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Electromagnetism}Small Oscillations


The potential is determined in the previous problem to be V=\frac{Q}{4\pi \epsilon_0 \sqrt{R^2+x^2}}. The field is given by \vec{E}=-\nabla V. Before taking derivatives, one can simplify the potential since it is given that R >> x.

Binomial expand it ((1+y)^n\approx 1+ny, for y small) to get


Taking the derivative, using the equations \vec{E}=-\nabla V, and \vec{F}=q\vec{E}, one gets,


Small oscillations have the same form as simple harmonic oscillations, i.e., \ddot{x} = -\omega^2 x. The angular frequency is \omega=\sqrt{q\frac{Q}{4\pi \epsilon_0 R^3 m}}, as in choice (A).


See below for user comments and alternate solutions! See below for user comments and alternate solutions!
Alternate Solutions
chri5tina
2006-11-27 05:11:24
It is possible to do this problem w/o the binomial expansion.

Take F = -k*x, plug in -dV/dx for F and solve for k.

Plug k into w = (k/m)^1/2 and you'll have an expression with (R^2 + x^2)^3/2 in the denominator.

At this point you can remember that R >> x and simply cancel out x as negligible, which leaves R^3 in the denominator and the correct solution.
Alternate Solution - Unverified
Comments
Muphrid
2009-10-08 14:06:53
It may be faster to keep working with electrical potential to find the spring constant. Simple harmonic oscillators satisfy F(x) = -kx, as has been said, but they also satisfy

U(x) \approx U_0 + \frac{1}{2} k x^2

and have angular frequency

\omega = \sqrt{\frac{k}{m}}

It's important to remember that what you know from problem (3) is V(x), potential energy per unit charge, not U(x), which is real potential energy. This is what alleviates the sign confusion later on.

As in the base solution, you can binomial expand V(x) and approximate it as

V(x) = \frac{Q}{4\pi \epsilon_0} \frac{1}{R} \left( 1 - \frac{1}{2} \frac{x^2}{R^2} \right)

Note that the 1 can be dropped; this just gives a constant overall potential that we're not interested in. This leaves us with

V(x) = V_0 - \frac{1}{2} \frac{Q x^2}{4 \pi \epsilon_0 R^3}

And now multiply through by -q, the charge of the test charge, to get real potential energy:

U(x) = -q V_0 + \frac{1}{2} \frac{qQ x^2}{4 \pi \epsilon_0 R^3}

Recognize this as a simple harmonic potential, where

\frac{1}{2} k x^2 = \frac{1}{2} \frac{qQ x^2}{4 \pi \epsilon_0 R^3} \rightarrow k = \frac{qQ}{4 \pi \epsilon_0 R^3}

And thus

\omega = \sqrt{\frac{k}{m}} = \sqrt{\frac{qQ}{4 \pi \epsilon_0 m R^3}}
NEC
tinytoon
2008-11-07 14:48:10
Also, you could derive the electric field from first principles to get the answer (although very inefficient). This is, nonetheless, a valid alternative:

E = \int \frac{dq}{4\pi\epsilon_0 r^2}

We only care about the horizontal component because the force in the vertical component is zero:


E = \int \frac{dqcos\theta}{4\pi\epsilon_0 r^2}.

Using cos\theta = \frac{x}{r} = \frac{x}{\sqrt{x^2+R^2}} and r^2 = x^2+R^2, we get:

E = \frac{qx}{4\pi\epsilon_0 (x^2+R^2)^{3/2}}

and

F = \frac{qQx}{4\pi\epsilon_0 (x^2+R^2)^{3/2}} =kx

We can clearly see now that:

k = \frac{qQ}{4\pi\epsilon_0 (x^2+R^2)^{3/2}}.

We know that:

\omega = \sqrt{k/m} = \sqrt{\frac{qQ}{4\pi\epsilon_0 (x^2+R^2)^{3/2}m}}

In the limit that R>>x , this reduces to:

\omega = \sqrt{k/m} = \sqrt{\frac{qQ}{4\pi\epsilon_0 R^3m}}.

NEC
gn0m0n
2008-10-19 17:49:35
What are we expanding, exactly?NEC
dcan
2008-04-09 16:32:33
Can someone tell me why it doesn't work to use conservation of energy? Supposedly the potential energy is qV, but when I solve for \omega I'm off by a factor of 1/\sqrt{2}. NEC
Gaffer
2007-10-26 14:12:55
This problem has some particularly generous writers.

For small oscillations, I believe it is safe to say \omega must be a constant, that is not dependent upon x. This knocks off BDE. Then all you need to remember is that \omega will most likely involve a square root due to the diffEQ yosun mentioned and you have choice A, no dimensional analysis or calculation necessary.

Though of course it is always better to know why a particular formula is correct, sometimes quick and dirty is the way to go.

Oh that they were all this easy!
jmason86
2009-09-29 16:40:35
This is exactly how I did the problem too. Definitely the right strategy under time pressure.
NEC
rmyers
2006-11-29 16:16:57
This can also be done just by dimensional analysis. Qq/(4pi(e0)R^2) has units of force = kg * m/s^2 and angular frequency is just 1/s. Only A & B are possible answers after this. From there I suppose you can just use the idea that the angular frequency usually doesn't depend on initial displacement in cases like these.
eliasds
2008-08-18 00:58:43
I believe that choice E has the same dimensions as A&B.
eliasds
2008-08-18 01:43:44
I believe that choice E has the same dimensions as A&B.
wangjj0120
2008-10-11 01:12:02
rmyers:
your comment "you can just use the idea that the angular frequency usually doesn't depend on initial displacement" is not always true. You can find the x dependence from the exact solution.
NEC
chri5tina
2006-11-27 05:11:24
It is possible to do this problem w/o the binomial expansion.

Take F = -k*x, plug in -dV/dx for F and solve for k.

Plug k into w = (k/m)^1/2 and you'll have an expression with (R^2 + x^2)^3/2 in the denominator.

At this point you can remember that R >> x and simply cancel out x as negligible, which leaves R^3 in the denominator and the correct solution.
Alternate Solution - Unverified
stiner905
2006-10-29 12:26:06
After the binomial expansion, the potential should have a "-" instead of a "+" in the expansion term. However, a minus exists in the force equation because the test charge has charge -q.NEC

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This problem has some particularly generous writers. For small oscillations, I believe it is safe to say \omega must be a constant, that is not dependent upon x. This knocks off BDE. Then all you need to remember is that \omega will most likely involve a square root due to the diffEQ yosun mentioned and you have choice A, no dimensional analysis or calculation necessary. Though of course it is always better to know why a particular formula is correct, sometimes quick and dirty is the way to go. Oh that they were all this easy!

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