(a) Use Eq. (14.14) with γ=5/3 to calculate the fundamental radial pulsation period for a one-zone model of a pulsating white dwarf (use the values for Sirius B) and a 1.4 M⊙ neutron star. Compare these to the observed range of pulsar periods.
(b) Use Eq. (16.29) to calculate the minimum rotation period for the same stars, and compare them to the range of pulsar periods.
(c) Give an explanation for the similarity of your results.