Simple Harmonic Current

P P is a point at a distance of d = 1 m d= \SI[per-mode=symbol]{1}{\meter} from the center O O of an earthed conducting sphere of radius R = 0.5 m , R= \SI[per-mode=symbol]{0.5}{\meter}, and a charge of q = 2 C q= \SI[per-mode=symbol]{2}{\coulomb} is undergoing simple harmonic motion (SHM) about P P along O P . OP.

If A = 1 0 3 m A = \SI[per-mode=symbol]{10^{-3}}{\meter} is the amplitude of the oscillations, and ω = 5 rad / s \omega= \SI[per-mode=symbol]{5}{\radian\per\second} is the angular frequency of the SHM, find the maximum value of current I I (in amperes) flowing in the wire C D CD . Submit your answer to 3 decimal places.


The answer is 0.005.

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1 solution

Spandan Senapati
May 30, 2017

Relevant wiki: Conductors

Let the charge q q be at a distance x x from the center of the sphere. The sphere is earthed, thus it will exchange the charge from the Earth to keep its potential zero. Let the sphere gets a charge q q .

Now, the potential of the sphere is zero, thus k q x + k Q R = 0 \frac{kq}{x} + \frac{kQ}{R} = 0 Q = q R x . Q=- \frac{qR}{x}.

The current can be calculated by differentiating the charge with respect to time. i = d Q d t i = \frac{dQ}{dt}

Hence, the current I = q R x 2 v I= \dfrac{qR}{x^2}v .

Since A > > d , x A>>d, \, x can be treated almost constant now and current will be maximum when the speed of the particle is maximum. We know that the maximum speed of a particle in SHM is v m a x = A ω v_{max} = A \omega .

So, I m a x = q R d 2 A ω I_{max} = \dfrac{qR}{d^2} A \omega . Substituting the data in the equation we get the maximum current 0.005 A \boxed{0.005 \text{ A}}

Good did the same way.

It was asked in our 'Monday' test.

Harsh Shrivastava - 4 years ago

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Hey try this one "supermassive black holes". I posted it some days back.This was a q in APHO 2017

Spandan Senapati - 4 years ago

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Bro I don't have sufficient knowledge and skills to solve it I guess, btw I already saw your problem.

Harsh Shrivastava - 4 years ago

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@Harsh Shrivastava Oh you don't need to... The only thing that is needed is gravitation and some energy related to it.....The gravitational power is already given.....And you know this was a q in inpho-2017(it was a star-blackhole system).....I hadn't encountered....But believe me give it a try and you can solve it easily.....

Spandan Senapati - 4 years ago

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@Spandan Senapati I get the following idea:

Use dE/dt and then use Kepler's law to relate w and radius at any instant and then we are done.

Am I correct?

Harsh Shrivastava - 4 years ago

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@Harsh Shrivastava Ya done. That's what the question asked.

Spandan Senapati - 4 years ago

@Spandan Senapati We will integrate then between required limits.

Harsh Shrivastava - 4 years ago

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@Harsh Shrivastava Can you help me with limits and what is that schwarzradius?

Harsh Shrivastava - 4 years ago

@Spandan Senapati We can write E = -GM^2/(2a) at any instant.

Harsh Shrivastava - 4 years ago

@Harsh Shrivastava Give it a try...if not I will give some hints.....

Spandan Senapati - 4 years ago

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