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A solution to pledged problem 3 from physics 102, which involves applying gauss' law to determine the electric fields at various points in space due to two spherical charged bodies with non-uniform and uniform charge distributions, respectively. The problem also requires calculating the charge densities on the inner and outer faces of the conducting shell surrounding the first charged body.
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Time allowed: 2 hours at a single sitting
DUE 4PM MONDAY, February 4, 2008, in the boxes marked Phys 101-102 in the physics lounge. You may use your own textbook, your notes, and a non-programmed calculator. You may also consult the on-line solutions to the corresponding suggested problems. You should consult no other help. Show how you arrived at your answer; the correct answer by itself may not be sufficient.
Further instructions:
(a) Write legibly on one side of 8.5” x 11” white or lightly tinted paper. (b) Staple all sheets together, including this one, in the upper left corner and make one vertical fold. (c) On the outside, staple side up. Print your name in capital letters, your LAST NAME first followed by your FIRST NAME. (d) Below your name, print the phrase “Pledged Problem 3”, followed by the due date. (e) Also indicate start time and end time. (f) Write and sign the pledge, with the understanding you may consult the materials noted above.
a) Use Gauss’ Law to determine the electric field at all points in space. Indicate the Gaussian surfaces used.
b) Show on a carefully labeled figure the radial dependence of the electric field.
c) What are the charge densities, σb and σc , on the inner and outer faces of the conductor?
radial symmetry (the charge densities for both the cloud and conducting shell depend only on r, the radial distance from the center), then one will use Gaussian surfaces having the same symmetry, namely concentric spheres of varying r. Applying Gauss’ Law first to a sphere inside the cloud, with radius r < a, one gets
ܧ රሬԦ^ ܣd ·Ԧ ൌ ܳ ߳
න ρሺrሻ4πr ᇱଶ^ dr ᇱ
୰
r ᇱଶ^
4πr ᇱଶ^ dr ᇱ
୰
߳4πA
න dr ᇱ
୰
4πAr߳
Again, symmetry indicates that on the Gaussian surface, the electric field, ܧሬԦ, will be constant
and parallel to ݀ Ԧ ܣ^ and so can be removed from the surface integration. The surface area is simply 4πr 2 , so that, for , ܽ൏ ݎ
For ܽ ܾ൏ ݎ , the charge enclosed will be the total charge in the inner cloud, or ܳ ܽܣߨ4 ൌ , and so Gauss’ Law indicates that
ܧ රሬԦ^ ܣd ·Ԧ ൌ E4πr ଶ^ ܳ ൌ ߳
and, therefore,
Within the conducting shell, for ܾ ܿ ݎ , sufficient charge will accumulate on the inner radius (equal in magnitude to the total charge in the cloud but of opposite sign), so that the field inside the conductor will be zero,
ܧሬԦ^ ൌ 0 ሺ ܾ ݎܿ ሻ
Outside the conducting shell, for ܿ ݎ ൏ ,
ܧ රሬԦ^ ܣd ·Ԧ ൌ E4πr ଶ^ ܳ ൌ ߳
and, therefore,
Superposition of electric fields. The key to solving the problem is to recognize that the net charge density shown in the figure can be treated as associated with two spherical clouds of uniform charge. The first, having a uniform charge density of ρ and radius a, is centered at the origin; the second, having a uniform charge density of -ρ and radius a/2, is centered at x = a/2. (When the charged densities in the cavity are added, they produce a net charge density of 0 in that volume).
The electric field associated with either charge distribution at a given distance from the center can be determined by using Gauss’ Law or can be recalled from the example in the book. It is directed radially from the center and equals Qtot/4πߝr 2 , where Qtot is the total charge in the cloud and r is measured from the center of the sphere (the same electric field obtained by considering the entire charge to be located at the center of the cloud).
The electric field at P a ssociated withthe charge density in the large cloud will then simply be
௧௧ ߝߨ4 ݎ ଶ^
The electric field at P associated with thecharge density in the smaller cloud will be
The total field will be the sum of the e ields –s f