323 citations · 3.6k across the 75 of their papers we have counts for
6 papers · 1 filter
The dynamics of neutron star crusts: Lagrangian perturbation theory for a relativistic superfluid-elastic system
N. Andersson, B. Haskell, G. L. Comer +1
The inner crust of a mature neutron star is composed of an elastic lattice of neutron-rich nuclei penetrated by free neutrons. These neutrons can flow relative to the crust once th…
Core and crust contributions in pulsar glitches: constraints from the slow rise of the largest glitch observed in the Crab pulsar
Brynmor Haskell, Vadym Khomenko, Marco Antonelli +1
Pulsar glitches are attributed to the sudden re-coupling of very weakly coupled large scale superfluid components in the neutron star interior. This process leads to rapid exchange…
Evidence for a minimum ellipticity in millisecond pulsars
G. Woan, M. D. Pitkin, B. Haskell +2
Neutron stars spin down over time due to a number of energy-loss processes. We provide tantalizing population-based evidence that millisecond pulsars (MSPs) have a minimum elliptic…
Fundamental physics and the absence of sub-millisecond pulsars
B. Haskell, J. L. Zdunik, M. Fortin +3
Observations of the spin distribution of rapidly rotating neutron stars show evidence for a lack of stars spinning at frequencies larger than Hz, well below the pred…
Estimating the EOS from the measurement of NS radii with 5% accuracy
M. Sieniawska, M. Bejger, B. Haskell
Observations of heavy () neutron stars in addition to the recent measurement of tidal deformability from the binary neutron-star merger GW170817, place interest…
Modelling pulsar glitches: the hydrodynamics of superfluid vortex avalanches in neutron stars
Vadym Khomenko, Brynmor Haskell
The dynamics of quantised vorticity in neutron star interiors is at the heart of most pulsar glitch models. However, the large number of vortices (up to ) involved…