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CalibratePhysics

1.10

Electric Dipole

Electric Charges and Fields · CBSE

Theory

Definition

An electric dipole is a pair of equal and opposite point charges +q+q and −q-q separated by a distance 2a2a. The line joining them defines the dipole axis, and its midpoint is the centre of the dipole. By convention the direction of the dipole is from −q-q to +q+q.

p⃗=q (2a) p^\vec{p} = q\,(2a)\,\hat{p}

  • The dipole moment p⃗\vec{p} is a vector of magnitude 2qa2qa directed along the axis from −q-q to +q+q. SI unit C m.
  • The total charge of a dipole is zero, but its field is not zero: the fields of +q+q and −q-q do not cancel exactly because the charges sit at different places.
  • At distances much greater than 2a2a they nearly cancel, so the dipole field falls off faster than 1/r21/r^2 — in fact as 1/r31/r^3.
  • A short (or ideal, or point) dipole means r≫ar\gg a, and it is only then that the simple 1/r31/r^3 formulas hold.

Field on the axial line — the derivation CBSE sets

Let PP lie on the axis at distance rr from the centre, on the side of +q+q. Then +q+q is at distance r−ar-a and −q-q at distance r+ar+a from PP. Let p^\hat{p} be the unit vector from −q-q to +q+q.

E⃗+q=14πε0q(r−a)2 p^,E⃗−q=−14πε0q(r+a)2 p^\vec{E}_{+q} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{(r-a)^2}\,\hat{p},\qquad \vec{E}_{-q} = -\dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{(r+a)^2}\,\hat{p}

The first points away from +q+q, that is along p^\hat{p}; the second points towards −q-q, that is along −p^-\hat{p}. Adding,

E⃗axial=q4πε0[1(r−a)2−1(r+a)2]p^\vec{E}_{\text{axial}} = \dfrac{q}{4\pi\varepsilon_0}\left[\dfrac{1}{(r-a)^2}-\dfrac{1}{(r+a)^2}\right]\hat{p}

=q4πε0⋅(r+a)2−(r−a)2(r2−a2)2 p^=q4πε0⋅4ar(r2−a2)2 p^= \dfrac{q}{4\pi\varepsilon_0}\cdot\dfrac{(r+a)^2-(r-a)^2}{(r^2-a^2)^2}\,\hat{p} = \dfrac{q}{4\pi\varepsilon_0}\cdot\dfrac{4ar}{(r^2-a^2)^2}\,\hat{p}

Using p=q(2a)p = q(2a),

E⃗axial=14πε0⋅2pr(r2−a2)2 p^\vec{E}_{\text{axial}} = \dfrac{1}{4\pi\varepsilon_0}\cdot\dfrac{2pr}{(r^2-a^2)^2}\,\hat{p}

For a short dipole, r≫ar\gg a, so a2a^2 may be neglected against r2r^2 and (r2−a2)2→r4(r^2-a^2)^2\to r^4:

E⃗axial=14πε02p⃗r3\vec{E}_{\text{axial}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{2\vec{p}}{r^3}

directed along p⃗\vec{p}. Writing it with xx in place of rr changes nothing.

Field on the equatorial line — the derivation CBSE sets

Let PP lie on the perpendicular bisector at distance rr from the centre. Each charge is at distance r2+a2\sqrt{r^2+a^2} from PP, so the two fields have equal magnitudes

E+q=E−q=14πε0q(r2+a2)E_{+q} = E_{-q} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{(r^2+a^2)}

Draw them at PP: the field of +q+q points away from +q+q, the field of −q-q points towards −q-q. Resolve each along and perpendicular to the dipole axis.

  • The components perpendicular to the axis are equal and opposite, so they cancel.
  • The components parallel to the axis are equal and both point from +q+q towards −q-q, that is along −p^-\hat{p}, so they add.

Enet=2E+qcos⁡θ,cos⁡θ=a(r2+a2)1/2E_{\text{net}} = 2E_{+q}\cos\theta,\qquad \cos\theta = \dfrac{a}{(r^2+a^2)^{1/2}}

Enet=2⋅14πε0q(r2+a2)⋅a(r2+a2)1/2=14πε0q (2a)(r2+a2)3/2=14πε0p(r2+a2)3/2E_{\text{net}} = 2\cdot\dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{(r^2+a^2)}\cdot\dfrac{a}{(r^2+a^2)^{1/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q\,(2a)}{(r^2+a^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}}

directed antiparallel to p⃗\vec{p}. For a short dipole, r≫ar\gg a:

E⃗equatorial=−14πε0p⃗r3\vec{E}_{\text{equatorial}} = -\dfrac{1}{4\pi\varepsilon_0}\dfrac{\vec{p}}{r^3}

The minus sign is worth a mark on its own: the equatorial field is opposite in direction to the dipole moment.

The diagram in words

  • Axial case: draw the dipole horizontally, −q-q on the left, +q+q on the right, separation 2a2a, centre OO, and p⃗\vec{p} as an arrow from −q-q to +q+q. Mark PP on the axis to the right of +q+q at distance rr from OO. At PP draw a long arrow to the right for E⃗+q\vec{E}_{+q} and a shorter one to the left for E⃗−q\vec{E}_{-q}.
  • Equatorial case: same dipole, with PP on the perpendicular through OO at distance rr. At PP draw E⃗+q\vec{E}_{+q} pointing directly away from +q+q and E⃗−q\vec{E}_{-q} pointing directly towards −q-q, both making angle θ\theta with the line OPOP produced. Mark their resolved components and show the perpendicular pair cancelling.

Standard results

ResultExpression
Dipole momentp=q×2ap = q\times 2a, from −q-q to +q+q
Axial field, exact14πε02pr(r2−a2)2\dfrac{1}{4\pi\varepsilon_0}\dfrac{2pr}{(r^2-a^2)^2}, along p⃗\vec{p}
Axial field, short dipole14πε02pr3\dfrac{1}{4\pi\varepsilon_0}\dfrac{2p}{r^3}
Equatorial field, exact14πε0p(r2+a2)3/2\dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}}, opposite to p⃗\vec{p}
Equatorial field, short dipole14πε0pr3\dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}
Ratio at equal distanceEaxial=2EequatorialE_{\text{axial}} = 2E_{\text{equatorial}}
  • The dipole field at large distances depends on qq and aa only through their product qaqa — which is why the dipole moment is the natural quantity to define.
  • The dipole field falls as 1/r31/r^3, in contrast to the 1/r21/r^2 of a point charge, and its magnitude and direction depend on the angle between r⃗\vec{r} and p⃗\vec{p} as well as on rr.
  • Torque and potential energy of a dipole, τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E} and U=−p⃗⋅E⃗U = -\vec{p}\cdot\vec{E}, are also examined under this heading: torque is maximum when p⃗\vec{p} is perpendicular to E⃗\vec{E}, and the potential energy in stable equilibrium is −pE=−qLE-pE = -qLE for a dipole of charge separation LL.

Theory Questions Asked on This Subtopic

Real board questions. Answers are at the end of the page.

  1. 1

    Torque acting on an electric dipole placed in an electric field is maximum when the angle between the electric field and the dipole moment is ______.

    1 markCBSE Class 12 Physics — Very Short Answer · 2020 · Section A, 1 markAnswer 1 ↓
  2. 2

    Obtain the expression for the electric field at a point on the equatorial line of an electric dipole.

    2 marksCBSE Class 12 Physics — SA · 2019C · Section B, 2 marksAnswer 2 ↓
  3. 3

    Derive an expression for the electric field due to a dipole of dipole moment p⃗\vec{p} at a point on its perpendicular bisector (equatorial line).

    3 marksCBSE Class 12 Physics — SA · 2/3, Delhi 2019, 2017 · Section C, 3 marksAnswer 3 ↓

Numericals

Every numerical set on this subtopic. Full working is at the end of the page.

  1. 4

    An electric dipole consisting of charges +q+q and −q-q separated by a distance LL is in stable equilibrium in a uniform electric field E⃗\vec{E}. The electrostatic potential energy of the dipole is

    • (a)

      qLEqLE

    • (b)

      zero

    • (c)

      −qLE-qLE

    • (d)

      −2qEL-2qEL

    1 markCBSE Class 12 Physics — Multiple Choice · 2020 · Section A, 1 markAnswer 4 ↓

Answers & Solutions

Work the questions above first, then check yourself here. Each answer is set out the way it should be written in the paper.

  1. τ⃗=p⃗×E⃗\vec{\tau} = \vec{p}\times\vec{E}, so τ=pEsin⁡θ\tau = pE\sin\theta, which is maximum when θ=90°\theta = 90° (the angle between the electric field and the dipole moment).

  2. The strength of an electric dipole is measured by its dipole moment, p⃗=q(2a)\vec{p} = q(2a), directed from the negative to the positive charge along the line joining them (2a2a = separation). Consider a point PP on the perpendicular bisector (equatorial line), at distance rr from the centre. The fields EPAE_{PA} (due to −q-q) and EPBE_{PB} (due to +q+q) are equal in magnitude (EPA=EPB=14πε0qr2+a2E_{PA}=E_{PB}=\dfrac{1}{4\pi\varepsilon_0}\dfrac{q}{r^2+a^2}); their components perpendicular to p⃗\vec{p} cancel, and the components along −p⃗-\vec{p} add: Enet=2EPAcos⁡θE_{net} = 2E_{PA}\cos\theta, where cos⁡θ=a(r2+a2)1/2\cos\theta = \dfrac{a}{(r^2+a^2)^{1/2}} Enet=14πε0q⋅2a(r2+a2)3/2=14πε0p(r2+a2)3/2E_{net} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q\cdot2a}{(r^2+a^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}} directed antiparallel to p⃗\vec{p}. For a short dipole (r≫ar \gg a): E=14πε0pr3E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}, or in vector form, E⃗=14πε0−p⃗r3\vec{E} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{-\vec{p}}{r^3}

  3. (Same derivation as Q26.) Electric field on the equatorial line at any point on the perpendicular bisector of the dipole, at distance rr from its centre: Enet=EPAcos⁡θ+EPBcos⁡θ=2EPAcos⁡θE_{net} = E_{PA}\cos\theta+E_{PB}\cos\theta = 2E_{PA}\cos\theta (EPA=EPBE_{PA}=E_{PB}, vertical components cancel) Enet=14πε0q⋅2a(r2+a2)3/2=14πε0p(r2+a2)3/2E_{net} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{q\cdot2a}{(r^2+a^2)^{3/2}} = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{(r^2+a^2)^{3/2}} directed antiparallel to p⃗\vec{p}. For a short dipole (r≫a)(r \gg a): E=14πε0pr3E = \dfrac{1}{4\pi\varepsilon_0}\dfrac{p}{r^3}

  4. For stable equilibrium, θ=0°\theta = 0° (dipole moment parallel to field). Potential energy, U=−p⃗⋅E⃗=−pEcos⁡0°=−pE=−(qL)E=−qLEU = -\vec{p}\cdot\vec{E} = -pE\cos0° = -pE = -(qL)E = -qLE (since p=qLp = qL).