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Question: The gravitational field due to a mass distribution is \(E = \dfrac{K}{{{x^3}}}\) in the x-direction....

The gravitational field due to a mass distribution is E=Kx3E = \dfrac{K}{{{x^3}}} in the x-direction. (K is a constant). Taking the gravitational potential to be zero at infinity, its value at a distance x is:

A. kx\dfrac{k}{x}

B. k2x\dfrac{k}{{2x}}

C. kx2\dfrac{k}{{{x^2}}}

D. k2x2\dfrac{k}{{2{x^2}}}

Explanation

Solution

Hint Use the definition of gravitational field as, the Force Exerted by a mass distribution on a unit mass, given by E=Kx3E = \dfrac{K}{{{x^3}}}
We will start with a test mass mmexperiencing the given field at dxdx distance and integrate it from infinity to x to compute Gravitational Potential.

Complete step by step answer
Given a test mass mm on the x-axis, the work done WW to move it a distance dxdx in the given gravitational field will be:

\Rightarrow W=mKx3.dxW = \dfrac{{mK}}{{{x^3}}}.dx [Since, W=F.SW = F.S, where F is the force and S is the displacement]

Hence, the work done in bringing the test mass from infinity to x will be

W=xmKx3dx \Rightarrow W = \int\limits_\infty ^x {\dfrac{{mK}}{{{x^3}}}} dx

Since gravitational potential is required work done to bring a unit mass from infinity to x,

P=Wm \Rightarrow P = \dfrac{W}{m}
Hence, for our case, gravitational potential PP will be,

P=1mxmKx3dx \Rightarrow P = \dfrac{1}{m}\int\limits_\infty ^x {\dfrac{{mK}}{{{x^3}}}} dx

Since, test mass m and constant K are independent of the variable x, we can bring it outside the integral,

P=1mmKx1x3dx \Rightarrow P = \dfrac{1}{m}mK\int\limits_\infty ^x {\dfrac{1}{{{x^3}}}} dx

Cancelling mm from the numerator and denominator and solving the integral usingx3dx=x3+13+1\int {{x^{ - 3}}}dx = \dfrac{{{x^{ - 3 + 1}}}}{{ - 3 + 1}} , we get
P=K[x22]x\Rightarrow P = K\left[ {\dfrac{{{x^{ - 2}}}}{{ - 2}}} \right]_\infty ^x

Hence we get the gravitational potential as:

P=K[12x2]x \Rightarrow P = - K\left[ {\dfrac{1}{{2{x^2}}}} \right]_\infty ^x

Putting the limits in the differential and using gravitational potential at \infty = 0, we get

P=K[12x20] \Rightarrow P = - K\left[ {\dfrac{1}{{2{x^2}}} - 0} \right]

This gives us the final value for potential at x, for the given electrical field as,

P=K2x2 \Rightarrow P = - \dfrac{K}{{2{x^2}}}

This is of the form,

P=k2x2 \Rightarrow P = \dfrac{k}{{2{x^2}}}

Note Alternative method – Use the formula for the Gravitational Potential as the Gravitational field from infinity to x as P=xKx3dxP = \int\limits_\infty ^x {\dfrac{K}{{{x^3}}}} dx. This method does not include the term for test mass m but is less intuitive.