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researcher

N. Andersson

145 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 author9
  • first author43
  • middle author39
  • last author50

Across the 141 of 145 papers where every author was matched, so the position is known.

fields
  • gr-qc55
  • astro-ph.HE32
  • astro-ph30
  • astro-ph.SR24
  • astro-ph.CO1
  • cond-mat.other1
same name
  • N. Andersson — 13 papers, h 6
  • N. Andersson — 10 papers, h 4
  • N. Andersson — 3 papers, h 3
  • N. Andersson — 2 papers, h 2
  • N. Andersson — 2 papers, h 3
  • N. Andersson — 1 paper, h 20

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
19952023
most citedSensitivity Studies for Third-Generation Gravitational Wave Observatories

1.1k citations · 12.5k across the 144 of their papers we have counts for

collaborators
Showing 1997Show all

4 papers · 1 filter

gr-qc1997★ 541 cited

Towards gravitational-wave asteroseismology

Nils Andersson, Kostas D. Kokkotas

We present new results for pulsating neutron stars. We have calculated the eigenfrequencies of the modes that one would expect to be the most important gravitational-wave sources:…

gr-qc1997★ 695 cited

A new class of unstable modes of rotating relativistic stars

Nils Andersson

The first numerical study of axial (toroidal) pulsation modes of a slowly rotating relativistic star is presented. The calculation includes terms of first order in $ε\equiv Ω\sqrt{…

gr-qc1997★ 26 cited

Pulsation modes for increasingly relativistic polytropes

Nils Andersson, Kostas D. Kokkotas

We present the results of a numerical study of the fluid f, p and the gravitational w modes for increasingly relativistic nonrotating polytropes. The results for f and w-…

gr-qc1997★ 126 cited

Gravitational waves from pulsating stars: Evolving the perturbation equations for a relativistic star

Gabrielle Allen, Nils Andersson, Kostas D. Kokkotas +1

We consider the perturbations of a relativistic star as an initial-value problem. Having discussed the formulation of the problem (the perturbation equations and the appropriate bo…

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