To determine the pressure distribution P(r) inside a fluid sphere of radius R and uniform density ρ in equilibrium under its own gravity, we consider a concentric spherical fluid element of radius r and thickness dr.
1. Gravitational Field inside the Sphere
The mass of the fluid enclosed within a sphere of radius r is:
M(r)=34πr3ρ
The gravitational field strength g(r) at a radial distance r (r≤R) is given by:
g(r)=r2GM(r)=r2G(34πr3ρ)=34πGρr
2. Condition for Hydrostatic Equilibrium
For the fluid element of thickness dr to be in equilibrium, the hydrostatic equation gives:
drdP=−ρg(r)
Substituting g(r) into the equation:
drdP=−34πGρ2r
3. Integrating to find P(r)
Assuming the pressure at the outer surface is zero, i.e., P(R)=0, we integrate from r to R:
∫P(r)0dP=−34πGρ2∫rRr′dr′
−P(r)=−34πGρ2[2R2−r2]
P(r)=32πGρ2(R2−r2)
Let C=32πGρ2. Thus, the pressure distribution is:
P(r)=C(R2−r2)
4. Evaluating the Options
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Option (A):
At the center (r=0):
P(r=0)=CR2=0
Therefore, Option (A) is incorrect.
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Option (B):
Calculating the pressures at r=43R and r=32R:
P(r=43R)=C[R2−(43R)2]=CR2(1−169)=167CR2
P(r=32R)=C[R2−(32R)2]=CR2(1−94)=95CR2
Taking their ratio:
P(r=32R)P(r=43R)=95167=16×57×9=8063
Therefore, Option (B) is correct.
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Option (C):
Calculating the pressures at r=53R and r=52R:
P(r=53R)=C[R2−(53R)2]=CR2(1−259)=2516CR2
P(r=52R)=C[R2−(52R)2]=CR2(1−254)=2521CR2
Taking their ratio:
P(r=52R)P(r=53R)=25212516=2116
Therefore, Option (C) is correct.
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Option (D):
Calculating the pressures at r=2R and r=3R:
P(r=2R)=C[R2−(2R)2]=43CR2
P(r=3R)=C[R2−(3R)2]=98CR2
Taking their ratio:
P(r=3R)P(r=2R)=9843=3227=2720
Therefore, Option (D) is incorrect.
Correct Options:
(B) and (C)