Featured
-
-
-
Letter |
Rotational evolution of young pulsars due to superfluid decoupling
The so-called braking index calculated for the spin-down of rotating neutron stars, or pulsars, doesn’t tally well with observations. But a model accounting for a changing moment of inertia, as an increasing fraction of the stellar core becomes superfluid, can explain the rotational evolution of young pulsars.
- Wynn C. G. Ho
- & Nils Andersson