Spherical multipole moments explained
In physics, spherical multipole moments are the coefficients in a series expansion of a potential that varies inversely with the distance to a source, i.e., as Examples of such potentials are the electric potential, the magnetic potential and the gravitational potential.
Through this article, the primed coordinates such as
refer to the position of charge(s), whereas the unprimed coordinates such as
refer to the point at which the potential is being observed. We also use
spherical coordinates throughout, e.g., the vector
has coordinates
where
is the radius,
is the
colatitude and
is the
azimuthal angle.
Spherical multipole moments of a point charge
The electric potential due to a point charge located at
is given by
where
}\ \left|\mathbf - \mathbf \right| is the distance between the charge position and the observation point and
is the angle between the vectors
and
. If the radius
of the observation point is
greater than the radius
of the charge, we may factor out 1/
r and expand the square root in powers of
using
Legendre polynomialsThis is exactly analogous to the
axial multipole expansion.
We may express
in terms of the coordinates of the observation point and charge position using the
spherical law of cosines (Fig. 2)
Substituting this equation for
into the
Legendre polynomials and factoring the primed and unprimed coordinates yields the important formula known as the spherical harmonic addition theorem
where the
functions are the
spherical harmonics. Substitution of this formula into the potential yields
which can be written aswhere the multipole moments are defined
As with axial multipole moments, we may also consider the case when the radius
of the observation point is
less than the radius
of the charge. In that case, we may write
which can be written as
where the interior spherical multipole moments are defined as the complex conjugate of
irregular solid harmonicsThe two cases can be subsumed in a single expression if
and
are defined to be the lesser and greater, respectively, of the two radii
and
; the potential of a point charge then takes the form, which is sometimes referred to as
Laplace expansionExterior spherical multipole moments
It is straightforward to generalize these formulae by replacing the point charge
with an infinitesimal charge element
and integrating. The functional form of the expansion is the same. In the exterior case, where
, the result is:
where the general multipole moments are defined
Note
The potential Φ(r) is real, so that the complex conjugate of the expansion is equally valid. Taking of the complex conjugate leads to a definition of the multipole moment which is proportional to Yℓm, not to its complex conjugate. This is a common convention, see molecular multipoles for more on this.
Interior spherical multipole moments
Similarly, the interior multipole expansion has the same functional form. In the interior case, where
, the result is:
with the interior multipole moments defined as
Interaction energies of spherical multipoles
A simple formula for the interaction energy of two non-overlapping but concentric charge distributions can be derived. Let the first charge distribution
be centered on the origin and lie entirely within the second charge distribution
. The interaction energy between any two static charge distributions is defined by
The potential
of the first (central) charge distribution may be expanded in exterior multipoles
where
represents the
exterior multipole moment of the first charge distribution. Substitution of this expansion yields the formula
Since the integral equals the complex conjugate of the interior multipole moments
of the second (peripheral) charge distribution, the energy formula reduces to the simple form
For example, this formula may be used to determine the electrostatic interaction energies of the atomic nucleus with its surrounding electronic orbitals. Conversely, given the interaction energies and the interior multipole moments of the electronic orbitals, one may find the exterior multipole moments (and, hence, shape) of the atomic nucleus.
Special case of axial symmetry
The spherical multipole expansion takes a simple form if the charge distribution is axially symmetric (i.e., is independent of the azimuthal angle
). By carrying out the
integrations that define
and
, it can be shown the multipole moments are all zero except when
. Using the mathematical identity
the exterior multipole expansion becomes
where the axially symmetric multipole moments are defined
In the limit that the charge is confined to the
-axis, we recover the exterior
axial multipole moments.
Similarly the interior multipole expansion becomeswhere the axially symmetric interior multipole moments are definedIn the limit that the charge is confined to the
-axis, we recover the interior
axial multipole moments.
See also
Notes and References
- Book: Jackson, John David . Classical electrodynamics . 1999 . Wiley . 978-0-471-30932-1 . New York.