Step 1: Define the surface mass density of the annular disc.
The inner radius is b = 3 R b = 3R b = 3 R and the outer radius is a = 4 R a = 4R a = 4 R . The total mass of the disc is M M M .
σ = M π ( a 2 − b 2 ) \sigma = \frac{M}{\pi(a^2 - b^2)} σ = π ( a 2 − b 2 ) M
σ = M π ( ( 4 R ) 2 − ( 3 R ) 2 ) \sigma = \frac{M}{\pi((4R)^2 - (3R)^2)} σ = π (( 4 R ) 2 − ( 3 R ) 2 ) M
σ = M 7 π R 2 \sigma = \frac{M}{7\pi R^2} σ = 7 π R 2 M
Step 2: Set up the integral for the gravitational potential at point P P P .
Point P P P is on the axis of the disc at a distance z = 4 R z = 4R z = 4 R from the center. Consider an elemental ring of radius r r r and width d r dr d r . Its mass d m dm d m is:
d m = σ ( 2 π r d r ) dm = \sigma(2\pi r \, dr) d m = σ ( 2 π r d r )
The gravitational potential d V dV d V at point P P P due to this elemental ring is:
d V = − G d m r 2 + z 2 dV = -\frac{G \, dm}{\sqrt{r^2 + z^2}} d V = − r 2 + z 2 G d m
d V = − 2 π G σ r d r r 2 + z 2 dV = -\frac{2\pi G \sigma r \, dr}{\sqrt{r^2 + z^2}} d V = − r 2 + z 2 2 π G σ r d r
Step 3: Integrate to find the total potential V ( P ) V(P) V ( P ) .
Integrate from the inner radius b b b to the outer radius a a a .
V ( P ) = − 2 π G σ ∫ b a r d r r 2 + z 2 V(P) = -2\pi G \sigma \int_{b}^{a} \frac{r \, dr}{\sqrt{r^2 + z^2}} V ( P ) = − 2 π G σ ∫ b a r 2 + z 2 r d r
V ( P ) = − 2 π G σ [ r 2 + z 2 ] b a V(P) = -2\pi G \sigma \left[ \sqrt{r^2 + z^2} \right]_{b}^{a} V ( P ) = − 2 π G σ [ r 2 + z 2 ] b a
V ( P ) = − 2 π G σ ( a 2 + z 2 − b 2 + z 2 ) V(P) = -2\pi G \sigma \left( \sqrt{a^2 + z^2} - \sqrt{b^2 + z^2} \right) V ( P ) = − 2 π G σ ( a 2 + z 2 − b 2 + z 2 )
Step 4: Substitute the given values.
Substitute a = 4 R a = 4R a = 4 R , b = 3 R b = 3R b = 3 R , and z = 4 R z = 4R z = 4 R into the square root terms.
a 2 + z 2 = ( 4 R ) 2 + ( 4 R ) 2 = 4 2 R \sqrt{a^2 + z^2} = \sqrt{(4R)^2 + (4R)^2} = 4\sqrt{2}R a 2 + z 2 = ( 4 R ) 2 + ( 4 R ) 2 = 4 2 R
b 2 + z 2 = ( 3 R ) 2 + ( 4 R ) 2 = 5 R \sqrt{b^2 + z^2} = \sqrt{(3R)^2 + (4R)^2} = 5R b 2 + z 2 = ( 3 R ) 2 + ( 4 R ) 2 = 5 R
Now substitute these values and σ \sigma σ into the expression for V ( P ) V(P) V ( P ) .
V ( P ) = − 2 π G ( M 7 π R 2 ) ( 4 2 R − 5 R ) V(P) = -2\pi G \left( \frac{M}{7\pi R^2} \right) \left( 4\sqrt{2}R - 5R \right) V ( P ) = − 2 π G ( 7 π R 2 M ) ( 4 2 R − 5 R )
V ( P ) = − 2 G M 7 R ( 4 2 − 5 ) V(P) = -\frac{2GM}{7R} \left( 4\sqrt{2} - 5 \right) V ( P ) = − 7 R 2 GM ( 4 2 − 5 )
Step 5: Calculate the work required to move a unit mass to infinity.
The work required W W W to move a unit mass from point P P P to infinity is given by the potential difference.
W = V ( ∞ ) − V ( P ) W = V(\infty) - V(P) W = V ( ∞ ) − V ( P )
Since V ( ∞ ) = 0 V(\infty) = 0 V ( ∞ ) = 0 :
W = − V ( P ) W = -V(P) W = − V ( P )
W = 2 G M 7 R ( 4 2 − 5 ) W = \frac{2GM}{7R} \left( 4\sqrt{2} - 5 \right) W = 7 R 2 GM ( 4 2 − 5 )
Answer:
The work required is 2 G M 7 R ( 4 2 − 5 ) \dfrac{2GM}{7R} \left( 4\sqrt{2} - 5 \right) 7 R 2 GM ( 4 2 − 5 ) .