Spherical multipole moments
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In physics, spherical multipole moments are the coefficients in a series expansion of a potential that varies inversely with the distance R to a source, i.e., as <math>\tfrac 1 R.</math> Examples of such potentials are the electric potential, the magnetic potential and the gravitational potential.
For clarity, we illustrate the expansion for a point charge, then generalize to an arbitrary charge density <math>\rho(\mathbf r').</math> Through this article, the primed coordinates such as <math>\mathbf r'</math> refer to the position of charge(s), whereas the unprimed coordinates such as <math>\mathbf{r}</math> refer to the point at which the potential is being observed. We also use spherical coordinates throughout, e.g., the vector <math>\mathbf r'</math> has coordinates <math>( r', \theta', \phi')</math> where <math>r'</math> is the radius, <math>\theta'</math> is the colatitude and <math>\phi'</math> is the azimuthal angle.
Spherical multipole moments of a point charge
The electric potential due to a point charge located at <math>\mathbf{r'}</math> is given by
<math display="block"> \Phi(\mathbf{r}) = \frac{q}{4\pi\varepsilon} \frac{1}{R} = \frac{q}{4\pi\varepsilon} \frac{1}{\sqrt{r^2 + r^{\prime 2} - 2 r' r \cos \gamma}}. </math> where <math>R \ \stackrel{\mathrm{def}}{=}\ \left|\mathbf{r} - \mathbf{r'} \right|</math> is the distance between the charge position and the observation point and <math>\gamma</math> is the angle between the vectors <math>\mathbf{r}</math> and <math>\mathbf{r'}</math>. If the radius <math>r</math> of the observation point is greater than the radius <math>r'</math> of the charge, we may factor out 1/r and expand the square root in powers of <math>(r'/r)<1</math> using Legendre polynomials
<math display="block">\Phi(\mathbf{r}) = \frac{q}{4\pi\varepsilon r} \sum_{\ell=0}^{\infty} \left( \frac{r'}{r} \right)^\ell P_\ell(\cos \gamma )</math>
This is exactly analogous to the axial multipole expansion.
We may express <math>\cos \gamma</math> in terms of the coordinates of the observation point and charge position using the spherical law of cosines (Fig. 2) <math display="block">\cos \gamma = \cos \theta \cos \theta' + \sin \theta \sin \theta' \cos(\phi - \phi')</math>
Substituting this equation for <math>\cos \gamma</math> into the Legendre polynomials and factoring the primed and unprimed coordinates yields the important formula known as the spherical harmonic addition theorem <math display="block"> P_\ell(\cos \gamma) = \frac{4\pi}{2\ell + 1} \sum_{m=-\ell}^\ell Y_{\ell m}(\theta, \phi) Y_{\ell m}^{*}(\theta', \phi') </math> where the <math>Y_{\ell m}</math> functions are the spherical harmonics. Substitution of this formula into the potential yields <math display="block"> \Phi(\mathbf{r}) = \frac{q}{4\pi\varepsilon r} \sum_{\ell=0}^{\infty} \left( \frac{r'}{r} \right)^\ell \left( \frac{4\pi}{2\ell+1} \right) \sum_{m=-\ell}^\ell Y_{\ell m}(\theta, \phi) Y_{\ell m}^{*}(\theta', \phi') </math>
which can be written as <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell \left( \frac{Q_{\ell m}}{r^{\ell+1}} \right) \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}(\theta, \phi) </math> where the multipole moments are defined <math display="block">Q_{\ell m} \ \stackrel{\mathrm{def}}{=}\ q \left( r' \right)^\ell \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}^{*}(\theta', \phi').</math>
As with axial multipole moments, we may also consider the case when the radius <math>r</math> of the observation point is less than the radius <math>r'</math> of the charge. In that case, we may write <math display="block"> \Phi(\mathbf{r}) = \frac{q}{4\pi\varepsilon r'} \sum_{\ell=0}^{\infty} \left( \frac{r}{r'} \right)^\ell \left( \frac{4\pi}{2\ell+1} \right) \sum_{m=-\ell}^\ell Y_{\ell m}(\theta, \phi) Y_{\ell m}^{*}(\theta', \phi') </math> which can be written as <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell I_{\ell m} r^\ell \sqrt{\frac{4\pi }{2\ell+1}} Y_{\ell m}(\theta, \phi) </math> where the interior spherical multipole moments are defined as the complex conjugate of irregular solid harmonics <math display="block"> I_{\ell m} \ \stackrel{\mathrm{def}}{=}\ \frac{q}{\left( r' \right)^{\ell+1}} \sqrt{\frac{4\pi }{2\ell+1}} Y_{\ell m}^{*}(\theta', \phi') </math>
The two cases can be subsumed in a single expression if <math>r_<</math> and <math>r_></math> are defined to be the lesser and greater, respectively, of the two radii <math>r</math> and <math>r'</math>; the potential of a point charge then takes the form, which is sometimes referred to as Laplace expansion <math display="block"> \Phi(\mathbf{r}) = \frac{q}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \frac{r_<^\ell}{r_>^{\ell+1}} \left( \frac{4\pi}{2\ell+1} \right) \sum_{m=-\ell}^\ell Y_{\ell m}(\theta, \phi) Y_{\ell m}^{*}(\theta', \phi') </math>
Exterior spherical multipole moments
It is straightforward to generalize these formulae by replacing the point charge <math>q</math> with an infinitesimal charge element <math>\rho(\mathbf{r}') d\mathbf{r}'</math> and integrating. The functional form of the expansion is the same. In the exterior case, where <math>r>r'</math>, the result is: <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell \left( \frac{Q_{\ell m}}{r^{\ell+1}} \right) \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}(\theta, \phi)\,, </math> where the general multipole moments are defined <math display="block"> Q_{\ell m} \ \stackrel{\mathrm{def}}{=}\ \int d\mathbf{r}' \rho(\mathbf{r}') \left( r' \right)^\ell \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}^{*}(\theta', \phi'). </math>
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 <math>r' > r</math>, the result is: <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell I_{\ell m} r^\ell \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}(\theta, \phi) , </math> with the interior multipole moments defined as <math display="block"> I_{\ell m} \ \stackrel{\mathrm{def}}{=}\ \int d\mathbf{r}' \frac{\rho(\mathbf{r}')}{\left( r' \right)^{\ell+1}} \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}^{*}(\theta', \phi'). </math>
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 <math>\rho_1(\mathbf{r}')</math> be centered on the origin and lie entirely within the second charge distribution <math>\rho_2(\mathbf{r}')</math>. The interaction energy between any two static charge distributions is defined by <math display="block"> U \ \stackrel{\mathrm{def}}{=}\ \int d\mathbf{r} \rho_2(\mathbf{r}) \Phi_1(\mathbf{r}). </math>
The potential <math>\Phi_1(\mathbf{r})</math> of the first (central) charge distribution may be expanded in exterior multipoles <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell Q_{1\ell m} \left( \frac{1}{r^{\ell+1}} \right) \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}(\theta, \phi) </math> where <math>Q_{1\ell m}</math> represents the <math>\ell m</math> exterior multipole moment of the first charge distribution. Substitution of this expansion yields the formula <math display="block"> U = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell Q_{1\ell m} \int d\mathbf{r} \ \rho_2(\mathbf{r}) \left( \frac{1}{r^{\ell+1}} \right) \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell m}(\theta, \phi) </math>
Since the integral equals the complex conjugate of the interior multipole moments <math>I_{2\ell m}</math> of the second (peripheral) charge distribution, the energy formula reduces to the simple form <math display="block">U = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \sum_{m=-\ell}^\ell Q_{1\ell m} I_{2\ell m}^{*}</math>
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 <math>\phi'</math>). By carrying out the <math>\phi'</math> integrations that define <math>Q_{\ell m}</math> and <math>I_{\ell m}</math>, it can be shown the multipole moments are all zero except when <math>m=0</math>. Using the mathematical identity <math display="block">P_\ell(\cos \theta) \ \stackrel{\mathrm{def}}{=}\ \sqrt{\frac{4\pi}{2\ell+1}} Y_{\ell 0}(\theta, \phi)</math> the exterior multipole expansion becomes <math display="block"> \Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} \left( \frac{Q_\ell}{r^{\ell+1}} \right) P_\ell(\cos \theta) </math> where the axially symmetric multipole moments are defined <math display="block">Q_\ell \ \stackrel{\mathrm{def}}{=}\ \int d\mathbf{r}' \rho(\mathbf{r}') \left( r' \right)^\ell P_\ell(\cos \theta')</math> In the limit that the charge is confined to the <math>z</math>-axis, we recover the exterior axial multipole moments.
Similarly the interior multipole expansion becomes <math display="block">\Phi(\mathbf{r}) = \frac{1}{4\pi\varepsilon} \sum_{\ell=0}^{\infty} I_\ell r^\ell P_\ell(\cos \theta)</math> where the axially symmetric interior multipole moments are defined <math display="block">I_\ell \ \stackrel{\mathrm{def}}{=}\ \int d\mathbf{r}' \frac{\rho(\mathbf{r}')}{\left( r' \right)^{\ell+1}} P_\ell(\cos \theta')</math> In the limit that the charge is confined to the <math>z</math>-axis, we recover the interior axial multipole moments.
