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N. Andersson

30 papers hereh-index 5212k citations225 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author1
  • first author3
  • middle author7
  • last author18

Across the 29 of 30 papers where every author was matched, so the position is known.

fields
  • astro-ph21
  • gr-qc6
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • N. Andersson — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20012011
most citedModelling magnetically deformed neutron stars

258 citations · 1.3k across the 20 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 219 cited

Neutron Star Asteroseismology. Axial Crust Oscillations in the Cowling Approximation

Lars Samuelsson, Nils Andersson

Recent observations of quasi-periodic oscillations in the aftermath of giant flares in soft gamma-ray repeaters suggest a close coupling between the seismic motion of the crust aft…

astro-ph2006★ 156 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-ph2006★ 63 cited

Ekman layer damping of r-modes revisited

Kostas Glampedakis, Nils Andersson

We investigate the damping of neutron star r-modes due to the presence of a viscous boundary (Ekman) layer at the interface between the crust and the core. Our study is motivated b…

astro-ph2006★ 103 cited

Elastic or magnetic? A toy model for global magnetar oscillations with implications for QPOs during flares

Kostas Glampedakis, Lars Samuelsson, Nils Andersson

We use a simple toy-model to discuss global MHD modes of a neutron star, taking into account the magnetic coupling between the elastic crust and the fluid core. Our results suggest…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.