr = distance from the element to P, θ\theta = angle between dl⃗d\vec{l} and r⃗\vec{r}.
dB⃗=μ04π I dl⃗×r⃗r3d\vec{B} = \dfrac{\mu_0}{4\pi}\,\dfrac{I\,d\vec{l} \times \vec{r}}{r^3}
  • Vector form. Still an inverse-square law, because r⃗\vec{r} in the numerator carries one power of rr.
B=μ0I2πRB = \dfrac{\mu_0 I}{2\pi R}
  • Field at a perpendicular distance RR from an infinitely long straight wire. Direction: circles round the wire, given by the right-hand thumb rule.
B=μ0I4πRB = \dfrac{\mu_0 I}{4\pi R}
  • Field at a perpendicular distance RR due to a semi-infinite straight wire (one half of the long wire above).
B=0(point on the line of the wire, produced)B = 0 \qquad \text{(point on the line of the wire, produced)}
  • A straight segment contributes nothing at a point lying along its own line, since sin⁡0∘=sin⁡180∘=0\sin 0^\circ = \sin 180^\circ = 0.

Force between two long parallel wires

FormulaSymbols, units and conditions
B1=μ0I12πdB_1 = \dfrac{\mu_0 I_1}{2\pi d}
  • Field produced by wire 1 at the location of wire 2, separation dd (m).
F=I2B1L=μ0I1I2L2πdF = I_2 B_1 L = \dfrac{\mu_0 I_1 I_2 L}{2\pi d}
  • Force on a length LL of wire 2 due to the current in wire 1.
FL=μ0I1I22πd\dfrac{F}{L} = \dfrac{\mu_0 I_1 I_2}{2\pi d}
  • Force per unit length (N/m). Parallel currents attract, antiparallel currents repel. F⃗21=−F⃗12\vec{F}_{21} = -\vec{F}_{12}, in agreement with Newton's third law.
FL=2×10−7 N/mwhen I1=I2=1 A, d=1 m\dfrac{F}{L} = 2 \times 10^{-7}\ \text{N/m} \quad \text{when } I_1 = I_2 = 1\ \text{A},\ d = 1\ \text{m}
  • Definition of the ampere: the constant current which, in two infinitely long parallel wires of negligible cross-section placed 1 m apart in vacuum, produces a force of 2×10−72 \times 10^{-7} N per metre of length on each wire.

Field due to a circular arc

FormulaSymbols, units and conditions
B=μ0Iθ4πrB = \dfrac{\mu_0 I \theta}{4\pi r}
  • Field at the centre O of a circular arc of radius rr subtending an angle θ\theta (in radians) at O. Every element of the arc is perpendicular to r⃗\vec{r}, so sin⁡90∘=1\sin 90^\circ = 1 throughout.
Bsemicircle=μ0I4r(θ=π)B_{\text{semicircle}} = \dfrac{\mu_0 I}{4 r} \qquad (\theta = \pi)
  • Half circle. Two straight leads in line with the centre add nothing.
Bcircle=μ0I2r(θ=2π)B_{\text{circle}} = \dfrac{\mu_0 I}{2 r} \qquad (\theta = 2\pi)
  • Full circular wire, field at the centre.

and 10.14 Circular loop: axial field and field lines

FormulaSymbols, units and conditions
Bz=μ0IR22 (R2+z2)3/2B_z = \dfrac{\mu_0 I R^2}{2\,(R^2 + z^2)^{3/2}}
  • Field on the axis of a circular loop of radius RR, at a distance zz from the centre. The components perpendicular to the axis cancel by symmetry.
B0=μ0I2R(z=0)B_0 = \dfrac{\mu_0 I}{2R} \qquad (z = 0)
  • Field at the centre of a single circular loop.
B0=μ0NI2RB_0 = \dfrac{\mu_0 N I}{2R}
  • Field at the centre of a flat circular coil of NN turns.
Bz=μ0IR22z3=μ04π 2IAz3=μ04π 2mz3(z≫R)B_z = \dfrac{\mu_0 I R^2}{2 z^3} = \dfrac{\mu_0}{4\pi}\,\dfrac{2 I A}{z^3} = \dfrac{\mu_0}{4\pi}\,\dfrac{2 m}{z^3} \qquad (z \gg R)
  • Far axial field of a current loop, with A=πR2A = \pi R^2 and m=IAm = IA. Compare the electric dipole axial field E=14πε02pz3E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{2p}{z^3}.
Bx=μ04π mx3(x≫R)B_x = \dfrac{\mu_0}{4\pi}\,\dfrac{m}{x^3} \qquad (x \gg R)
  • Field on the perpendicular bisector (equatorial line) of a magnetic dipole, from the electrostatic analogue.

Ampere's circuital law

FormulaSymbols, units and conditions
∮CB⃗⋅dl⃗=μ0I\oint_C \vec{B} \cdot d\vec{l} = \mu_0 I
  • Line integral of B⃗\vec{B} around a closed Amperian loop equals μ0\mu_0 times the net current enclosed by that loop.
∮Bcos⁡θ dl=μ0(I1+I2−I3)\oint B\cos\theta\,dl = \mu_0 (I_1 + I_2 - I_3)
  • Sign rule: curl the right palm along the loop with the fingers in the direction of integration; a current along the stretched thumb is positive, a current opposite to it negative. Currents outside the loop contribute nothing to the integral.
B=μ0I2πrB = \dfrac{\mu_0 I}{2\pi r}
  • Long straight wire recovered from Ampere's law with a circular Amperian loop of radius rr, on which B⃗⋅dl⃗=Br dθ\vec{B}\cdot d\vec{l} = B r\,d\theta.
B=μ0I2πr  (a<r<b),B=0  (r>b)B = \dfrac{\mu_0 I}{2\pi r} \ \ (a < r < b), \qquad B = 0 \ \ (r > b)
  • Coaxial cable: inner core of radius aa and outer cylinder of radius bb carrying equal and opposite currents II. Outside the cable the enclosed current is zero.
B=μ0Jr2B = \dfrac{\mu_0 J r}{2}
  • Inside a long cylindrical wire of uniform current density JJ (A/m2^2), at radial distance rr from the axis.
B=μ0J0r23aB = \dfrac{\mu_0 J_0 r^2}{3a}
  • Inside a long cylindrical wire of radius aa whose current density varies as J=J0r/aJ = J_0 r/a.

Solenoid and toroid

FormulaSymbols, units and conditions
B=μ0ni=μ0(NL)iB = \mu_0 n i = \mu_0 \left(\dfrac{N}{L}\right) i
  • Field inside a long (ideal) solenoid; nn = turns per unit length (m−1^{-1}), NN = total turns, LL = length (m), ii = current (A). The field is uniform, parallel to the axis, and independent of the radius. Outside an ideal solenoid, B=0B = 0.
B⋅2πR=μ0Ni⇒B=μ0Ni2πRB \cdot 2\pi R = \mu_0 N i \quad \Rightarrow \quad B = \dfrac{\mu_0 N i}{2\pi R}
  • Field along the central axis of a toroid of mean radius RR with NN total turns. Here B∝1/RB \propto 1/R, so unlike the solenoid the field is not constant across the cross-section. For an ideal toroid, B=0B = 0 at all points outside it.

Results the exercises set

FormulaSymbols, units and conditions
B=μ0IπRsin⁡2θB = \dfrac{\mu_0 I}{\pi R}\sin 2\theta
  • Two long parallel wires a distance RR apart carrying equal currents II in the same direction, at a point P equidistant from both and subtending an angle θ\theta at each wire from the plane containing them. Add the two fields μ0I2πd\dfrac{\mu_0 I}{2\pi d} vectorially; the components perpendicular to the plane cancel and the field at P comes out parallel to the line joining the wires.
p=qBR=qB(S2+L22S)p = qBR = qB\left(\dfrac{S^2 + L^2}{2S}\right)
  • Momentum of a particle deflected across a field region of width LL through a sideways displacement SS, from the chord geometry (R−S)2+L2=R2(R - S)^2 + L^2 = R^2.
I=mgBaI = \dfrac{mg}{Ba}
  • Current needed to levitate a wire (or a loaded loop) of mass mm whose horizontal arm of length aa lies in a perpendicular field BB: set IBa=mgIBa = mg.
Short NotesThe chapter subtopic by subtopic, in the textbook's own order.13 subtopics
  1. 1Introduction
  2. 2Magnetic Force
  3. 3Cyclotron Motion3 board questions
  4. 4Helical Motion
  5. 5Magnetic Force on a Wire Carrying a Current
  6. 6Force on a Closed Circuit in a Magnetic Field1 board question
  7. 7Torque on a Current Loop6 board questions
  8. 8Magnetic Dipole Moment3 board questions
  9. 9Magnetic Field due to a Current: Biot-Savart Law3 board questions
  10. 10Force of Attraction between two Long Parallel Wires2 board questions
  11. 11Magnetic Lines for a Current Loop1 board question
  12. 12Ampere's Law2 board questions
  13. 13Magnetic Field of a Solenoid and a Toroid3 board questions
The whole chapter in brief

What the chapter is about

  • Oersted first showed that a current produces a magnetic field; Gauss, Henry, Faraday and Maxwell established that electric and magnetic fields are partners. Motors, generators, communication systems and computers all follow from it.
  • Two parallel hanging wires attract when the currents are in the same direction and repel when they are opposite. The forces are not electrostatic — the wires stay electrically neutral throughout, so the origin must be magnetic.
  • Right hand thumb rule: grab the wire with the right hand, thumb along the current; the curled fingers give the direction of the circular magnetic field lines.
  • Notation: ⊙\odot means out of the plane of the paper, ⊗\otimes means into it.

10.2 Magnetic force and the Lorentz force

  • Magnetic force on a charge qq moving with velocity v⃗\vec{v} in a field B⃗\vec{B}: F⃗m=q(v⃗×B⃗)\vec{F}_m = q(\vec{v}\times\vec{B}). For an electron F⃗m=−e(v⃗×B⃗)\vec{F}_m = -e(\vec{v}\times\vec{B}).
  • Magnitude Fm=qvBsin⁡θF_m = qvB\sin\theta, direction perpendicular to the plane containing v⃗\vec{v} and B⃗\vec{B}.
  • Lorentz force (both fields present): F⃗=q[E⃗+(v⃗×B⃗)]=F⃗e+F⃗m\vec{F} = q[\vec{E} + (\vec{v}\times\vec{B})] = \vec{F}_e + \vec{F}_m.
  • Consequences: (i) if v⃗\vec{v} is parallel (or antiparallel) to B⃗\vec{B}, Fm=0F_m = 0; (ii) if the charge is stationary, Fm=0F_m = 0 even when B⃗≠0\vec{B} \neq 0.
  • Because F⃗m⊥v⃗\vec{F}_m \perp \vec{v}, F⃗m⋅v⃗=0\vec{F}_m \cdot \vec{v} = 0: the magnetic force never does work. It can change the direction of motion but never the speed or the kinetic energy.
  • The electric force depends only on E⃗\vec{E} and qq; the magnetic force depends on qq, on the speed, and on the angle between v⃗\vec{v} and B⃗\vec{B}.
  • Unit of BB: from B=F/qvB = F/qv, 1 tesla = 1 N s / (C m). 1 T=1041\ \text{T} = 10^4 gauss.

10.3 Cyclotron motion

  • In a uniform field perpendicular to its velocity a charged particle moves in a circle, the magnetic force supplying the centripetal force: qvB=mv2/RqvB = mv^2/R, hence mv=p=qBRmv = p = qBR (the cyclotron formula).
  • Radius R=mv/qBR = mv/qB; period T=2πm/qBT = 2\pi m/qB; cyclotron frequency fc=qB/2πmf_c = qB/2\pi m.
  • The key fact: TT and fcf_c do not depend on the speed or on the radius. The particle takes the same time for every semicircle however fast it goes.

10.3.1 The cyclotron accelerator

  • Invented by Lawrence and Livingston in 1934 to study nuclear structure; accelerates charged particles to MeV-GeV energies for particle-matter interaction studies and for treating certain tumours.
  • Construction: two hollow semicircular metal chambers, the dees D1D_1 and D2D_2, placed in a vacuum chamber, with a uniform magnetic field (up to about 1.5 T) perpendicular to their plane, and a high-frequency alternating voltage (up to 10000 V, about 10 MHz) applied across the gap between them. An ion source sits at O in the gap. The electric and magnetic fields are perpendicular to each other — crossed fields.
  • Working: the magnetic field bends the ion into a semicircle inside a dee (there is no electric field inside a dee); each time it crosses the gap the alternating field accelerates it, adding qVqV to its kinetic energy; the radius grows each time, so the path is a spiral. At the largest radius it is deflected out through an exit slit.
  • Resonance condition: fa=fcf_a = f_c, so that the polarity of the dees reverses exactly as the ion reaches the gap. The interval after which the field must be reversed is t=T/2=πm/qBt = T/2 = \pi m/qB.
  • Final energy: K.E.=q2B2Rexit22m=2π2mf2R2\text{K.E.} = \dfrac{q^2B^2R_{\text{exit}}^2}{2m} = 2\pi^2 m f^2 R^2, proportional to the square of the outermost radius.
  • Accelerators in India: the 2 GeV electron Synchrotron at RRCAT, Indore, and the 8-10 MeV Microtron at Savitribai Phule Pune University.

10.4 Helical motion

  • If the velocity has a component v⃗∥\vec{v}_\parallel along B⃗\vec{B}, then for that component Fm=qv∥Bsin⁡0∘=0F_m = qv_\parallel B \sin 0^\circ = 0, so it is unaffected and the particle drifts steadily along the field.
  • The perpendicular component v⃗⊥\vec{v}_\perp produces the circular motion as before.
  • The two together give a helix: circular motion in the plane perpendicular to B⃗\vec{B} superposed on uniform translation along B⃗\vec{B}.
  • Radius r=mv⊥/qBr = mv_\perp / qB; period T=2πm/qBT = 2\pi m/qB (unchanged); pitch =v∥T= v_\parallel T.

10.5 Magnetic force on a wire carrying a current

  • Straight wire, field perpendicular: the drifting electrons each feel q(v⃗d×B⃗)q(\vec{v}_d\times\vec{B}); with q=IL/vdq = IL/v_d this gives Fm=ILBF_m = ILB.
  • If B⃗\vec{B} is not perpendicular to the wire, F⃗m=IL⃗×B⃗\vec{F}_m = I\vec{L}\times\vec{B}, magnitude ILBsin⁡θILB\sin\theta, where L⃗\vec{L} points along the current.
  • Arbitrarily shaped wire: dF⃗m=I dl⃗×B⃗d\vec{F}_m = I\,d\vec{l}\times\vec{B} and F⃗m=∫I dl⃗×B⃗\vec{F}_m = \displaystyle\int I\,d\vec{l}\times\vec{B}.
  • For uniform B⃗\vec{B}: F⃗m=I(∫dl⃗)×B⃗\vec{F}_m = I\left(\displaystyle\int d\vec{l}\right)\times\vec{B} — only the straight line joining the two ends matters.
  • Diagram (Fig. 10.8): a vertical wire in the plane of the page carrying current II upward, field B⃗\vec{B} shown as dots coming out of the page, electrons drifting downward with velocity v⃗d\vec{v}_d, and the resulting force F⃗m\vec{F}_m marked horizontally, perpendicular to both.

10.6 Force on a closed circuit in a magnetic field

  • Extending the wire result to a closed circuit C: F⃗m=I(∮Cdl⃗)×B⃗\vec{F}_m = I\left(\displaystyle\oint_C d\vec{l}\right)\times\vec{B} for uniform B⃗\vec{B}.
  • The sum of the length vectors right round a closed circuit is zero.
  • Therefore the net force on a closed circuit placed in a uniform magnetic field is zero. This is a standard one-mark question — the answer is simply "zero".
  • Careful: zero net force does not mean zero net torque. A current loop in a uniform field usually experiences a couple.

10.7 Torque on a current loop

  • Take a rectangular loop abcd, sides l1l_1 (ab, cd) and l2l_2 (bc, da), carrying current II in a uniform field B⃗\vec{B}, with ab and cd perpendicular to B⃗\vec{B}. Let θ\theta be the angle between the normal n^\hat{n} to the plane of the loop and B⃗\vec{B}.
  • Forces on bc and da: F=Il2Bsin⁡(90∘−θ)F = Il_2 B\sin(90^\circ - \theta) each. They are equal, opposite and act along the same line, so they cancel completely and produce no torque.
  • Forces on ab and cd: F=Il1BF = Il_1 B each. They are equal and opposite but do not act along the same line, so they form a couple. Moment arm of each about the central axis is 12l2sin⁡θ\dfrac{1}{2}l_2\sin\theta.
  • Torque τ=2×(Il1B×12l2sin⁡θ)=Il1l2Bsin⁡θ=IABsin⁡θ\tau = 2 \times \left(Il_1 B \times \dfrac{1}{2}l_2\sin\theta\right) = Il_1 l_2 B\sin\theta = IAB\sin\theta.
  • For a flat coil of NN turns: τ=NIABsin⁡θ\tau = NIAB\sin\theta. This holds for a planar coil of any shape in a uniform field.
  • This is the principle of an electric motor. To keep the coil rotating past the position where its plane is parallel to B⃗\vec{B}, a commutator with carbon brushes reverses the current every half rotation, so the torque keeps turning the coil the same way.

10.7.1 Moving coil galvanometer

  • Principle: when a coil carrying a current is suspended in a uniform magnetic field, a torque acts on it, tending to rotate it about the axis of suspension so that the magnetic flux through the coil becomes maximum.
  • Construction and working, as the board wants it: (i) a coil of several turns, suspended or pivoted so that it can rotate freely about a fixed axis in a radial uniform magnetic field; (ii) a soft iron cylindrical core makes the field radial and strong; (iii) current through the coil produces τ=NIABsin⁡θ\tau = NIAB\sin\theta, and since the field is radial θ=90∘\theta = 90^\circ, so τ=NIAB\tau = NIAB; (iv) a spring provides a counter torque, so a steady current gives a steady deflection ϕ\phi; (v) the restoring torque of the spring is KϕK\phi, with KK the torsional constant.
  • At equilibrium Kϕ=NIABK\phi = NIAB, so ϕ=(NABK)I\phi = \left(\dfrac{NAB}{K}\right)I, i.e. ϕ∝I\phi \propto I. A galvanometer therefore has a linear (uniform) scale.
  • Diagram: a rectangular coil of NN turns wound on a frame, suspended by a phosphor bronze strip between the concave pole pieces of a permanent magnet, with a soft iron cylindrical core between the poles; a spring at the bottom, a pointer or mirror to read the deflection, and terminals for the current.

10.8 Magnetic dipole moment

  • A current carrying coil behaves as a magnetic dipole with moment m⃗\vec{m} (also written μ⃗\vec{\mu}), directed along the normal n^\hat{n} to the plane of the coil, sense given by the right-hand thumb rule.
  • Magnitude m=NIAm = NIA; SI unit A m2^2, equivalently J/T.
  • Torque on it in a uniform field: τ=mBsin⁡θ\tau = mB\sin\theta, or in vector form τ⃗=m⃗×B⃗\vec{\tau} = \vec{m}\times\vec{B} — the exact analogue of τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E} for an electric dipole.
  • For a single loop, m⃗=IA⃗\vec{m} = I\vec{A}.

10.9 Magnetic potential energy of a dipole

  • A dipole freely suspended in a field has potential energy on account of its orientation: U=−m⃗⋅B⃗=−mBcos⁡θU = -\vec{m}\cdot\vec{B} = -mB\cos\theta, analogous to U=−p⃗⋅E⃗U = -\vec{p}\cdot\vec{E}.
  • Case (i): θ=0∘\theta = 0^\circ gives U=−mBU = -mB, the minimum — m⃗\vec{m} parallel to B⃗\vec{B}, the stable orientation.
  • Case (ii): θ=180∘\theta = 180^\circ gives U=+mBU = +mB, the maximum — m⃗\vec{m} antiparallel to B⃗\vec{B}.

10.10 Biot-Savart law

  • Statement: the magnitude of the field dBdB at a point P due to a current element I dl⃗I\,d\vec{l} is dB=μ04πI dlsin⁡θr2dB = \dfrac{\mu_0}{4\pi}\dfrac{I\,dl\sin\theta}{r^2}, where rr is the distance of P from the element and θ\theta the angle between dl⃗d\vec{l} and r⃗\vec{r}.
  • Vector form: dB⃗=μ04πI dl⃗×r⃗r3d\vec{B} = \dfrac{\mu_0}{4\pi}\dfrac{I\,d\vec{l}\times\vec{r}}{r^3}. The direction of dB⃗d\vec{B} is that of dl⃗×r⃗d\vec{l}\times\vec{r}.
  • μ0=4π×10−7\mu_0 = 4\pi\times 10^{-7} T m/A ≈1.26×10−6\approx 1.26\times 10^{-6} T m/A.
  • It is still an inverse square law: r⃗\vec{r} in the numerator cancels one power of the r3r^3 below.
  • Biot-Savart law plays the role in magnetostatics that Coulomb's law plays in electrostatics.
  • Long straight wire, perpendicular distance RR: integrating over the whole wire (substitute l=Rtan⁡θl = R\tan\theta) gives B=μ0I2πRB = \dfrac{\mu_0 I}{2\pi R}. Half of the wire alone (semi-infinite) gives B=μ0I4πRB = \dfrac{\mu_0 I}{4\pi R}.

10.11 Force between two long parallel wires

  • Wire 1 produces B1=μ0I12πdB_1 = \dfrac{\mu_0 I_1}{2\pi d} at wire 2. The Lorentz force law then gives, on a length LL of wire 2, F21=I2B1L=μ0I1I2L2πdF_{21} = I_2 B_1 L = \dfrac{\mu_0 I_1 I_2 L}{2\pi d}.
  • Force per unit length: FL=μ0I1I22πd\dfrac{F}{L} = \dfrac{\mu_0 I_1 I_2}{2\pi d}.
  • Parallel currents attract; antiparallel currents repel. F⃗21=−F⃗12\vec{F}_{21} = -\vec{F}_{12}, consistent with Newton's third law.
  • Definition of the ampere: two infinitely long parallel wires 1 m apart in vacuum, each carrying the same constant current, experience a force of 2×10−72\times10^{-7} N per metre of length; that current is 1 ampere.
  • Note that for infinitely long wires the total force would be infinite, which is why the result is always quoted per unit length.

10.12 Field due to a current in a circular arc

  • On an arc, dl⃗d\vec{l} is always perpendicular to r⃗\vec{r}, so sin⁡θ=1\sin\theta = 1 and every element contributes in the same sense at the centre.
  • B=μ0Iθ4πrB = \dfrac{\mu_0 I \theta}{4\pi r} at the centre, with the subtended angle θ\theta in radians.
  • Semicircle: B=μ0I4rB = \dfrac{\mu_0 I}{4r}. Full circle: B=μ0I2rB = \dfrac{\mu_0 I}{2r}.
  • Straight sections in line with the centre contribute nothing, because sin⁡0∘=sin⁡180∘=0\sin 0^\circ = \sin 180^\circ = 0. That is the whole trick in the "two straight sections and one arc" problems.

10.13 Axial field of a circular current loop

  • Loop of radius RR in the x-y plane, centre at the origin, point P on the z axis at distance zz; r2=R2+z2r^2 = R^2 + z^2 and every dl⃗d\vec{l} is perpendicular to r⃗\vec{r}.
  • Components of dB⃗d\vec{B} perpendicular to the axis cancel in pairs from diametrically opposite elements; only the z components survive, with dBz=dBcos⁡θdB_z = dB\cos\theta and cos⁡θ=R/R2+z2\cos\theta = R/\sqrt{R^2+z^2}.
  • Result: Bz=μ0IR22(R2+z2)3/2B_z = \dfrac{\mu_0 I R^2}{2(R^2+z^2)^{3/2}}.
  • Setting z=0z = 0: B0=μ0I2RB_0 = \dfrac{\mu_0 I}{2R}, and for NN turns B0=μ0NI2RB_0 = \dfrac{\mu_0 N I}{2R}.

10.14 Magnetic lines for a current loop

  • Diagram (Fig. 10.20): closed loops that pass through the ring, crowded and nearly straight along the axis inside, spreading out and returning round the outside — exactly the pattern of a short bar magnet.
  • Right hand thumb rule for a loop: curl the fingers of the right hand along the current in the wire; the stretched thumb points along the field on the axis, i.e. towards the north face.
  • The face from which the field lines emerge behaves as the north pole, the other face as the south pole.
  • For z≫Rz \gg R: Bz=μ0IR22z3=μ04π2IAz3=μ04π2mz3B_z = \dfrac{\mu_0 I R^2}{2z^3} = \dfrac{\mu_0}{4\pi}\dfrac{2IA}{z^3} = \dfrac{\mu_0}{4\pi}\dfrac{2m}{z^3}, with m=IAm = IA. So at large distances a current loop is a magnetic dipole. B⃗z\vec{B}_z and m⃗\vec{m} point the same way.
  • By the electrostatic analogue, on the perpendicular bisector B⃗=μ04πm⃗x3\vec{B} = \dfrac{\mu_0}{4\pi}\dfrac{\vec{m}}{x^3} for x≫Rx \gg R.
  • Fundamental difference between an electric and a magnetic dipole: an electric dipole can be split into two isolated charges, but a magnetic dipole cannot be split into isolated poles — no magnetic monopole has ever been found.

10.15 Ampere's circuital law

  • Statement: the line integral of the magnetic induction B⃗\vec{B} around any closed path in free space equals μ0\mu_0 times the total current flowing through the area bounded by the path: ∮B⃗⋅ds⃗=μ0I\displaystyle\oint \vec{B}\cdot d\vec{s} = \mu_0 I.
  • The closed path is called the Amperian loop; II is the net current it encircles.
  • Since B⃗⋅dl⃗=B dlcos⁡θ\vec{B}\cdot d\vec{l} = B\,dl\cos\theta, the law is an integral of the tangential component of B⃗\vec{B} round the loop.
  • Sign convention: curl the right palm along the loop with the fingers in the direction of integration; a current parallel to the stretched thumb is positive, one opposite to it negative. For the standard figure with I1,I2I_1, I_2 out of the page, I3I_3 into the page and I4I_4 outside the loop: ∮Bcos⁡θ dl=μ0(I1+I2−I3)\displaystyle\oint B\cos\theta\,dl = \mu_0(I_1 + I_2 - I_3). I4I_4 contributes nothing, as its contributions cancel over the full loop.
  • Ampere's law plays the role in magnetostatics that Gauss' law plays in electrostatics; it can be derived from the Biot-Savart law and is at its most useful when the current distribution is symmetric.
  • Long straight wire: take a circle of radius rr round the wire, on which BB is constant and tangential, so B⃗⋅dl⃗=Br dθ\vec{B}\cdot d\vec{l} = B r\,d\theta and ∮B⃗⋅dl⃗=B(2πr)=μ0I\displaystyle\oint\vec{B}\cdot d\vec{l} = B(2\pi r) = \mu_0 I, giving B=μ0I2πrB = \dfrac{\mu_0 I}{2\pi r}.

10.16 Solenoid

  • A solenoid is a long, closely wound helical coil whose diameter is much smaller than its length.
  • Inside, the field lines are dense, parallel and uniform along the axis; outside they are widely spaced, so the field there is weak. In an ideal solenoid (infinite length, square cross-section wire, very closely wound) the field inside is uniform and along the axis, and outside it is exactly zero.
  • Derivation: take a rectangular Amperian loop abcd with side ab of length LL inside and parallel to the axis, cd outside, bc and da perpendicular to the axis. Then ∫ab+∫bc+∫cd+∫da=μ0I\displaystyle\int_{ab} + \int_{bc} + \int_{cd} + \int_{da} = \mu_0 I. The bc and da integrals vanish because B⃗⊥dl⃗\vec{B} \perp d\vec{l} there; the cd integral vanishes because B=0B = 0 outside. So BL=μ0IBL = \mu_0 I.
  • With nn turns per unit length and current ii, the current enclosed is I=nLiI = nLi, so BL=μ0nLiBL = \mu_0 nLi and B=μ0niB = \mu_0 n i.
  • Valid for a real solenoid too at points near the middle, but not near its ends.

10.16 Toroid

  • A toroid is a solenoid of finite length bent into a hollow circular tube, like the inner tube of a tyre.
  • The field lines inside are concentric circles; the direction of B⃗\vec{B} at a point is along the tangent to the circle through that point, fixed by the direction of the current.
  • Derivation: take a circular Amperian loop of radius RR along the central axis of the tube. Here B⃗\vec{B} and dl⃗d\vec{l} are in the same direction, so θ=0∘\theta = 0^\circ, cos⁡θ=1\cos\theta = 1, and ∮B⃗⋅dl⃗=B∮dl=B(2πR)\displaystyle\oint\vec{B}\cdot d\vec{l} = B\oint dl = B(2\pi R). The net enclosed current is NiNi, so B(2πR)=μ0NiB(2\pi R) = \mu_0 Ni and B=μ0Ni2πRB = \dfrac{\mu_0 N i}{2\pi R}.
  • Since B∝1/RB \propto 1/R, the field is not constant over the cross-section of a toroid — unlike a solenoid. For an ideal toroid, B=0B = 0 everywhere outside.

Electrostatic - magnetostatic analogy

ElectrostaticsMagnetostatics
Coulomb's lawBiot-Savart law
Gauss' lawAmpere's circuital law
14πε0\dfrac{1}{4\pi\varepsilon_0}μ04π\dfrac{\mu_0}{4\pi}
Electric dipole moment p⃗\vec{p}Magnetic dipole moment m⃗\vec{m}
τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E}τ⃗=m⃗×B⃗\vec{\tau} = \vec{m}\times\vec{B}
U=−p⃗⋅E⃗U = -\vec{p}\cdot\vec{E}U=−m⃗⋅B⃗U = -\vec{m}\cdot\vec{B}
Axial field 14πε02pz3\dfrac{1}{4\pi\varepsilon_0}\dfrac{2p}{z^3}Axial field μ04π2mz3\dfrac{\mu_0}{4\pi}\dfrac{2m}{z^3}
Equatorial field 14πε0px3\dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{x^3}Equatorial field μ04πmx3\dfrac{\mu_0}{4\pi}\dfrac{m}{x^3}

Distinguish between: electric force and magnetic force on a charge

Electric force F⃗e=qE⃗\vec{F}_e = q\vec{E}Magnetic force F⃗m=q(v⃗×B⃗)\vec{F}_m = q(\vec{v}\times\vec{B})
Acts on a charge whether it moves or notActs only on a moving charge
Independent of the direction of motionDepends on the angle between v⃗\vec{v} and B⃗\vec{B}
Along (or opposite to) E⃗\vec{E}Perpendicular to both v⃗\vec{v} and B⃗\vec{B}
Does work; changes speed and kinetic energyDoes no work; changes direction only

Distinguish between: Biot-Savart law and Ampere's law

Biot-Savart lawAmpere's circuital law
dB⃗=μ04πI dl⃗×r⃗r3d\vec{B} = \dfrac{\mu_0}{4\pi}\dfrac{I\,d\vec{l}\times\vec{r}}{r^3}∮B⃗⋅dl⃗=μ0I\displaystyle\oint\vec{B}\cdot d\vec{l} = \mu_0 I
Field of a single current element, summed by integrationField found from the net current enclosed by a loop
Works for any current distribution, symmetric or notPractical only when the distribution is symmetric
Magnetostatic analogue of Coulomb's lawMagnetostatic analogue of Gauss' law

Distinguish between: solenoid and toroid

SolenoidToroid
Straight helical coil, length much greater than diameterSolenoid bent into a closed circular ring
B=μ0niB = \mu_0 n i insideB=μ0Ni2πRB = \dfrac{\mu_0 N i}{2\pi R} along the central axis
Field uniform inside, independent of position across the sectionField varies as 1/R1/R, not uniform across the section
Field lines straight inside, closing outside; B=0B = 0 outside an ideal solenoidField lines are closed concentric circles inside; B=0B = 0 outside an ideal toroid
Has identifiable north and south endsHas no free ends and no poles

Traps that cost marks

  • Magnetic force does no work. If a question asks what happens to the kinetic energy of a charge entering a magnetic field perpendicular to v⃗\vec{v}, the answer is that it remains unchanged.
  • θ\theta in τ=NIABsin⁡θ\tau = NIAB\sin\theta is measured from the normal to the plane of the coil, not from the plane. When the question says "the axis of the coil is inclined at 30∘30^\circ to B⃗\vec{B}", the axis is the normal, so θ=90∘−30∘=60∘\theta = 90^\circ - 30^\circ = 60^\circ. Read the wording of the paper carefully: board solutions have used this conversion.
  • In the cyclotron the quantity asked for is almost always the half period t=πm/qBt = \pi m / qB, the interval between field reversals — not the full period T=2πm/qBT = 2\pi m/qB.
  • nn in B=μ0niB = \mu_0 n i is turns per metre, not the total number of turns. Divide by the length first. Two layers of windings of 500 turns each means N=1000N = 1000.
  • In the toroid formula B=μ0Ni/2πRB = \mu_0 N i / 2\pi R, NN is the total number of turns, not turns per unit length, and RR is the radius of the Amperian circle (the mean radius of the tube).
  • Do not mix up B=μ0I2πRB = \dfrac{\mu_0 I}{2\pi R} (long straight wire) with B=μ0I2RB = \dfrac{\mu_0 I}{2R} (centre of a circular loop). One has π\pi in it, the other does not.
  • Net force on a closed circuit in a uniform field is zero, but the net torque is generally not zero. Do not write that both vanish.
  • Convert centimetres and millimetres to metres, and diameter to radius, before substituting. Circular coil problems usually give the diameter.
  • A straight wire segment produces no field at a point lying on the line of the wire produced, because sin⁡θ=0\sin\theta = 0 there. Do not attempt to add a contribution from it.
  • Ampere's law counts only the current enclosed by the Amperian loop; a current outside contributes zero to the line integral, even though it does contribute to B⃗\vec{B} at points on the loop.
  • Parallel currents attract, antiparallel currents repel. This is the opposite of the like-charges rule from electrostatics, and it is easy to write down backwards.
  • State the units: BB in tesla (or Wb/m2^2), mm in A m2^2 (or J/T), τ\tau in N m, F/LF/L in N/m. Marks are given for units in numericals.
Solved Numerical ExamplesWorked numericals to attempt first, each with a hint before the full solution.Coming soon

These are being added chapter by chapter. They are solved numericals from the prescribed book and the reference guides — not previous board questions, which live under Practice — so that you can work through the method before meeting it in a real paper.

Important DerivationsEvery derive / obtain / prove question in this chapter. 3 have come up in two or more papers.6
  1. 1
    Orbital magnetic moment of an electron revolving around the nucleus (and Bohr magneton) Repeats
    Derive an expression for the orbital magnetic moment of an electron revolving around the nucleus in an atom. State the formula for the Bohr magneton.

    Asked in: March 2014; October 2014; February 2020; July 2022 (Q.19, 3 marks); July 2023 (Q.20, 3 marks)

    Show the derivation
    Expression for magnetic dipole moment:
    Step 1
    Consider an electron of mass mem_e and charge e revolving in a circular orbit of radius r around the positive nucleus in clockwise direction, leading to an anticlockwise current.
    Step 2
    If the electron travels a distance 2πr2\pi r in time T then, its orbital speed v=2πr/Tv=2\pi r/T
    Step 3
    Magnitude of circulating current is given by,
    I=e(1T)I=e\left(\dfrac{1}{T}\right)
    But, T=2πrvT=\dfrac{2\pi r}{v}
    ∴I=e(12πr/v)=ev2πr....(1)\therefore I=e\left(\dfrac{1}{2\pi r/v}\right)=\dfrac{ev}{2\pi r}\qquad....(1)
    Step 4
    The orbital magnetic moment associated with orbital current loop is given by,
    morb=IA=ev2πr×πr2(∵Area of current loop, A=πr2)m_{orb}=IA=\dfrac{ev}{2\pi r}\times\pi r^2\qquad(\because\text{Area of current loop, }A=\pi r^2)
    ∴morb=evr2....(2)\therefore m_{orb}=\dfrac{evr}{2}\qquad....(2)
    Step 5
    The angular momentum of an electron due to its orbital motion is given by,
    L=mevr....(3)L=m_evr\qquad....(3)
    Step 6
    Multiplying and dividing the R.H.S of equation (2) by mem_e,
    morb=e2me×mevrm_{orb}=\dfrac{e}{2m_e}\times m_evr
    ∴morb=eL2me....(4)\therefore m_{orb}=\dfrac{eL}{2m_e}\qquad....(4)
    Step 7
    This equation shows that orbital magnetic moment is proportional to the angular momentum. But as the electron bears negative charge, the orbital magnetic moment and orbital angular momentum are in opposite directions and perpendicular to the plane of the orbit.
    Using vector notation, m⃗orb=−(e2me)L⃗\vec{m}_{orb}=-\left(\dfrac{e}{2m_e}\right)\vec{L}
  2. 2
    Magnetic induction of a toroid (N turns) Repeats
    Obtain an expression for magnetic induction of a toroid of 'N' turns about an axis passing through its centre and perpendicular to its plane.

    Asked in: March 2014; February 2023 (Q.4, 2 marks)

    Show the derivation
    StatementThe line integral of magnetic field of induction B⃗\vec{B} around any closed path in free space is equal to absolute permeability of free space μ0\mu_0 times the total current flowing through area bounded by the path.
    Mathematically, ∮B⃗⋅ds⃗=μ0I\oint\vec{B}\cdot\vec{ds}=\mu_0I
    The sign ∮\oint indicates that the integral is to be evaluated over a closed loop called Amperian loop. The current I on the right hand side is the net current encircled by the Amperian loop.
    Explanation:
    Step 1
    Consider cross-sections of four long straight wires carrying currents I1I_1, I2I_2, I3I_3, I4I_4 into or out of the plane of the paper are shown in figure below.
    Step 2
    An Amperian loop is drawn to encircle 3 of the current wires and not the fourth one.
    Step 3
    As the current goes perpendicular to the plane of the paper, B⃗\vec{B} is in the plane of the paper even if its direction is unknown.
    Step 4
    The length element on the Amperian loop is dl⃗d\vec{l} (in the plane of the paper).
    ∴B⃗⋅dl⃗=Bdlcos⁡θ,\therefore \vec{B}\cdot d\vec{l}=Bdl\cos\theta,
    Using Ampere's law, ∮B⃗⋅dl⃗=∮Bdlcos⁡θ=μ0I\oint\vec{B}\cdot d\vec{l}=\oint Bdl\cos\theta=\mu_0I
    Step 5
    Thus the integration is over the product of length dl of the Amperian loop and the component of the magnetic field B cos θ, tangent to the loop.
    Step 6
    Using curled palm right hand thumb rule, for the distribution of currents as shown I1I_1 and I2I_2 are coming out of the paper, (⊙) parallel to the stretched thumb. Hence these are positive. I3I_3, on the other hand is going into the plane of the paper (⊗). Thus, it is negative.
    ∴∮Bcos⁡θdl=μ0(I1+I2−I3)\therefore \oint B\cos\theta dl=\mu_0(I_1+I_2-I_3)
    The Current I4I_4 is not within the Amperian loop. As the integration is over a full loop, contributions of I4I_4 to B cancel out.
    Expression for magnetic induction at a point along the axis of a toroid:
    Step 1
    Consider a toroid carrying steady current I and having turns N.
    Step 2
    The magnetic field around the toroid consists of concentric circular lines of force around it. Magnetic field is produced, when a steady current 'I' flows through toroid.
    Step 3
    The direction of magnetic field at a point is along the tangent to the circular path at that point.
    Step 4
    Let R be the radius of the Amperian loop. This loop is concentric with the axis of toroid. P is a point on the loop.
    Step 5
    Applying Ampere's law,
    ∮B⃗⋅dl⃗=μ0I=μ0Ni....(1)\oint\vec{B}\cdot d\vec{l}=\mu_0I=\mu_0Ni\qquad....(1)
    where,
    N = total number of turns in the toroid.
    I = total current flowing through toroid.
    i = Current flowing in each turn
    Now, ∮B⃗⋅dl⃗=∮Bdlcos⁡θ....(2)\oint\vec{B}\cdot d\vec{l}=\oint Bdl\cos\theta\qquad....(2)
    Step 6
    But, B⃗\vec{B} and dl⃗d\vec{l} are in same direction
    ∴θ=0°\therefore \theta=0°
    ∴cos⁡θ=1\therefore \cos\theta=1
    ∴\therefore Equation (2) can be written as,
    ∮B⃗⋅dl⃗=∮Bdl=B∮dl....(3)\oint\vec{B}\cdot d\vec{l}=\oint Bdl=B\oint dl\qquad....(3)
    Step 7
    Also ∮dl=2πR\oint dl=2\pi R
    ....(total length of circle is its circumference)
    From equation (3),
    ∮B⃗⋅dl⃗=B(2πR)....(4)\oint\vec{B}\cdot d\vec{l}=B(2\pi R)\qquad....(4)
    Step 8
    From equation (1) and (4),
    B(2πR)=μ0NiB(2\pi R)=\mu_0Ni
    ∴B=μ0Ni2πR....(5)\therefore B=\dfrac{\mu_0Ni}{2\pi R}\qquad....(5)
    This is the required expression.
  3. 3
    Shunt resistance for a moving-coil galvanometer, S=Gn−1S = \dfrac{G}{n-1}
    For a moving coil galvanometer, show that S=Gn−1S = \dfrac{G}{n-1}, where S is shunt resistance, G is galvanometer resistance, n is the ratio of total current to the full scale deflection current.

    Asked in: July 2023 (Q.9, 2 marks)

    Show the derivation
    Step 1
    To use a M.C.G as an ammeter, a shunt (low resistance) is connected in parallel to the coil of M.C.G.
    Step 2
    In the arrangement as shown in the figure, I and IgI_g are the current through the circuit and galvanometer respectively.
    Therefore, the current through shunt S is,
    Is=(I−Ig)I_s=(I-I_g)
    Step 3
    Since S and G are parallel, potential difference across them is same.
    ∴GIg=SIs\therefore GI_g=SI_s
    ∴GIg=S(I−Ig)\therefore GI_g=S(I-I_g)
    ∴S=(IgI−Ig)G....(1)\therefore S=\left(\dfrac{I_g}{I-I_g}\right)G\qquad....(1)
    Equation (1) is useful to calculate the range of current that the galvanometer can measure.
    Step 4
    If the current I is n times current IgI_g, then I=nIgI=nI_g. Using this in equation (1),
    S=(GIgnIg−Ig)S=\left(\dfrac{GI_g}{nI_g-I_g}\right)
    ∴S=Gn−1\therefore S=\dfrac{G}{n-1}
    This is the required shunt to increase the range n times.
    Step 5
    If IsI_s is the current through the shunt resistance, then the remaining current (I−Is)(I-I_s) will flow through galvanometer.
    ∴G(I−Is)=SIs\therefore G(I-I_s)=SI_s
    ∴GI−GIs=SIs\therefore GI-GI_s=SI_s
    ∴SIs+GIs=GI\therefore SI_s+GI_s=GI
    ∴IsI=(GS+G)\therefore \dfrac{I_s}{I}=\left(\dfrac{G}{S+G}\right)
    This equation gives the fraction of the total current through the shunt resistance.
  4. 4
    Deflection of a moving-coil galvanometer is proportional to the current
    Show that the deflection produced in a moving coil galvanometer is directly proportional to the current flowing through its coil or vice-versa.

    Asked in: July 2023 (Q.16, 3 marks)

    Show the derivation
    [From 10.7, Q1]
    Principle of M.C.G:
    When a coil carrying an electric current is suspended in a uniform magnetic field, a torque acts on it. This torque tends to rotate the coil about the axis of suspension so that the magnetic flux passing through the coil is maximum.
    Working:
    Step 1
    M.C.G. consists of a coil of several turns mounted (suspended or pivoted) in such a way that it can freely rotate about a fixed axis, in a radial uniform magnetic field.
    Step 2
    A soft iron cylindrical core makes the field radial and strong.
    Step 3
    The coil rotates due to a torque acting on it as the current flows through it. Torque acting on current carrying coil is τ=NIABsin⁡θ\tau=NIAB\sin\theta.
    Here θ=90°\theta=90° as the field is radial.
    ∴τ=NIAB\therefore \tau=NIAB
    where A is the area of the coil, B the strength of the magnetic field, N the number of turns of the coil and I the current in the coil.
    Step 4
    This torque is counter balanced by a torque due to a spring fitted at the bottom so that a fixed steady current I in the coil produces a steady angular deflection φ.
    Step 5
    Larger the current is, larger is the deflection and larger is the torque due to the spring. If the deflection is φ, the restoring torque due to the spring is equal to Kφ where K is the torsional constant of the spring.
    Thus, Kφ = NIAB,
    and the deflection ϕ=(NABK)I\text{and the deflection }\phi=\left(\dfrac{NAB}{K}\right)I
    This means, the deflection φ is proportional to the current I i.e., ϕ∝I\phi\propto I.Working [(iii), (iv), and (v)]
  5. 5
    Force on a closed circuit of arbitrary shape in a uniform magnetic field
    Assuming an equation of magnetic force due to an arbitrarily shaped wire, obtain an expression for force on a closed circuit in a uniform magnetic field.

    Asked in: June 2025 (Q.7, 2 marks)

    Show the derivation

    The question is a real board question. This working is ours — no source printed a derivation for it.

    Diagram

    Draw a closed loop of arbitrary (irregular) shape carrying a current II, placed in a uniform magnetic field B⃗\vec{B} shown by equally spaced parallel arrows. Mark a small element of the wire dl⃗d\vec{l} on the loop, with the current direction arrowed along it, and label the start and end points of the circuit as the same point PP.

    Starting point

    For a small element dl⃗d\vec{l} of a wire carrying current II in a magnetic field B⃗\vec{B}, the force is

    dF⃗=I dl⃗×B⃗d\vec{F} = I\,d\vec{l} \times \vec{B}

    For a wire of arbitrary shape the total force is the sum of these over the whole wire:

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

    Derivation

    The current II is the same at every point of a series circuit, and the field is uniform, so both II and B⃗\vec{B} are constants and can be taken outside the integral:

    F⃗=I(∮dl⃗)×B⃗\vec{F} = I \left(\oint d\vec{l}\right) \times \vec{B}

    The circle on the integral is the point: the circuit is closed, so the path starts and ends at the same point PP. The vector sum of the small displacements around a closed path is the displacement from PP back to PP, which is the null vector:

    ∮dl⃗=0⃗\oint d\vec{l} = \vec{0}

    Hence

     F⃗=I(0⃗)×B⃗=0⃗ \boxed{\,\vec{F} = I\left(\vec{0}\right) \times \vec{B} = \vec{0}\,}

    Conclusion

    The net magnetic force on **any** closed circuit of any shape placed in a **uniform** magnetic field is zero, whatever the current and whatever the orientation.

    Two cautions worth writing:

    • Zero net force does not mean zero torque. A current loop in a uniform field

    generally experiences a couple, τ⃗=m⃗×B⃗\vec{\tau} = \vec{m} \times \vec{B}, which is what turns the coil of a motor and of a moving-coil galvanometer.

    • The result depends on the field being uniform. In a non-uniform field

    B⃗\vec{B} cannot come out of the integral and the net force is generally not zero.

  6. 6
    Magnetic field at the centre of a circular arc of current-carrying wire (Biot-Savart law) Repeats
    Derive an expression for the magnetic field produced at the centre of a circular arc of a wire carrying current I.

    Asked in: June 2025 (Q.20, 3 marks); February 2026 (Q.9, 2 marks)

    Show the derivation

    The question is a real board question. This working is ours — no source printed a derivation for it.

    Diagram

    Draw a circular arc of radius rr with its centre at OO, subtending an angle ϕ\phi at OO, carrying current II. Mark a small element dl⃗d\vec{l} on the arc, the position vector r⃗\vec{r} from that element to OO, and the angle between them. Show the resulting field dB⃗d\vec{B} at OO as an arrow perpendicular to the plane of the paper (into the page for a clockwise current), with the two straight radial leads drawn along OAOA and OBOB.

    Starting point — the Biot-Savart law

    The magnetic induction at a point due to a current element I dl⃗I\,d\vec{l} at a position r⃗\vec{r} from it is

    dB⃗=μ04π I dl⃗×r⃗r3⟹dB=μ04π I dlsin⁡θr2d\vec{B} = \dfrac{\mu_0}{4\pi}\,\dfrac{I\,d\vec{l} \times \vec{r}}{r^{3}} \qquad\Longrightarrow\qquad dB = \dfrac{\mu_0}{4\pi}\,\dfrac{I\,dl \sin\theta}{r^{2}}

    Derivation

    Take the point at the centre OO of the arc. Every element dl⃗d\vec{l} of the arc is a tangent to the circle, and the line joining it to the centre is a radius, so the two are always perpendicular:

    θ=90∘,sin⁡θ=1\theta = 90^\circ, \qquad \sin\theta = 1

    Every element is also at the same distance rr from OO. Therefore

    dB=μ04π I dlr2dB = \dfrac{\mu_0}{4\pi}\,\dfrac{I\,dl}{r^{2}}

    By the right-hand rule, dB⃗d\vec{B} from every element of the arc points the same way — perpendicular to the plane of the arc — so the contributions add as scalars rather than as vectors:

    B=∫dB=μ0I4πr2∫dlB = \int dB = \dfrac{\mu_0 I}{4\pi r^{2}} \int dl

    The integral is simply the length of the arc, and an arc of radius rr subtending an angle ϕ\phi (in radians) at the centre has length l=rϕl = r\phi:

    B=μ0I4πr2×rϕB = \dfrac{\mu_0 I}{4\pi r^{2}} \times r\phi

     B=μ0Iϕ4πr \boxed{\,B = \dfrac{\mu_0 I \phi}{4\pi r}\,}

    Special cases

    • **Full circular loop**, ϕ=2π\phi = 2\pi:

    B=μ0I(2π)4πr=μ0I2rB = \dfrac{\mu_0 I (2\pi)}{4\pi r} = \dfrac{\mu_0 I}{2r}.

    • **Semicircle**, ϕ=π\phi = \pi: B=μ0I4rB = \dfrac{\mu_0 I}{4r}.
    • **Quarter circle**, ϕ=π/2\phi = \pi/2: B=μ0I8rB = \dfrac{\mu_0 I}{8r}.

    The straight radial leads running to and from the centre contribute nothing, because for them dl⃗d\vec{l} is along r⃗\vec{r} and sin⁡θ=0\sin\theta = 0.