Chapter 2: Q37P (page 97)
Find the interaction energy
for two point
charges and a distance aapart.
Short Answer
The interaction energy is
Chapter 2: Q37P (page 97)
Find the interaction energy
for two point
charges and a distance aapart.
The interaction energy is
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We know that the charge on a conductor goes to the surface, but just
how it distributes itself there is not easy to determine. One famous example in which the surface charge density can be calculated explicitly is the ellipsoid:
In this case15
(2.57) where Q is the total charge. By choosing appropriate values for a , b and c. obtain (from Eq. 2.57):
(a) the net (both sides) surface charge density a(r) on a circular disk of radius R; (b) the net surface charge density a(x) on an infinite conducting "ribbon" in the xy plane, which straddles they axis from x = - a to x = a (let A be the total charge per unit length of ribbon);
(c) the net charge per unit length on a conducting "needle," running from x = - a to x = a. In each case, sketch the graph of your result.
(a) A point chargeis inside a cavity in an uncharged conductor (Fig. 2.45). Is the force on necessarily zero?
(b) Is the force between a point charge and a nearby uncharged conductor always
attractive?
Use Eq. 2.29 to calculate the potential inside a uniformly charged
solid sphere of radiusRand total charge q.Compare your answer to Pro b. 2.21.
Use Gauss's law to find the electric field inside and outside a spherical shell of radius Rthat carries a uniform surface charge densityCompare your answer to Prob. 2.7.
All of electrostatics follows from the character of Coulomb's law, together with the principle of superposition. An analogous theory can therefore be constructed for Newton's law of universal gravitation. What is the gravitational energy of a sphere, of mass M and radius R,assuming the density is uniform? Use your result to estimate the gravitational energy of the sun (look up the relevant numbers). Note that the energy is negative-masses attract,whereas (like) electric charges repel.As the matter "falls in," to create the sun, its energy is converted into other forms (typically thermal), and it is subsequently released in the form of radiation. The sun radiates at a rate of ; if all this came from gravitational energy, how long would the sun last? [The sun is in fact much older than that, so evidently this is notthe source of its power.]
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