activity
20012022
most citedModelling magnetically deformed neutron stars

258 citations · 1.8k across the 39 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.HE20211 cited

Thermal aspects of neutron star mergers

Peter Hammond, Ian Hawke, Nils Andersson

In order to extract maximal information from neutron-star merger signals, both gravitational and electromagnetic, we need to ensure that our theoretical models/numerical simulation…

gr-qc202120 cited

A covariant approach to relativistic large-eddy simulations: The fibration picture

Thomas Celora, Nils Andersson, Ian Hawke +1

Models of turbulent flows require the resolution of a vast range of scales, from large eddies to small-scale features directly associated with dissipation. As the required resoluti…

astro-ph.HE2021

The I-Love-Q Relations for Superfluid Neutron Stars

Cheung-Hei Yeung, Lap-Ming Lin, Nils Andersson +1

The I-Love-Q relations are approximate equation-of-state independent relations that connect the moment of inertia, the spin-induced quadrupole moment, and the tidal deformability o…

gr-qc20211 cited

A gravitational-wave perspective on neutron-star seismology

N. Andersson

We provide a bird's-eye view of neutron-star seismology, which aims to probe the extreme physics associated with these objects, in the context of gravitational-wave astronomy. Focu…

gr-qc2021

A multifluid perspective on multimessenger modelling

N. Andersson

This brief review introduces the notion of a relativistic multifluid system -- a multi-component system with identifiable relative flows -- and outlines a set of models for scenari…

astro-ph.HE202132 cited

A superfluid perspective on neutron star dynamics

N. Andersson

As mature neutron stars are cold (on the relevant temperature scale), one has to carefully consider the state of matter in their interior. The outer kilometer or so is expected to…