A pulsar's spin-down can be written as a power law
PHYSICS · Multi-part · Fermi University Physics · Relativity & Gravitation · Astrophysics & Cosmology · Stellar death and compact objects
Stars from the Inside, Ch Neutron stars and pulsars: the densest matter, the maximum mass and the spinning magnet
Problem
A pulsar's spin-down can be written as a power law Ω˙=−KΩn, where K>0 is a constant fixed by the star's moment of inertia I, magnetic moment and inclination angle, and n is the braking index. Observationally n is found from n≡Ω˙2ΩΩ¨.
((a)) Show that evaluating this ratio on the power law above returns n itself, independent of K and of the instantaneous value of Ω, so n can be measured from Ω, Ω˙ and Ω¨ alone without ever knowing K.
((b)) Magnetic-dipole spin-down gives Ω˙∝−Ω3. State the braking index a pure magnetic dipole predicts.
((c)) The Crab pulsar's rotation frequency and its first two time derivatives are measured to be ν=29.6Hz, ν˙=−3.71×10−10Hzs−1 and ν¨=1.17×10−20Hzs−2. Because n is a ratio of logarithmic derivatives it takes the same value whether computed from Ω=2πν or from ν directly. Compute the observed braking index and compare it with the pure-dipole prediction of part (b).
((d)) Integrate Ω˙=−KΩn from birth, when the period was P0, to today, and show that the age is t=(n−1)P˙P[1−(PP0)n−1], which reduces to τc=P/2P˙ for n=3 and P0≪P. The Crab has P=33.4ms, P˙=4.2×10−13, τc=1260yr and a true age of about 970yr. Taking n=2.52, find its birth period P0, and say whether n<3 or a non-negligible P0 is what makes τc exceed the true age.