Quick Recap — Magnetic Field of Currents

  • Oersted: a current produces a magnetic field; its direction follows the right-hand thumb rule.
  • Standard fields: straight wire B=μ0I2πrB = \dfrac{\mu_0 I}{2\pi r}; centre of a loop B=μ0I2RB = \dfrac{\mu_0 I}{2R}; solenoid B=μ0nIB = \mu_0 nI (with μ0=4π×107\mu_0 = 4\pi\times10^{-7} T m/A).
  • Ampere's law relates Bdl\oint\vec{B}\cdot d\vec{l} to the enclosed current.
  • Lorentz force: F=qv×B\vec{F} = q\vec{v}\times\vec{B} (F=qvBsinθF = qvB\sin\theta); it does no work, so the speed stays constant.
  • Charge in a field (vBv\perp B): a circular path of radius r=mvqBr = \dfrac{mv}{qB} and period T=2πmqBT = \dfrac{2\pi m}{qB} (independent of speed).

Beyond-NCERT JEE Formulae

The definitions (F=qv×B\vec F=q\vec v\times\vec B, Ampere's law, and B=μ0I2πrB=\dfrac{\mu_0 I}{2\pi r}) are taken as known from the practice sets. This sheet collects the higher-yield results and the extended finite-geometry formulae that JEE Main tests beyond the NCERT core, each with a note on when it applies.

1. Biot-Savart law and standard field sources

  • Biot-Savart (vector form): dB=μ04πIdl×r^r2d\vec B=\dfrac{\mu_0}{4\pi}\dfrac{I\,d\vec l\times\hat r}{r^2}. Reach for this whenever the geometry is an arc, a finite segment or a polygon, i.e. too unsymmetric for Ampere's law.
  • Long straight wire: B=μ0I2πrB=\dfrac{\mu_0 I}{2\pi r}, the lines circling the wire by the right-hand grip.
  • Finite straight wire (perpendicular distance rr; the ends subtend θ1\theta_1 and θ2\theta_2 at the foot of the perpendicular): B=μ0I4πr(sinθ1+sinθ2)B=\dfrac{\mu_0 I}{4\pi r}(\sin\theta_1+\sin\theta_2). A semi-infinite wire ending level with the point gives μ0I4πr\dfrac{\mu_0 I}{4\pi r}, and the infinite wire recovers μ0I2πr\dfrac{\mu_0 I}{2\pi r}.
  • Centre of a circular coil of NN turns: B=μ0NI2RB=\dfrac{\mu_0 N I}{2R}, while a bare arc of angle ϕ\phi contributes μ0Iϕ4πR\dfrac{\mu_0 I\phi}{4\pi R}.
  • On the axis of a loop, a distance xx from the centre: B=μ0IR22(R2+x2)3/2B=\dfrac{\mu_0 I R^2}{2(R^2+x^2)^{3/2}}, which becomes μ0I2R\dfrac{\mu_0 I}{2R} at the centre and dies off as 1x3\dfrac{1}{x^3} far away.
  • Long solenoid (interior): B=μ0nIB=\mu_0 nI with nn the turns per metre; it drops to exactly μ0nI2\dfrac{\mu_0 nI}{2} at each open end.
  • Toroid (inside the core): B=μ0NI2πrB=\dfrac{\mu_0 N I}{2\pi r}, and it is zero everywhere outside.

[JEE Tip] The finite-wire formula is the master key for polygon loops: every side of a regular loop shares the same perpendicular distance and the same pair of half-angles, so the centre field of a square of side aa works out to 22μ0Iπa\dfrac{2\sqrt2\,\mu_0 I}{\pi a}. Learn the route, not the number.

2. Forces on currents

  • On a wire: F=IL×B\vec F=I\vec L\times\vec B, of magnitude BILsinθBIL\sin\theta. In a uniform field a bent or curved wire feels exactly the force of the straight wire joining its ends (the effective length Leff\vec L_{eff}), so a closed loop feels zero net force.
  • Between parallel wires: FL=μ0I1I22πd\dfrac{F}{L}=\dfrac{\mu_0 I_1 I_2}{2\pi d}; parallel currents attract and antiparallel currents repel, the opposite of the rule for like charges.
  • Useful constants: μ02π=2×107\dfrac{\mu_0}{2\pi}=2\times10^{-7} and μ04π=107\dfrac{\mu_0}{4\pi}=10^{-7} in SI units.

[JEE Tip] Effective length is a uniform-field shortcut only. Near another current-carrying wire the field varies as 1r\dfrac{1}{r}, so it is non-uniform and you must integrate rather than collapse the wire to its chord.

3. Charged particle in a magnetic field

  • Circular motion (vB\vec v\perp\vec B): radius r=mvqB=2mKqB=2mqVqBr=\dfrac{mv}{qB}=\dfrac{\sqrt{2mK}}{qB}=\dfrac{\sqrt{2mqV}}{qB}; period T=2πmqBT=\dfrac{2\pi m}{qB}; cyclotron frequency f=qB2πmf=\dfrac{qB}{2\pi m}. The last two are independent of speed and radius, which is exactly what makes the cyclotron work.
  • Helical motion (velocity at angle θ\theta to B\vec B): only v=vsinθv_\perp=v\sin\theta bends the path, so r=mvsinθqBr=\dfrac{mv\sin\theta}{qB}, while v=vcosθv_\parallel=v\cos\theta drives the particle forward one pitch p=vT=2πmvcosθqBp=v_\parallel T=\dfrac{2\pi m v\cos\theta}{qB} per turn.
  • Velocity selector (crossed E\vec E and B\vec B): a charge crosses undeflected only at v=EBv=\dfrac{E}{B}, independent of qq and mm, which is why it heads every mass spectrometer.
  • Cyclotron exit energy: Kmax=q2B2R22mK_{max}=\dfrac{q^2 B^2 R^2}{2m}, fixed entirely by the dee radius RR and the field BB.

[JEE Tip] The magnetic force does no work, so vv and KK never change, only the direction does. Equal-KK particles then compare by rmqr\propto\dfrac{\sqrt m}{q}, but equal-VV particles by rmqr\propto\sqrt{\dfrac{m}{q}}; confusing the two wrecks isotope and e/me/m problems.

4. Magnetic dipole: moment, torque and energy

  • Moment of a coil: M=NIAM=NIA (units A m2^2), pointing along the normal by the right-hand rule.
  • Torque in a field: τ=M×B\vec\tau=\vec M\times\vec B, of magnitude MBsinθMB\sin\theta, largest when the coil's plane contains B\vec B.
  • Orientation energy: U=MB=MBcosθU=-\vec M\cdot\vec B=-MB\cos\theta, so the external work to reorient a dipole is W=MB(cosθ1cosθ2)W=MB(\cos\theta_1-\cos\theta_2).
  • Bar magnet as a solenoid / short dipole: a uniformly magnetised bar behaves as a solenoid of the same moment M=NIAM=NIA; its far field is axial B=μ04π2Mr3B=\dfrac{\mu_0}{4\pi}\dfrac{2M}{r^3} and equatorial B=μ04πMr3B=\dfrac{\mu_0}{4\pi}\dfrac{M}{r^3} (axial twice equatorial, both 1r3\propto\dfrac{1}{r^3}), and its small oscillations in a field obey T=2πIMBT=2\pi\sqrt{\dfrac{I}{MB}} with II the moment of inertia.
  • From a moving charge (beyond NCERT): an orbiting charge has the gyromagnetic ratio ML=q2m\dfrac{M}{L}=\dfrac{q}{2m}, and a charge qq smeared round a ring of radius RR spun at ω\omega carries M=qωR22M=\dfrac{q\omega R^2}{2}.

[JEE Tip] Torque is not energy: turn the coil with MBsinθMB\sin\theta, but budget the work with (cosθ1cosθ2)(\cos\theta_1-\cos\theta_2). And a loop in a uniform field feels a torque yet zero net force, so it rotates on the spot without drifting.

Solved Examples — Beyond-NCERT Formulae

Example 1 — Field at the centre and on the axis of a coil

Q. A flat circular coil of 100100 turns and radius 55 cm carries a steady current of 22 A. Find the magnetic field at its centre and at a point on the axis 55 cm from the centre, and compare the two.

Solution. At the centre all NN turns add, so Bc=μ0NI2RB_c=\dfrac{\mu_0 N I}{2R}: Bc=(4π×107)(100)(2)2(0.05)=2.513×1040.1.B_c=\frac{(4\pi\times10^{-7})(100)(2)}{2(0.05)}=\frac{2.513\times10^{-4}}{0.1}. So Bc=2.51×103B_c=2.51\times10^{-3} T. On the axis, Bx=μ0NIR22(R2+x2)3/2B_x=\dfrac{\mu_0 N I R^2}{2(R^2+x^2)^{3/2}}; putting x=Rx=R makes (R2+x2)3/2=22R3(R^2+x^2)^{3/2}=2\sqrt2\,R^3, so Bx=Bc22B_x=\dfrac{B_c}{2\sqrt2}: Bx=2.51×10322=2.51×1032.828.B_x=\frac{2.51\times10^{-3}}{2\sqrt2}=\frac{2.51\times10^{-3}}{2.828}. So Bx=8.89×104B_x=8.89\times10^{-4} T, only 1220.354\dfrac{1}{2\sqrt2}\approx0.354 of the central value just one radius off-axis. Once you set x=Rx=R the ratio needs no re-substitution.

Example 2 — Field at the centre of a square loop

Q. A wire carries a steady current of 55 A once around a square loop of side 2020 cm. Using the finite-wire result, find the magnetic field at the centre of the square.

Solution. Each side is a finite straight wire at perpendicular distance r=a2=0.1r=\dfrac{a}{2}=0.1 m, and its two ends each subtend 4545^\circ at the centre, so sinθ1+sinθ2=2sin45=2\sin\theta_1+\sin\theta_2=2\sin45^\circ=\sqrt2. One side therefore gives Bside=μ0I4π(a/2)2=2μ0I2πa.B_{side}=\frac{\mu_0 I}{4\pi (a/2)}\sqrt2=\frac{\sqrt2\,\mu_0 I}{2\pi a}. All four sides drive the field the same way at the centre, so they simply add: B=4Bside=22μ0Iπa=22×(4×107)(5)0.2.B=4B_{side}=\frac{2\sqrt2\,\mu_0 I}{\pi a}=2\sqrt2\times\frac{(4\times10^{-7})(5)}{0.2}. So B=22×105=2.83×105B=2\sqrt2\times10^{-5}=2.83\times10^{-5} T. The value drops straight out of the finite-wire law; the circular-loop formula does not apply to a polygon.

Example 3 — Force between two parallel wires

Q. Two long parallel wires 55 cm apart carry steady currents of 1010 A and 1515 A in the same direction. Find the force per unit length between them and its nature, and the total force on a 22 m length.

Solution. With μ02π=2×107\dfrac{\mu_0}{2\pi}=2\times10^{-7}, the force per metre is FL=μ0I1I22πd\dfrac{F}{L}=\dfrac{\mu_0 I_1 I_2}{2\pi d}: FL=(2×107)(10)(15)0.05=3×1050.05.\frac{F}{L}=\frac{(2\times10^{-7})(10)(15)}{0.05}=\frac{3\times10^{-5}}{0.05}. So FL=6×104\dfrac{F}{L}=6\times10^{-4} N/m, and because the currents are parallel the wires attract. Over a 22 m length the total force is F=(FL)L=(6×104)(2).F=\left(\frac{F}{L}\right)L=(6\times10^{-4})(2). So F=1.2×103F=1.2\times10^{-3} N. Reversing one current keeps this magnitude but turns the pull into a push.

Example 4 — Radius, period and frequency of a proton

Q. A proton (m=1.67×1027m=1.67\times10^{-27} kg, q=1.6×1019q=1.6\times10^{-19} C) moves at 2×1062\times10^{6} m/s at right angles to a uniform field of 0.50.5 T. Find the radius, period and frequency of its circular path.

Solution. The magnetic force is centripetal, so r=mvqBr=\dfrac{mv}{qB}: r=(1.67×1027)(2×106)(1.6×1019)(0.5)=3.34×10218×1020.r=\frac{(1.67\times10^{-27})(2\times10^{6})}{(1.6\times10^{-19})(0.5)}=\frac{3.34\times10^{-21}}{8\times10^{-20}}. So r=4.18×102r=4.18\times10^{-2} m, about 4.24.2 cm. The period is T=2πmqBT=\dfrac{2\pi m}{qB}: T=2π(1.67×1027)(1.6×1019)(0.5)=1.049×10268×1020.T=\frac{2\pi(1.67\times10^{-27})}{(1.6\times10^{-19})(0.5)}=\frac{1.049\times10^{-26}}{8\times10^{-20}}. So T=1.31×107T=1.31\times10^{-7} s, and the frequency is f=1T=qB2πm=7.62×106f=\dfrac{1}{T}=\dfrac{qB}{2\pi m}=7.62\times10^{6} Hz, about 7.67.6 MHz. Doubling the speed would double the radius but leave TT and ff unchanged.

Example 5 — Velocity selector, then bending

Q. In a velocity selector a 3×1053\times10^{5} V/m electric field and a 0.20.2 T magnetic field act at right angles to each other and to a proton beam. Find the selected speed. The emerging protons then enter a 0.50.5 T field at right angles; find the radius of their path.

Solution. Undeflected passage needs the electric and magnetic forces to cancel, qE=qvB1qE=qvB_1, so v=EB1v=\dfrac{E}{B_1}, independent of charge and mass: v=3×1050.2.v=\frac{3\times10^{5}}{0.2}. So v=1.5×106v=1.5\times10^{6} m/s. In the second field the magnetic force is centripetal, so r=mvqB2r=\dfrac{mv}{qB_2}: r=(1.67×1027)(1.5×106)(1.6×1019)(0.5)=2.505×10218×1020.r=\frac{(1.67\times10^{-27})(1.5\times10^{6})}{(1.6\times10^{-19})(0.5)}=\frac{2.505\times10^{-21}}{8\times10^{-20}}. So r=3.13×102r=3.13\times10^{-2} m, about 3.13.1 cm. The selector sets the speed and the second field does the bending, so never reuse B1B_1 in the radius.

Example 6 — Torque, energy and work on a coil

Q. A coil of 5050 turns and area 8×1038\times10^{-3} m2^2 carries 33 A in a uniform field of 0.50.5 T. Find its magnetic moment, the maximum torque, the torque when the moment is 3030^\circ from the field, and the work to turn it from alignment to 6060^\circ.

Solution. The moment is M=NIA=(50)(3)(8×103)M=NIA=(50)(3)(8\times10^{-3}), so M=1.2M=1.2 A m2^2. The torque τ=MBsinθ\tau=MB\sin\theta is greatest when the coil's plane lies along B\vec B (so sinθ=1\sin\theta=1): τmax=MB=(1.2)(0.5).\tau_{max}=MB=(1.2)(0.5). So τmax=0.6\tau_{max}=0.6 N m. At θ=30\theta=30^\circ the torque falls to τ=MBsin30=(0.6)(0.5)\tau=MB\sin30^\circ=(0.6)(0.5), giving τ=0.3\tau=0.3 N m. Using U=MBcosθU=-MB\cos\theta, the work to swing the coil from θ1=0\theta_1=0 to θ2=60\theta_2=60^\circ is W=MB(cos0cos60)=(0.6)(10.5).W=MB(\cos0^\circ-\cos60^\circ)=(0.6)(1-0.5). So W=0.3W=0.3 J. The turning factor sinθ\sin\theta and the energy factor (1cosθ)(1-\cos\theta) are different, so do not swap them.

Example 7 — Radius and pitch of a helix

Q. An electron (m=9.1×1031m=9.1\times10^{-31} kg, q=1.6×1019q=1.6\times10^{-19} C) enters a uniform field of 1×1031\times10^{-3} T at a speed of 3×1063\times10^{6} m/s, its velocity making 3030^\circ with the field. Find the radius and the pitch of the resulting helix.

Solution. Split the velocity into v=vsin30=1.5×106v_\perp=v\sin30^\circ=1.5\times10^{6} m/s, which bends the path, and v=vcos30=2.60×106v_\parallel=v\cos30^\circ=2.60\times10^{6} m/s, which carries it along the field. The radius uses vv_\perp, so r=mvqBr=\dfrac{mv_\perp}{qB}: r=(9.1×1031)(1.5×106)(1.6×1019)(103)=1.365×10241.6×1022.r=\frac{(9.1\times10^{-31})(1.5\times10^{6})}{(1.6\times10^{-19})(10^{-3})}=\frac{1.365\times10^{-24}}{1.6\times10^{-22}}. So r=8.53×103r=8.53\times10^{-3} m, about 8.58.5 mm. One full turn takes T=2πmqB=3.57×108T=\dfrac{2\pi m}{qB}=3.57\times10^{-8} s, and in that time vv_\parallel advances the pitch: p=vT=(2.60×106)(3.57×108).p=v_\parallel T=(2.60\times10^{6})(3.57\times10^{-8}). So p=9.28×102p=9.28\times10^{-2} m, about 9.39.3 cm. Only vv_\perp fixes the radius, while vv_\parallel alone sets the pitch.