258 citations · 652 across the 6 of their papers we have counts for
7 papers
On the oscillations of dissipative superfluid neutron stars
N. Andersson, K. Glampedakis, B. Haskell
We investigate the oscillations of slowly rotating superfluid stars, taking into account the vortex mediated mutual friction force that is expected to be the main damping mechanism…
Oscillations of Rapidly Rotating Superfluid Stars
Andrea Passamonti, Brynmor Haskell, Nils Andersson
Using time evolutions of the relevant linearised equations we study non-axisymmetric oscillations of rapidly rotating and superfluid neutron stars. We consider perturbations of New…
Oscillations of rapidly rotating stratified neutron stars
A. Passamonti, B. Haskell, N. Andersson +2
We use time-evolutions of the linear perturbation equations to study the oscillations of rapidly rotating neutrons stars. Our models account for the buoyancy due to composition gra…
Are neutron stars with crystalline colour superconducting cores interesting for the LIGO experiment?
B. Haskell, N. Andersson, D. I. Jones +1
We estimate the maximal deformation that can be sustained by a rotating neutron star with a crystalline colour superconducting quark core. Our results suggest that current gravitat…
Modelling magnetically deformed neutron stars
B. Haskell, L. Samuelsson, K. Glampedakis +1
Rotating deformed neutron stars are important potential sources for groundbased gravitational-wave interferometers such as LIGO, GE0600 and VIRGO. One mechanism that may lead to si…
Mountains on Neutron Stars: Accreted vs. Non-Accreted crusts
B. Haskell, D. I. Jones, N. Andersson
The aim of this paper is to compare the two cases of an isolated neutron star, with a non-accreted crust, and that of an accreting neutron star, with an accreted crust, and try to…