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Question: A semicircular ring of mass m and radius $R$ is fixed as shown. A point mass $m_0$ is moved by an ex...

A semicircular ring of mass m and radius RR is fixed as shown. A point mass m0m_0 is moved by an external agent from OO to OO'. The work done by gravitational field in moving m0m_0 from OO to OO' is:

A

Gmm0R[{2πln(2+1)}1]\frac{Gmm_0}{R}\left[\left\{\frac{2}{\pi}ln(\sqrt{2}+1)\right\}-1\right]

B

Gmm0R[{1πln(2+1)}1]\frac{Gmm_0}{R}\left[\left\{\frac{1}{\pi}ln(\sqrt{2}+1)\right\}-1\right]

C

Gmm0R[{2πln(2+1)}1]\frac{Gmm_0}{R}\left[\left\{-\frac{2}{\pi}ln(\sqrt{2}+1)\right\}-1\right]

D

Gmm0R[{1πln(2+1)}1]\frac{Gmm_0}{R}\left[\left\{-\frac{1}{\pi}ln(\sqrt{2}+1)\right\}-1\right]

Answer

Gmm0R[2πln(2+1)1]\frac{G m m_0}{R}\left[\frac{2}{\pi}\ln(\sqrt2+1)-1\right]

Explanation

Solution

To find the work done by the gravitational field when a point mass m0m_0 is moved from point OO to OO', we need to calculate the change in gravitational potential energy.

  1. Potential at O: Every element of the ring is at a distance RR, so V(O)=GmRV(O) = -\frac{Gm}{R}.

  2. Potential at O': The distance from a mass element at (Rcosθ,Rsinθ)(R \cos\theta, R \sin\theta) to OO' (which is (0,R)(0, -R)) is r(θ)=R2(1+sinθ)r(\theta) = R \sqrt{2(1 + \sin\theta)}.

The potential at OO' is V(O)=GmπR20πdθ1+sinθV(O') = -\frac{Gm}{\pi R \sqrt{2}} \int_0^\pi \frac{d\theta}{\sqrt{1 + \sin\theta}}.

  1. Evaluating the integral: Using the identity 1+sinθ=(sin(θ2)+cos(θ2))21 + \sin\theta = (\sin(\frac{\theta}{2}) + \cos(\frac{\theta}{2}))^2, the integral becomes:

I=0πdθsin(θ2)+cos(θ2)=22ln(21)I = \int_0^\pi \frac{d\theta}{\sin(\frac{\theta}{2}) + \cos(\frac{\theta}{2})} = -2\sqrt{2} \ln(\sqrt{2} - 1).

  1. Potential at O': V(O)=GmπR2I=2GmπRln(2+1)V(O') = -\frac{Gm}{\pi R \sqrt{2}} \cdot I = -\frac{2Gm}{\pi R} \ln(\sqrt{2} + 1).

  2. Work done by gravity: Wgrav=V(O)V(O)=GmR+2GmπRln(2+1)=Gmm0R[2πln(2+1)1]W_{grav} = V(O) - V(O') = -\frac{Gm}{R} + \frac{2Gm}{\pi R} \ln(\sqrt{2} + 1) = \frac{Gmm_0}{R} \left[ \frac{2}{\pi} \ln(\sqrt{2} + 1) - 1 \right].

Thus, the work done by the gravitational field is Gmm0R[2πln(2+1)1]\frac{G m m_0}{R} \left[ \frac{2}{\pi} \ln(\sqrt{2} + 1) - 1 \right].