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in Gravitation by (20 points)
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The gravitational potential at the centre \( O \) of a uniform solid hemisphere of mass \( M \) and radius \( R \) is Zero \( -\frac{G M}{2 R} \) \( -\frac{3 G M}{2 R} \) \( -\frac{3 G M}{4 R} \)

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+1 vote
by (34.1k points)

Let the elemental disc or radius Rsinθ and thickness Rdθ. it mass

dM = \(\frac{M}{\frac23\pi R^3}\pi\)(Rsinθ)2(Rdθsinθ)

dM = \(\frac{3M}{2R^3}\)R2sin2θ Rsinθ dθ

dM = \(\frac{3M}2\)sin3θ dθ

Net potential due to a element under consideration at the centre at the hemisphere

dV = \(-\frac{2GdM}{r(cosec\theta-cot\theta)}\) (potential due to circular phase)

dV = \(\frac{3GMsin^3\theta(cosec\theta-cot\theta)}{(Rsin\theta)}d\theta\) 

dV = \(-\frac{+3GM}{R}\)(sin2θ cosec θ - sin2θ cot θ)

dV = \(-\frac{3GM}R\)(sin θ - cos θ) dθ

there

V = \(-\frac{3GM}R\)\(\int\limits_0^{\pi/2}(sin\theta-cos\theta.sin\theta)d\theta\) 

V = \(-\frac{3GM}R\)  \([-cos\theta+\frac{cos^2\theta}2]_0^{\pi/2}\)

V =  \(-\frac{3GM}R\)

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