The Translation Dictionary

Here's one of the most elegant shortcuts in Class 12 physics. The far field of a bar magnet has exactly the same mathematical form as the field of an electric dipole. So every result you derived in Chapter 1 can be translated into magnetism with three replacements:

E⃗→B⃗,p⃗→m⃗,14πε0→μ04π\vec{E} \to \vec{B}, \qquad \vec{p} \to \vec{m}, \qquad \frac{1}{4\pi\varepsilon_0} \to \frac{\mu_0}{4\pi}

The complete dipole analogy:

Quantity Electrostatics Magnetism
Constant in dipole-field formula 14πε0\dfrac{1}{4\pi\varepsilon_0} μ04π\dfrac{\mu_0}{4\pi}
Dipole moment p⃗\vec{p} m⃗\vec{m}
Equatorial field (short dipole) −p⃗4πε0r3-\dfrac{\vec{p}}{4\pi\varepsilon_0 r^3} −μ0m⃗4πr3-\dfrac{\mu_0 \vec{m}}{4\pi r^3}
Axial field (short dipole) 2p⃗4πε0r3\dfrac{2\vec{p}}{4\pi\varepsilon_0 r^3} μ0 2m⃗4πr3\dfrac{\mu_0\, 2\vec{m}}{4\pi r^3}
Torque in external field p⃗×E⃗\vec{p} \times \vec{E} m⃗×B⃗\vec{m} \times \vec{B}
Energy in external field −p⃗⋅E⃗-\vec{p} \cdot \vec{E} −m⃗⋅B⃗-\vec{m} \cdot \vec{B}

[JEE Tip] Don't memorise magnetism formulas separately — memorise the dictionary. One table, two chapters.

Axial and Equatorial Fields of a Bar Magnet

For a bar magnet of size ll and moment m⃗\vec{m}, at distance r≫lr \gg l from its centre:

Equatorial field (on the perpendicular bisector):

B⃗E=−μ0m⃗4πr3\vec{B}_E = -\frac{\mu_0 \vec{m}}{4\pi r^3}

Axial field (on the axis):

B⃗A=μ0 2m⃗4πr3\vec{B}_A = \frac{\mu_0\, 2\vec{m}}{4\pi r^3}

Axial and equatorial fields of a bar magnet

Read the signs carefully — they carry the physics:

  • On the axis, B⃗A\vec{B}_A is parallel to m⃗\vec{m}. On the N-side axial point it points away from the N pole; on the S-side axial point it points towards the S pole, but in both cases it is parallel to m⃗\vec{m}.
  • On the equator, B⃗E\vec{B}_E is antiparallel to m⃗\vec{m} — the minus sign! A compass on the perpendicular bisector points opposite to the magnet's moment.
  • At the same distance, the axial field magnitude is twice the equatorial field magnitude: ∣B⃗A∣=2∣B⃗E∣|\vec{B}_A| = 2|\vec{B}_E|.
  • Both fall as 1/r31/r^3 — the universal dipole signature.

[NEET Important] If a short bar magnet's axial field at distance rr equals its equatorial field at distance r′r', then setting 2mr3=mr′3\dfrac{2m}{r^3} = \dfrac{m}{r'^3} gives r=21/3r′r = 2^{1/3}r'. This is a common exam-pattern comparison.

Two Dipoles Together

Place a dipole Q near a fixed dipole P. Q sits in P's field B⃗P\vec{B}_P, so its energy is U=−m⃗Q⋅B⃗PU = -\vec{m}_Q \cdot \vec{B}_P. The rules:

  • Equilibrium is stable when m⃗Q\vec{m}_Q is parallel to B⃗P\vec{B}_P, unstable when antiparallel.
  • On P's axis, B⃗P\vec{B}_P points along m⃗P\vec{m}_P (strength ∝2/r3\propto 2/r^3).
  • On P's normal bisector, B⃗P\vec{B}_P points opposite to m⃗P\vec{m}_P (strength ∝1/r3\propto 1/r^3).

So at the same distance rr:

Position of Q Orientation of m⃗Q\vec{m}_Q Equilibrium Energy
On axis parallel to m⃗P\vec{m}_P Stable −μ02mPmQ4πr3-\dfrac{\mu_0 2 m_P m_Q}{4\pi r^3} (lowest!)
On axis antiparallel to m⃗P\vec{m}_P Unstable +μ02mPmQ4πr3+\dfrac{\mu_0 2 m_P m_Q}{4\pi r^3}
On bisector antiparallel to m⃗P\vec{m}_P Stable −μ0mPmQ4πr3-\dfrac{\mu_0 m_P m_Q}{4\pi r^3}
On bisector parallel to m⃗P\vec{m}_P Unstable +μ0mPmQ4πr3+\dfrac{\mu_0 m_P m_Q}{4\pi r^3}
Either place perpendicular to B⃗P\vec{B}_P Not in equilibrium (torque acts) 0

The lowest-energy configuration of all: Q on the axis with both moments aligned — because the axial field is twice as strong.

[JEE Tip] At a general point at angle θ\theta from the axis (distance rr), the magnitude is B=μ0m4πr31+3cos⁡2θB = \dfrac{\mu_0 m}{4\pi r^3}\sqrt{1 + 3\cos^2\theta} — it interpolates between 2m2m-type (axis, θ=0\theta = 0) and mm-type (equator, θ=90∘\theta = 90^{\circ}). Beyond board level, but standard in JEE.

Solved Examples

Example 1: Axial field of a short magnet

A short bar magnet has magnetic moment 0.48 J/T. Find the magnetic field at a distance of 10 cm from its centre on the axis.

Solution:

  1. Formula: BA=μ04π2mr3B_A = \dfrac{\mu_0}{4\pi}\dfrac{2m}{r^3} with μ04π=10−7\dfrac{\mu_0}{4\pi} = 10^{-7} T m/A.
  2. Substitute: r=0.1r = 0.1 m, r3=10−3r^3 = 10^{-3} m3^3: BA=10−7×2×0.4810−3B_A = 10^{-7} \times \dfrac{2 \times 0.48}{10^{-3}}.
  3. Calculate: BA=10−7×960=0.96×10−4B_A = 10^{-7} \times 960 = 0.96 \times 10^{-4} T.
  4. Answer: 0.96×10−40.96 \times 10^{-4} T (0.96 gauss), directed along the moment (from S to N).

Example 2: Equatorial field of the same magnet

For the same magnet, find the field at 10 cm on the equatorial (perpendicular bisector) line.

Solution:

  1. Magnitude formula: ∣B⃗E∣=μ04πmr3|\vec{B}_E| = \dfrac{\mu_0}{4\pi}\dfrac{m}{r^3} — half the axial value at the same rr. Vectorially, B⃗E\vec{B}_E is opposite to m⃗\vec{m}.
  2. ∣B⃗E∣=10−7×0.4810−3=0.48×10−4|\vec{B}_E| = 10^{-7} \times \dfrac{0.48}{10^{-3}} = 0.48 \times 10^{-4} T.
  3. Answer: 0.48×10−40.48 \times 10^{-4} T (0.48 gauss), directed opposite to the moment m⃗\vec{m}.

Example 3: Where do axial and equatorial fields match?

At what distance on the axis does a short magnet produce the same field magnitude as it produces at 10 cm on the equator?

Solution:

  1. Set equal: 2mrA3=mrE3\dfrac{2m}{r_A^3} = \dfrac{m}{r_E^3} with rE=0.1r_E = 0.1 m.
  2. rA3=2rE3r_A^3 = 2 r_E^3, so rA=21/3×0.1=1.26×0.1r_A = 2^{1/3} \times 0.1 = 1.26 \times 0.1 m.
  3. Answer: rA≈12.6r_A \approx 12.6 cm.

Example 4: Compass direction on the bisector

A compass is placed on the perpendicular bisector of a short bar magnet, far from it. Which way does its north tip point?

Solution:

  1. On the equatorial line, B⃗E=−μ0m⃗4πr3\vec{B}_E = -\dfrac{\mu_0\vec{m}}{4\pi r^3} — antiparallel to m⃗\vec{m}.
  2. The compass aligns along the local field, so its north tip points opposite to the magnet's moment (i.e. in the N-to-S direction of the magnet).
  3. On the axis it would instead point along m⃗\vec{m}.

Example 5: Stable configurations of two needles

Dipole Q is placed at distance rr from dipole P, either on P's axis or on its normal bisector, with m⃗Q\vec{m}_Q parallel or antiparallel to m⃗P\vec{m}_P. Which configurations are in stable equilibrium?

Solution:

  1. Rule: stable when m⃗Q∥B⃗P\vec{m}_Q \parallel \vec{B}_P at Q's location.
  2. On the axis: B⃗P∥m⃗P\vec{B}_P \parallel \vec{m}_P. Stable when m⃗Q\vec{m}_Q is parallel to m⃗P\vec{m}_P.
  3. On the bisector: B⃗P\vec{B}_P is antiparallel to m⃗P\vec{m}_P. Stable when m⃗Q\vec{m}_Q is antiparallel to m⃗P\vec{m}_P.
  4. The reversed orientations in each position are unstable; perpendicular orientations are not equilibria at all (torque acts).

Example 6: The lowest-energy configuration

Among all the stable configurations of Example 5 (same rr), which has the lowest potential energy?

Solution:

  1. U=−mQBPU = -m_Q B_P, so the lowest energy needs the largest BPB_P.
  2. The axial field (∝2/r3\propto 2/r^3) is twice the equatorial field (∝1/r3\propto 1/r^3).
  3. Answer: Q on P's axis with moments parallel: U=−μ02mPmQ4πr3U = -\dfrac{\mu_0 2 m_P m_Q}{4\pi r^3} — twice as negative as the bisector case.

Example 7: Interaction energy numerical

Two short magnets, each of moment 1.0 A m2^2, are coaxial with their moments aligned, centres 1.0 m apart. Find their interaction energy.

Solution:

  1. Field of magnet 1 at magnet 2 (axial): B=10−7×2×1.01.03=2×10−7B = 10^{-7} \times \dfrac{2 \times 1.0}{1.0^3} = 2 \times 10^{-7} T.
  2. Energy: U=−m2B=−1.0×2×10−7U = -m_2 B = -1.0 \times 2 \times 10^{-7}.
  3. Answer: U=−2×10−7U = -2 \times 10^{-7} J. Negative — the aligned coaxial pair is bound (stable).

Example 8: Translating an electrostatics result

The electric field of a short dipole at a general point is E=p4πε0r31+3cos⁡2θE = \dfrac{p}{4\pi\varepsilon_0 r^3}\sqrt{1+3\cos^2\theta}. Write the magnetic counterpart.

Solution:

  1. Apply the dictionary: p→mp \to m, 1/4πε0→μ0/4π1/4\pi\varepsilon_0 \to \mu_0/4\pi, E→BE \to B.
  2. Answer: B=μ0m4πr31+3cos⁡2θB = \dfrac{\mu_0 m}{4\pi r^3}\sqrt{1+3\cos^2\theta}.
  3. Check the limits: θ=0\theta = 0 gives μ02m4πr3\dfrac{\mu_0 2m}{4\pi r^3} (axial); θ=90∘\theta = 90^{\circ} gives μ0m4πr3\dfrac{\mu_0 m}{4\pi r^3} (equatorial). The dictionary works perfectly.

Example 9: Field at a general point (JEE pattern)

A short magnet has moment 1.0 A m2^2. Find the field magnitude at 10 cm from its centre, at 60 degrees from the axis.

Solution:

  1. Formula: B=μ0m4πr31+3cos⁡2θB = \dfrac{\mu_0 m}{4\pi r^3}\sqrt{1+3\cos^2\theta}.
  2. cos⁡60∘=0.5\cos 60^{\circ} = 0.5, so 1+3(0.25)=1.751 + 3(0.25) = 1.75, 1.75≈1.32\sqrt{1.75} \approx 1.32.
  3. μ0m4πr3=10−7×1.010−3=10−4\dfrac{\mu_0 m}{4\pi r^3} = 10^{-7} \times \dfrac{1.0}{10^{-3}} = 10^{-4} T.
  4. Answer: B≈1.32×10−4B \approx 1.32 \times 10^{-4} T.

Example 10: Same field, two distances

The equatorial field of a magnet at 5 cm is B0B_0. At what axial distance is the field also B0B_0?

Solution:

  1. B0=μ0m4π(0.05)3B_0 = \dfrac{\mu_0 m}{4\pi (0.05)^3} and we need μ02m4πr3=B0\dfrac{\mu_0 2m}{4\pi r^3} = B_0.
  2. Dividing: 2(0.05)3r3=1\dfrac{2 (0.05)^3}{r^3} = 1, so r=21/3×5r = 2^{1/3} \times 5 cm ≈6.3\approx 6.3 cm.
  3. Takeaway: the factor 2 always shows up as a 21/3≈1.262^{1/3} \approx 1.26 stretch in distance.