323 citations · 3.6k across the 75 of their papers we have counts for
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The effect of superfluid hydrodynamics on pulsar glitch sizes and waiting times
Brynmor Haskell
Pulsar glitches, sudden jumps in frequency observed in many radio pulsars, may be the macroscopic manifestation of superfluid vortex avalanches on the microscopic scale. Small scal…
Pinned vortex hopping in a neutron star crust
Brynmor Haskell, Andrew Melatos
The motion of superfluid vortices in a neutron star crust is at the heart of most theories of pulsar glitches. Pinning of vortices to ions can decouple the superfluid from the crus…
Observational constraints on neutron star crust-core coupling during glitches
William G. Newton, Sabrina Berger, Brynmor Haskell
We demonstrate that observations of glitches in the Vela pulsar can be used to investigate the strength of the crust-core coupling in a neutron star, and suggest that recovery from…
Models of Pulsar Glitches
Brynmor Haskell, Andrew Melatos
Radio pulsars provide us with some of the most stable clocks in the universe. Nevertheless several pulsars exhibit sudden spin-up events, known as glitches. More than forty years a…
Detecting gravitational waves from mountains on neutron stars in the Advanced Detector Era
Brynmor Haskell, Maxim Priymak, Alessandro Patruno +3
Rapidly rotating Neutron Stars (NSs) in Low Mass X-ray Binaries (LMXBs) are thought to be interesting sources of Gravitational Waves (GWs) for current and next generation ground ba…
Mesoscopic pinning forces in neutron star crusts
Stefano Seveso, Pierre M. Pizzochero, Fabrizio Grill +1
The crust of a neutron star is thought to be comprised of a lattice of nuclei immersed in a sea of free electrons and neutrons. As the neutrons are superfluid their angular momentu…