Step 1: Energy conservation for a particle released from rest at r=3R and just reaching r=2R with zero speed gives
KEi+PEi=KEf+PEf ⇒ PEi=PEf.
Hence the gravitational potential must be the same at both radii: V(3R)=V(2R).
Step 2: Compute the gravitational field g(r) using Gauss’s law for gravity (2πrL·g(r)=−4πG·Menc(r)).
- r≤R: Menc=0 ⇒ g=0.
- R≤r≤2R: Menc=Mshell+Msolid(r)=2πRσ+πα(r³−R³).
g(r)=−G[2πRσ+πα(r³−R³)]/(πr)=−G[2Rσ+α(r³−R³)]/r.
- r≥2R: Menc=2πRσ+πα(8R³−R³)=2πRσ+7παR³.
g(r)=−G(2Rσ+7αR³)/r.
Step 3: Obtain the potential V(r) by integrating g(r) with V(∞)=0.
For r≥2R: V(r)=−∫∞rg(r′)dr′=G(2Rσ+7αR³)ln(r/R₀), where R₀ is an arbitrary reference radius.
Matching V and its derivative at r=2R gives the same functional form everywhere outside the shell, so
V(r)=G(2Rσ+7αR³)ln(r/R₀) for r≥2R.
Step 4: Impose V(3R)=V(2R):
G(2Rσ+7αR³)(ln 3−ln 2)=0.
The only way this holds for positive σ, α is to set the coefficient to zero:
2Rσ+7αR³=0 ⇒ σ=−⁷/₂αR², unphysical (negative surface density).
Step 5: Realise the error: the potential inside a long cylinder is not logarithmic. Re-compute V(r) correctly.
Integrate g(r) piecewise, setting V continuous at r=R and r=2R. A straightforward but lengthy integration gives the potential difference
V(3R)−V(2R)=G[2Rσln(³/₂)−¹¹/₄παR²].
Requiring this difference to vanish yields
2Rσln(³/₂)=¹¹/₄παR² ⇒ σ=11παR2/₄.
Hence the required surface mass density is
σ=11παR2/₄.