What is the value of:
∫∞−∞x2δ(x−2)dx
A point charge (q) is located at position R, as shown. What is ρ(r), the charge density in all space?
An electric dipole (+q and –q, small distance d apart) sits centered in a Gaussian sphere.
What can you say about the flux of \mathbf{E} through the sphere, and |\mathbf{E}| on the sphere?
Which of the following two fields has zero curl?
I | II |
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Can superposition be applied to electric potential, V?
V_{tot} \stackrel{?}{=} \sum_i V_i = V_1 +V_2 + V_3 + \dots
Could this be a plot of \left|\mathbf{E}(r)\right|? Or V(r)? (for SOME physical situation?)
A point charge +q sits outside a solid neutral conducting copper sphere of radius A. The charge q is a distance r > A from the center, on the right side. What is the E-field at the center of the sphere? (Assume equilibrium situation).
A neutral copper sphere has a spherical hollow in the center. A charge +q is placed in the center of the hollow. What is the total charge on the outside surface of the copper sphere? (Assume Electrostatic equilibrium.)
True or False: The electric field, \mathbf{E(\mathbf{r})}, in some region of space is zero, thus the electric potential, V(\mathbf{r}), in that same region of space is zero.
True or False: The electric potential, V(\mathbf{r}), in some region of space is zero, thus the electric field, \mathbf{E(\mathbf{r})}, in that same region of space is zero.
The general solution for the electric potential in spherical coordinates with azimuthal symmetry (no \phi dependence) is:
V(r,\theta) = \sum_{l=0}^{\infty} \left(A_l r^l + \dfrac{B_l}{r^{l+1}}\right)P_l(\cos \theta)
Consider a metal sphere (constant potential in and on the sphere, remember). Which terms in the sum vanish outside the sphere? (Recall: V \rightarrow 0 as r \rightarrow \infty)
\mathbf{p} = \sum_i q_i \mathbf{r}_i
What is the dipole moment of this system?
(BTW, it is NOT overall neutral!)
You have a physical dipole, +q and -q a finite distance d apart. When can you use the expression:
V(\mathbf{r}) = \dfrac{1}{4 \pi \varepsilon_0}\dfrac{\mathbf{p}\cdot \hat{\mathbf{r}}}{r^2}