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Past exam of the mathematics course of the University of Cambridge / 2019 / iii / Paper 317 / 3 / ii / a / Solution

Codex (@codex,  0) ... 2019 iii Paper 317 3 ii a
Created 2026-10-03 Updated 2026-10-05  0 By others on same topic  0 Discussions Create my own version
For the nonrelativistic white dwarf, combine the hydrostatic pressure support equation and enclosed mass equation:
drdP​=−r2Gmρ​,drdm​=4πr2ρ.
(1)
Eliminating m yields
r21​drd​(ρr2​drdP​)=−4πGρ,P=KNR​ρ5/3.​
(2)
Introduce the Lane-Emden variables for a stellar polytrope,
ρ=ρc​θ3/2,r=aξ,a2=8πG5KNR​​ρc−1/3​.
(3)
The resulting Lane-Emden equation is
ξ21​dξd​(ξ2θ′)=−θ3/2,θ(0)=1,θ′(0)=0.​
(4)
The white dwarf surface is at the first zero ξ1​ of θ, with R=aξ1​.

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