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 \(a^{4} / r^{5}\).)

Short Answer

Expert verified
If so, find the leading correction to the monopole term. Answer: Yes, the quadrupole term vanishes for this system of six equal point masses. The leading correction to the monopole term is -6Gm/r.

Step by step solution

01

Compute the tensor \(Q_{ij}\) for the quadrupole moment

First, let's recall the expression for the quadrupole moment tensor: $$ Q_{ij}=m\sum_{\alpha}\left(3x_{\alpha i}x_{\alpha j}-\delta_{ij}r_{\alpha}^{2}\right), $$ where \(\alpha\) enumerates the masses, and \(x_{\alpha i}\) denotes the \(i\)-th component of the \(\alpha\)-th mass. For our given points, we can compute \(Q_{ij}\): $$ Q_{ij}=m\left[3(atot)\left(\begin{array}{ccc} 1 & 0 & 0 \\ 0 & 1 & 0 \\ 0 & 0 & 1 \end{array}\right)-\left(\begin{array}{ccc} a^{2} & 0 & 0 \\ 0 & a^{2} & 0 \\ 0 & 0 & a^{2} \end{array}\right)\right]. $$
02

Evaluate the trace of the quadrupole moment tensor

Now, we'll find the trace of the quadrupole moment tensor. The trace is the sum of the diagonal elements, denoted as \(Q_{ii}\): $$ \mathrm{Tr}(Q_{ij})=Q_{11}+Q_{22}+Q_{33}=3(atot)m-a^{2}m=0. $$ Since the trace of the quadrupole moment tensor vanishes, the quadrupole term also vanishes.
03

Find the expansion of the potential up to order \(a^{4} / r^{5}\)

We know that the monopole term of the potential is given by \(-6 \mathrm{Gm} / \mathrm{r}\). Now, we need to find the leading correction term up to order \(a^{4} / r^{5}\). We can do this by using the general expression of potential in the form of multipole expansion: $$ V(r) = -GM \left(\frac{1}{r} + \frac{Q_{ij} x_i x_j}{2 r^5} + \ldots\right). $$ Considering only terms that have an order of \(a^{4} / r^{5}\), the potential expansion becomes: $$ V(r) = -6 \frac{GM}{r} - \frac{1}{2}\frac{GQ_{ij}x_i x_j}{r^5} + \dots. $$ Since we showed in step 2 that the quadrupole term vanishes, the only term we need to consider is the monopole term: $$ V(r) = -6 \frac{GM}{r}. $$ Thus, the quadrupole term vanishes and the leading correction to the monopole term is \(-6 \mathrm{Gm} / \mathrm{r}\).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Two equal charges \(q\) are located at the points \((\pm a, 0,0)\), and two charges \(-q\) at \((0, \pm a, 0)\). Find the leading term in the potential at large distances, and the corresponding electric field.

*Show that the moment of the solar tidal force \(m \boldsymbol{g}_{\mathrm{S}}\) on an Earth satellite is $$m \boldsymbol{r} \wedge \boldsymbol{g}_{\mathrm{S}}=\frac{3 G M_{\mathrm{S}} m}{a_{\mathrm{S}}^{5}}\left(\boldsymbol{r} \cdot \boldsymbol{a}_{\mathrm{S}}\right)\left(\boldsymbol{r} \wedge \boldsymbol{a}_{\mathrm{S}}\right)$$ where \(a_{\mathrm{S}}\) is the position vector of the Sun relative to the Earth. Consider the effect on the Moon, whose orbit is inclined at \(\alpha=5^{\circ}\) to the ecliptic (the Earth's orbital plane). Introduce axes \(i\) and \(j\) in the plane of the ecliptic, with \(\boldsymbol{i}\) in the direction where the Moon's orbit crosses it. Write down the positions of the Sun and Moon, relative to Earth, as functions of time. By averaging both over a month and over a year (i.e., over the positions in their orbits of both bodies), show that the moment leads to a precession of the Moon's orbital plane, at a precessional angular velocity $$ \boldsymbol{\Omega}=-\frac{3 \varpi^{2}}{4 \omega} \cos \alpha \boldsymbol{k} $$ where \(\varpi\) is the Earth's orbital angular velocity. Compute the precessional period. (Note that this calculation is only approximately correct.)

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.

Two small identical uniform spheres of density \(\rho\) and radius \(r\) are orbiting the Earth in a circular orbit of radius \(a\). Given that the spheres are just touching, with their centres in line with the Earth's centre, and that the only force between them is gravitational, show that they will be pulled apart by the Earth's tidal force if \(a\) is less than \(a_{c}=\) \(2\left(\rho_{\mathrm{E}} / \rho\right)^{1 / 3} R_{\mathrm{E}}\), where \(\rho_{\mathrm{E}}\) is the mean density of the Earth and \(R_{\mathrm{E}}\) its radius. (This is an illustration of the existence of the Roche limit, within which small planetoids would be torn apart by tidal forces. The actual limit is larger than the one found here, because the spheres themselves would be distorted by the tidal force, thus enhancing the effect. It is \(a_{\mathrm{c}}=2.45\left(\rho_{\mathrm{E}} / \rho\right)^{1 / 3} R_{\mathrm{E}} .\) For the mean density of the Moon, for example, \(\rho=3.34 \times 10^{3} \mathrm{~kg} \mathrm{~m}^{-3}\), this gives \(\left.a_{\mathrm{c}}=2.89 R_{\mathrm{E}} \cdot\right)\)

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free