Find the quadrupole moment of a distribution of charge on the surface of a sphere of radius \(a\) with surface charge density \(\sigma=\sigma_{0}\left(\frac{3}{2} \cos ^{2} \theta-\frac{1}{2}\right)\). Find the total energy stored in this distribution.

Short Answer

Expert verified
Answer: The total energy stored in the distribution of charge due to the quadrupole moment for the given charge distribution on a sphere is 0.

Step by step solution

01

Calculate the charge distribution on the sphere's surface

To find the charge distribution on the sphere's surface, we multiply the surface charge density formula by the surface area element \(dS\) which is given by \(a^2 \sin \theta d\theta d\phi\). This gives: $$d Q = \sigma dS = \sigma_0 \left(\frac{3}{2}\cos^2\theta - \frac{1}{2}\right) a^2 \sin \theta d\theta d\phi$$
02

Compute the quadrupole moment tensor components

The components of the quadrupole moment tensor are given by the following integral: $$ Q_{lm} = \frac{1}{2}\int \rho(\vec{r}) (3x_l x_m - r^2 \delta_{lm}) d^3 r$$ In spherical coordinates, the tensor components are given by: $$ Q_{\theta\theta}=\frac{1}{2}\int dQ(3a^2 \cos^2\theta - a^2)$$ $$ Q_{\phi\phi}=\frac{1}{2}\int dQ a^2(3 \cos^2\theta \sin^2\theta - \sin^2\theta)$$ $$ Q_{\theta\phi}=\frac{1}{2}\int dQ(3a^2 \cos\theta \sin\theta \cos\phi \sin\theta \sin\phi)$$
03

Compute the quadrupole moment tensor

Now, let's compute each component of the quadrupole moment tensor. First, we calculate \(Q_{\theta \theta}\): $$ Q_{\theta\theta}=\frac{1}{2}\int_{0}^{\pi}\int_{0}^{2\pi} dQ (3a^2 \cos^2\theta - a^2) =\frac{3}{2} a^2 \sigma_0 \int_{0}^{\pi}\int_{0}^{2\pi} (\cos^2\theta\sin\theta-\frac{1}{3}\sin\theta)d\theta d\phi = 0$$ Next, let's compute \(Q_{\phi\phi}\): $$ Q_{\phi\phi}=\frac{1}{2}\int_{0}^{\pi}\int_{0}^{2\pi} dQ a^2(3 \cos^2\theta \sin^2\theta - \sin^2\theta) = a^2 \sigma_0\int_{0}^{\pi}\int_{0}^{2\pi} (\frac{3}{2}\cos^2\theta\sin^3\theta-\frac{1}{2}\sin^3\theta)d\theta d\phi = 0$$ Lastly, we compute \(Q_{\theta\phi}\): $$ Q_{\theta\phi}=\frac{1}{2}\int_{0}^{\pi}\int_{0}^{2\pi} dQ(3a^2 \cos\theta \sin\theta \cos\phi \sin\theta \sin\phi) = 0$$ Since all components of the quadrupole moment tensor are zero, the quadrupole moment is also zero.
04

The Total Energy Stored

Now that we have found the quadrupole moment tensor, we can find the total energy stored in the distribution of charge. To find the total stored energy, we can use the following formula: $$ W = \frac{1}{2}\frac{1}{4\pi\epsilon_0}\int d^3 r \rho(\vec{r}) V(\vec{r})$$ However, since the quadrupole moment tensor is zero, the potential \(V(\vec{r})\) due to the quadrupole moment is also zero. Therefore, there is no energy stored in the distribution of charge due to the quadrupole moment.$$ W = 0$$.

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Most popular questions from this chapter

Show that the work done in bringing two charges \(q_{1}\) and \(q_{2}\), initially far apart, to a separation \(r_{12}\) is \(q_{1} q_{2} / 4 \pi \epsilon_{0} r_{12}\). Write down the corresponding expression for a system of many charges. Show that the energy stored in the charge distribution is $$ V=\frac{1}{2} \sum_{j} q_{j} \phi_{j}\left(\boldsymbol{r}_{j}\right) $$ where \(\phi_{j}\left(\boldsymbol{r}_{j}\right)\) is the potential at \(\boldsymbol{r}_{j}\) due to all the other charges. Why does a factor of \(\frac{1}{2}\) appear here, but not in the corresponding expression for the potential energy in an external potential \(\phi(\boldsymbol{r}) ?\)

Find the potential and electric field at points on the axis of symmetry of a uniformly charged flat circular disc of charge \(q\) and radius \(a\). What happens to the field if we keep the charge per unit area \(\sigma=q / \pi a^{2}\) fixed, and let \(a \rightarrow \infty\) ?

The potential \(\phi(\boldsymbol{r})=\left(q / 4 \pi \epsilon_{0} r\right) \mathrm{e}^{-\mu r}\) may be regarded as representing the effect of screening of a charge \(q\) at the origin by mobile charges in a plasma. Calculate the charge density \(\rho\) (at points where \(r \neq 0\) ) and find the total charge throughout space, excluding the origin.

By considering the equilibrium of a small volume element, show that in a fluid in equilibrium under pressure and gravitational forces, \(\nabla p=\rho \boldsymbol{g}\), where \(\rho\) is the density and \(p\) the pressure (the equation of hydrostatic equilibrium). Deduce that, for an incompressible fluid of uniform density \(\rho, p+\rho \Phi\) is a constant. Use this result to obtain a rough estimate of the pressure at the centre of the Earth. (Mean density of Earth \(=5.5 \times 10^{3} \mathrm{~kg} \mathrm{~m}^{-3}\). Note that the pressure at the surface is essentially zero. The actual pressure at the centre is more than this estimate - in fact about \(3.6 \times 10^{11} \mathrm{~Pa}\) - because of the non-uniformity of \(\rho .\) It should be noted that - as indicated in Problem 12 - even very small departures from hydrostatic equilibrium would result in collapse on a short time scale, only checked by an increase in internal pressure via other processes.)

Six equal point masses \(m\) are located at the points \(\pm a \boldsymbol{i}, \pm a \boldsymbol{j}\) and \(\pm a \boldsymbol{k}\). Show that the quadrupole term in the potential vanishes, and find the leading correction to the monopole term \(-6 \mathrm{Gm} / \mathrm{r} .\) (Note: This requires expansion of the potential up to terms of order \(a^{4} / r^{5}\).)

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