Imprint of magnetic obliquity in apparent spin-down of radio pulsars
Sign Up to like & getrecommendations! Published in 2023 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1437
Abstract: Numerical simulations predict that the spin-down rate of a single rotation-powered neutron star depends on the angle α between its spin and magnetic axes as $P\dot{P} \propto \mu ^2 (k_0 + k_1\sin ^2\alpha )$, where… read more here.
Keywords: magnetic obliquity; obliquity apparent; imprint magnetic; spin ... See more keywords