The Setup
A Disc with a Gradient
Imagine a flat, circular disc of radius R resting in space. If the charge were spread evenly across it, calculating the electric flux would be a walk in the park. But physics loves a good challenge! Here, the surface charge density σ isn't constant; it fades as you move outward from the center.
The density is governed by the function σ(r)=σ0(1−Rr). At the very center (r=0), the density is at its maximum, σ0. As you travel to the edge (r=R), the density drops exactly to zero.
The Master Tool
Gauss's Law
We are asked to find the ratio of electric fluxes through two different spherical surfaces. Whenever you hear "electric flux through a closed surface," your brain should immediately scream Gauss's Law.
Gauss's Law states that the total electric flux ϕ through any closed surface is directly proportional to the net charge enclosed within that surface:
This means we don't need to worry about the complex electric field vectors pointing in all directions. We just need to count the charge trapped inside our imaginary spheres!
Slicing the Disc
The Elemental Ring
Because the charge density varies with the radial distance r, we cannot simply multiply the total area by a single density value. We must use the power of calculus.
Imagine slicing the disc into infinitely many thin, concentric rings. Let's pick one such elemental ring at a distance r from the center, with an infinitesimally small thickness dr.
If we were to cut this ring and unroll it, it would look like a very long, thin rectangle. Its length is the circumference 2πr, and its width is dr. Therefore, the area of this tiny ring is:
The amount of charge dq sitting just on this ring is the area multiplied by the local charge density:
dq=σ(r)dA=σ0(1−Rr)2πrdr
Calculating the Total Flux (ϕ0)
The problem defines ϕ0 as the flux through a large spherical surface that completely encloses the disc. This means the sphere traps 100% of the disc's charge. To find this total charge, we integrate our dq expression from the center (r=0) all the way to the edge (r=R):
qtotal=∫0Rσ0(1−Rr)2πrdr
Let's pull out the constants and distribute the r:
qtotal=2πσ0∫0R(r−Rr2)dr
Integrating term by term gives:
qtotal=2πσ0[2r2−3Rr3]0R
Substituting the upper limit R:
qtotal=2πσ0(2R2−3RR3)=2πσ0(2R2−3R2)=2πσ0(6R2)
By Gauss's Law, the total flux is:
Calculating the Partial Flux (ϕ)
Now, we look at the second spherical surface. This one is concentric with the disc but only has a radius of 4R. It acts like a smaller net, only catching the charge located in the central region of the disc up to r=4R.
We use the exact same integral setup, but we change our upper limit to reflect the boundary of this new sphere:
qinner=2πσ0∫0R/4(r−Rr2)dr
qinner=2πσ0[2r2−3Rr3]0R/4
Now, we must carefully substitute r=4R:
qinner=2πσ0(2(R/4)2−3R(R/4)3)
qinner=2πσ0(2R2/16−3RR3/64)=2πσ0(32R2−192R2)
To subtract these fractions, we find a common denominator of 192:
qinner=2πσ0(1926R2−R2)=2πσ0(1925R2)
So, the flux through the smaller sphere is:
The Grand Finale
The Ratio
We have both fluxes! The final step is to find the ratio ϕϕ0. Watch how beautifully the physics constants melt away, leaving behind pure, elegant geometry:
ϕϕ0=ϵ02πσ0(1925R2)ϵ02πσ0(6R2)
Cancel out ϵ02πσ0 and R2:
ϕϕ0=5/1921/6=6×5192=30192
Dividing both the numerator and denominator by 6 gives:
And there we have it! A beautiful application of Gauss's Law and integral calculus.