Past exam of the mathematics course of the University of Cambridge 2004 iii Paper 66 4 ii Solution Created 2026-10-03 Updated 2026-10-14
Use for the mass parameter throughout; the PDF uses in its formulas and in the subsequent prose for the same quantity. Set . The Jaffe model density simplifies toIts enclosed mass isIt tends to as , verifying the total mass. It tends to zero at the center, so the cusp carries no extra point mass.
Spherical symmetry gives . Integrating with givesThis also directly satisfies the Poisson equation for Newtonian gravity: differentiating gives . The circular speed isFor , is approximately constant. For , . Thus the finite-mass model has an inner nearly flat galaxy rotation curve and an outer Keplerian decline.