Solution

ID: past-exam-of-the-mathematics-course-of-the-university-of-cambridge/2019/iii/paper-317/3/ii/a/solution

For the nonrelativistic white dwarf, combine the hydrostatic pressure support equation and enclosed mass equation:
Eliminating yields
Introduce the Lane-Emden variables for a stellar polytrope,
The resulting Lane-Emden equation is
The white dwarf surface is at the first zero of , with .

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