For a single point charge q at rβ², the potential at any location in space is
V(r)=kΤqβ=β£rβrβ²β£qβ
Often we are interested in an approximation of this potential at points that are far away.
Previously, the binomial expansion was used to find the electric field for point charges along an axis and only at locations on the same axis. The same approximation procedure that is used for the electric field may be used for potential. (In general, it is often easier to start with finding the scalar V and then using it to find the vector E.)
In the following, a general equation for potential at any location in space due to a point charge at any location in space is developed by considering two generalizations:
finding the potential at any location in space due to a point charge on the zβaxis and then
finding the potential at any location in space due to a point charge at any location in space.
where the β¦ terms are proportional to (d/r)3, (d/r)4, β¦. When only the term proportional to (d/r)2 is kept, the result is referred to as βV to second order in d/rβ. Equivalently, one can say that this is V to third order in 1/r (after multiplying through by 1/r, the highest power of 1/r is 1/r3) .
When both the charge and point of interest are at arbitrary locations in space, the angle between r and rβ² is no longer the spherical polar angle, ΞΈ. In this case, the angle Ξ± between r and rβ² will in general depend on both ΞΈ and Ο. From the definition of the dot product, cosΞ± is given by
To derive an expansion for this configuration, the same steps used in Generalization I can be used but with the replacement of zβ² with rβ² and ΞΈ with Ξ±. With this replacement, we have
The angleβdependent terms that are multiplied by the powers of rβ²/r are related to the Legendre polynomials. These polynomials also appear in the solution to Laplaceβs equation in spherical coordinates. Labeling these terms as P0β, P1β, β¦, and including their functional dependence on cosΞ± gives
where the first three terms are P0β=1, P1β=cosΞ±, P2β=(3cos2Ξ±β1)/2. To write these terms as Legendre poloynomials, use the definition u=cosΞ± so that P0β=1, P1β=u, and P2β=(3u2β1)/2.
where the first three terms given earlier are P0β=1, P1β=cosΞΈ, P2β=(3cos2ΞΈβ1)/2. The P3β term can be found in a table of Legendre polynomials. It is P3β=(5u3β3u)/2, so P3β=(5cos3ΞΈβ3cosΞΈ)/2. Using these,
2. Find E with spherical coordinates and unit vectors using the V(r) that you computed in part 1.
Answer
1.
V+β=rkqβ[1+rr+β²ββcosΞ±+β+β¦]
Vββ=rkqβ[1+rrββ²ββcosΞ±ββ+β¦]
In this problem, Ξ±+β, the angle between r and r+β²β is not simply the polar angle ΞΈ in spherical coordinates. It can be computed from the definition of the dot product:
cosΞ±+β=r+β²βrrβ r+β²ββ
Using r+β²β=(d/2)x^ and r=xx^+yy^β+zz^ gives
cosΞ±+β=rxβ
which can be written in spherical coordinates using x=rsinΞΈcosΟ (you should know this formula or be able to derive it from a diagram). Then,
cosΞ±+β=sinΞΈcosΟ
Checks: For ΞΈ=0 and Ο=0, this gives Ξ±+β=0 as expected. For ΞΈ=90β and Ο=0, this gives Ξ±+β=90β as expected.
Similar calculation (or using Ο=Ξ±+β+Ξ±ββ, which applies to this problem but not in general) gives
cosΞ±ββ=βsinΞΈcosΟ
Finally, using V=V+β+Vββ, we get
V=r2kqdβsinΞΈcosΟ
To compute the potential using
V(r)=kr2pβ r^β
use p=q(r+β²ββrββ²β)=qdx^ and r^=(xx^+yy^β+zz^)/r
2.
Use
V(r,ΞΈ)=r2kqdβsinΞΈcosΟ and E=ββV with β in spherical coordinates. This requires evaluation of the partials in
Checks: For Ο=0 and ΞΈ=Ο/2, expect field to be in +r^ direction. For Ο=Ο/2 and ΞΈ=Ο/2, expect +Ο^β. For Ο=Ο and ΞΈ=Ο/2, expect βr^.
Note that an alternative approach to solving both 1. and 2. problem is to take the solution for the dipole along the z axis and rotate the coordinate system around the yβaxis.
If rβ²=yβ²y^β, find an equation for V(r,ΞΈ,Ο) to second order in d/r.
Check your answer by plugging in ΞΈ=Ο/2 and Ο=Ο/2 so that r=y. For yβ«yβ², does your equation match the expected potential from approximating V(y)=kq/β£yβyβ²β£ for yβ«yβ²?