JEE Challenger
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Work Done Moving Mass from Axis of Annular Disc to Infinity

A thin uniform annular disc (see figure) of mass M has outer radius 4R and inner radius 3R. The work required to take a unit mass from point P on its axis to infinity is

Diagram 0

Options

A

2GM7R(42−5)\frac{2GM}{7R}(4\sqrt{2}-5)

Correct
B

−2GM7R(42−5)-\frac{2GM}{7R}(4\sqrt{2}-5)

C

GM4R\frac{GM}{4R}

D

2GM5R(2−1)\frac{2GM}{5R}(\sqrt{2}-1)

Topics & Concepts

Step-by-Step Solution

To find the work required to move a unit mass from point PP on the axis of the annular disc to infinity, we first need to determine the gravitational potential at point PP.

1. Surface Mass Density of the Annular Disc

The outer radius of the disc is R2=4RR_2 = 4R and the inner radius is R1=3RR_1 = 3R.
The total surface area of the annular disc is:
A=πR22−πR12=π(4R)2−π(3R)2=7πR2A = \pi R_2^2 - \pi R_1^2 = \pi (4R)^2 - \pi (3R)^2 = 7\pi R^2

Thus, the surface mass density σ\sigma of the disc is:
σ=MA=M7πR2\sigma = \frac{M}{A} = \frac{M}{7\pi R^2}


2. Gravitational Potential at Point PP

Point PP lies on the central axis of the disc at a distance z=4Rz = 4R from its center.

Consider a thin circular ring element of radius rr and thickness drdr centered on the disc. The mass of this element is:
dm=σ⋅(2πr dr)dm = \sigma \cdot (2\pi r \, dr)

The gravitational potential dVdV at point PP due to this differential ring element is:
dV=−G dmr2+z2=−2πGσr drr2+z2dV = -\frac{G \, dm}{\sqrt{r^2 + z^2}} = -\frac{2\pi G \sigma r \, dr}{\sqrt{r^2 + z^2}}

Integrating dVdV over the entire annular disc from r=3Rr = 3R to r=4Rr = 4R:
VP=−2πGσ∫3R4Rr drr2+z2V_P = -2\pi G \sigma \int_{3R}^{4R} \frac{r \, dr}{\sqrt{r^2 + z^2}}

Using the integration rule ∫r drr2+z2=r2+z2\int \frac{r \, dr}{\sqrt{r^2 + z^2}} = \sqrt{r^2 + z^2}:
VP=−2πGσ[r2+z2]3R4RV_P = -2\pi G \sigma \left[ \sqrt{r^2 + z^2} \right]_{3R}^{4R}

Substitute z=4Rz = 4R:
VP=−2πGσ((4R)2+(4R)2−(3R)2+(4R)2)V_P = -2\pi G \sigma \left( \sqrt{(4R)^2 + (4R)^2} - \sqrt{(3R)^2 + (4R)^2} \right)
VP=−2πGσ(32R2−25R2)=−2πGσ(42R−5R)V_P = -2\pi G \sigma \left( \sqrt{32 R^2} - \sqrt{25 R^2} \right) = -2\pi G \sigma (4\sqrt{2} R - 5R)

Substituting the value of σ=M7πR2\sigma = \frac{M}{7\pi R^2}:
VP=−2πG(M7πR2)R(42−5)V_P = -2\pi G \left( \frac{M}{7\pi R^2} \right) R (4\sqrt{2} - 5)
VP=−2GM7R(42−5)V_P = -\frac{2GM}{7R}(4\sqrt{2} - 5)


3. Calculation of Work Done

The work required by an external agent to take a unit mass (m=1m = 1) from point PP to infinity (r→∞r \to \infty) slowly is given by the change in gravitational potential energy:
W=U(∞)−U(P)=m(V∞−VP)W = U(\infty) - U(P) = m \left( V_\infty - V_P \right)

Since V∞=0V_\infty = 0 and m=1m = 1:
W=0−VP=−VPW = 0 - V_P = -V_P

Substituting VPV_P:
W=−(−2GM7R(42−5))=2GM7R(42−5)W = -\left( -\frac{2GM}{7R}(4\sqrt{2} - 5) \right) = \frac{2GM}{7R}(4\sqrt{2} - 5)

Thus, the correct option is A.