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20032008
most citedMountains on Neutron Stars: Accreted vs. Non-Accreted crusts

156 citations · 350 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph200889 cited

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…

astro-ph200832 cited

Do superfluid instabilities prevent neutron star precession?

K. Glampedakis, N. Andersson, D. I. Jones

We discuss short wavelength (inertial wave) instabilities present in the standard two-fluid neutron star model when there is sufficient relative flow along the superfluid neutron v…

gr-qc200773 cited

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…

astro-ph2006156 cited

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…

astro-ph2003

The nature of low T/|W| dynamical instabilities in differentially rotating stars

A. L. Watts, N. Andersson, D. I. Jones

Recent numerical simulations indicate the presence of dynamical instabilities of the f-mode in differentially rotating stars even at very low values of , the ratio of kineti…