The multipole expansion is a powerful mathematical technique used to approximate the electrostatic potential V(r) due to a localized charge distribution ρ(r′) when the observation point lies far from the source region. In such cases, when ∣r∣≫∣r′∣, it is possible to expand the potential in a series of inverse powers of r. Each term in this expansion corresponds to a distinct multipole moment of the charge distribution, capturing increasingly fine details of its spatial structure.
This approach is invaluable in both classical and astrophysical electrodynamics. It allows us to:
Truncate the potential at low-order terms when higher-order structure is negligible (e.g., monopole or dipole approximations),
Classify field behavior by symmetry and falloff rate (∝1/rℓ+1 for the ℓ-th multipole),
Connect physical intuition about charge distributions to analytic representations of fields.
Physically, the first few terms have clear interpretations:
The monopole term reflects the total charge.
The dipole term accounts for the net separation of positive and negative charge.
The quadrupole and higher-order terms describe finer angular structure in the distribution.
The multipole expansion is especially effective when solving boundary value problems, analyzing radiation fields at large distances, or evaluating the asymptotic behavior of potentials in astrophysical and molecular systems.
Recall the potential at point P due to a charge distribution ρ(r′) is given by the integral form of Coulomb's law:
V(r)=4πϵ01∫∣r−r′∣ρ(r′)dτ′,
where dτ′ is the volume element at the source point r′, and where r is the distance between the origin of our coordinate system and point P as shown in the diagram.
where θ′ is the angle between the vectors r′ and r.
This can now be simplified further by writing it as
∣r−r′∣=r1+ϵ,
with
ϵ=(rr′)2−2(rr′)cos(θ′).
In this form, it becomes obvious that if r≫r′ (we are looking at points far away from the source charges), than ϵ≪1, thus warranting a binomial expansion:
Multipole moments are a sequence of scalar, vector, and tensor quantities that encode increasingly fine details of a charge distribution's spatial structure. In the context of the multipole expansion of the potential,
V(r)=4πϵ01ℓ=0∑∞rℓ+11∫r′ℓPℓ(cosθ′)ρ(r′)dτ′,
each term is associated with a distinct multipole moment. These moments, monopole, dipole, quadrupole, and higher, determine the angular and radial behavior of the potential and field far from the source.
Octupole moment (rank-3 tensor): ∫xi′xj′xk′ρ(r′)dτ′
Hexadecapole moment (rank-4 tensor), etc.
In general, the ℓ-th multipole moment is a rank-ℓ Cartesian tensor constructed from integrals of ρ(r′) times r′ir′j…r′ℓ. These contributions fall off as 1/rℓ+1.
Multipole moments provide a systematic way to approximate the fields of complex charge distributions. They offer deep physical insight into the structure and symmetries of the source and are widely used in electrostatics, astrophysics, quantum chemistry, and gravitational theory. In many cases, only the first few moments are needed to describe the system to high accuracy in the far field.