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Nonlinear viscous damping and gravitational wave detectability of the f-mode instability in neutron stars
A. Passamonti, K. Glampedakis
We study the damping of the gravitational radiation-driven f-mode instability in rotating neutron stars by nonlinear bulk viscosity in the so-called supra-thermal regime. In this r…
Magnetars: super(ficially) hot and super(fluid) cool
Wynn C. G. Ho, Kostas Glampedakis, Nils Andersson
We examine to what extent the inferred surface temperature of magnetars in quiescence can constrain the presence of a superfluid in the neutron star core and the role of magnetic f…
Scientific Potential of Einstein Telescope
B. Sathyaprakash, M. Abernathy, F. Acernese +138
Einstein gravitational-wave Telescope (ET) is a design study funded by the European Commission to explore the technological challenges of and scientific benefits from building a th…
Hydromagnetic equilibrium in non-barotropic multifluid neutron stars
Kostas Glampedakis, Nils Andersson, Samuel K. Lander
Traditionally, the subject of hydromagnetic equilibrium in neutron stars has been addressed in the context of standard magnetohydrodynamics, with matter obeying a barotropic equati…
Magnetic neutron star equilibria with stratification and type-II superconductivity
S. K. Lander, N. Andersson, K. Glampedakis
We construct two-fluid equilibrium configurations for neutron stars with magnetic fields, using a self-consistent and nonlinear numerical approach. The two-fluid approach - likely…
Magneto-rotational neutron star evolution: the role of core vortex pinning
Kostas Glampedakis, Nils Andersson
We consider the pinning of superfluid (neutron) vortices to magnetic fluxtubes associated with a type II (proton) superconductor in neutron star cores. We demonstrate that core pin…