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Q.Establish expression for magnetic field at equatorial position of a magnet.

Bihar BsebBihar Board Intermediate 2022Subjective· 5mImportance★★★★★
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Equatorial field of a bar magnet: Beq=μ04πM(r2+l2)3/2≈μ04πMr3B_{eq}=\dfrac{\mu_0}{4\pi}\dfrac{M}{(r^2+l^2)^{3/2}}\approx\dfrac{\mu_0}{4\pi}\dfrac{M}{r^3}, antiparallel to MM.

Set-up: Consider a bar magnet NS of magnetic length 2l2l, with pole strength mm (so M=m⋅2lM=m\cdot 2l). Let P be a point on the equatorial line (perpendicular bisector of the magnet) at distance rr from its centre O.

Step 1 — Field due to each pole: The distance of P from either pole is

d=r2+l2.d=\sqrt{r^2+l^2}.

Field at P due to the N-pole (repulsive, along N→P):

BN=μ04πm(r2+l2)(directed away from N).B_N=\frac{\mu_0}{4\pi}\frac{m}{(r^2+l^2)}\quad(\text{directed away from N}).

Field due to the S-pole (attractive, along P→S):

BS=μ04πm(r2+l2)(directed towards S).B_S=\frac{\mu_0}{4\pi}\frac{m}{(r^2+l^2)}\quad(\text{directed towards S}).

Both have equal magnitude.

Step 2 — Resolve the fields: Resolve BNB_N and BSB_S into components along and perpendicular to the axis (i.e. parallel to NS and along OP).

  • The components perpendicular to the magnet's axis (along OP) are equal and opposite → they cancel.
  • The components parallel to the axis (each Bcos⁡θB\cos\theta, directed from N to S, i.e. antiparallel to MM) add up.

Here cos⁡θ=lr2+l2\cos\theta=\dfrac{l}{\sqrt{r^2+l^2}}.

Step 3 — Net field: …

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