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researcher

N. Andersson

77 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 author5
  • first author15
  • middle author23
  • last author33

Across the 76 of 77 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE26
  • gr-qc23
  • astro-ph21
  • astro-ph.SR5
  • astro-ph.CO1
  • hep-ph1
same name
  • N. Andersson — 13 papers, h 6
  • N. Andersson — 9 papers, h 4
  • N. Andersson — 2 papers, h 2
  • 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
20012023
most citedModelling magnetically deformed neutron stars

258 citations · 1.9k across the 48 of their papers we have counts for

collaborators
Showing 2022 · gr-qcShow all

4 papers · 2 filters

gr-qc2022★ 14 cited

The r-modes of slowly rotating, stratified neutron stars

Fabian Gittins, Nils Andersson

The only r-modes that exist in a globally barotropic, rotating, Newtonian star are the fundamental l=∣m∣ solutions, where l and m are the indices of the spherical harmonic…

gr-qc2022★ 8 cited

Formulating the r-mode problem for slowly rotating neutron stars

Nils Andersson, Fabian Gittins

We revisit the problem of inertial r-modes in stratified stars, drawing on a more precise description of the composition stratification in a mature neutron star. The results highli…

gr-qc2022★ 9 cited

Building post-Newtonian neutron stars

Nils Andersson, Fabian Gittins, Shanshan Yin +1

Owed to their compactness, neutron stars involve strong gravity and extreme density physics. Nevertheless, at present, there are a variety of problems where progress (at least conc…

gr-qc2022★ 16 cited

Rotating Love: The dynamical tides of spinning Newtonian stars

Pantelis Pnigouras, Fabian Gittins, Amlan Nanda +2

We carefully develop the framework required to model the dynamical tidal response of a spinning neutron star in an inspiralling binary system, in the context of Newtonian gravity,…

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