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researcher

K. Reuter

10 papers hereh-index 114.1k citations30 works total

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

author position
  • first author2
  • middle author5
  • last author2

Across the 9 of 10 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • cs.DC2
  • physics.comp-ph2
  • physics.plasm-ph2
  • math.NA1
  • physics.flu-dyn1
same name
  • K. Reuter — 116 papers, h 75
  • K. Reuter — 4 papers, h 2
  • K. Reuter — 4 papers, h 14
  • K. Reuter — 3 papers, h 6
  • K. Reuter — 2 papers, h 4
  • K. Reuter — 1 paper, h 19

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
20092026
most citedA Spherical Plasma Dynamo Experiment

36 citations · 122 across the 9 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.GA2026

Simulating tidal disruption events in nuclear star clusters

Philip Cho, Kai Wu, Francesco Flammini Dotti +5

Context. Nuclear star clusters (NSCs) and supermassive black holes (SMBHs) often coexist at the centers of galaxies, engaging in complex dynamical interactions that influence SMBH…

physics.plasm-ph2026

A High-order piecewise field-aligned triangular finite element method for electromagnetic gyrokinetic particle simulations of tokamak plasmas with open field lines

Zhixin Lu, Guo Meng, Eric Sonnendruecker +6

A high-order piecewise field-aligned triangular finite element method is developed and implemented for global electromagnetic gyrokinetic particle-in-cell simulations of tokamak pl…

astro-ph.GA2026★ 1 cited

FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters

Antti Rantala, Thorsten Naab, Natalia Lahén +4

We explore the formation of intermediate mass black holes (IMBHs), potential seeds for supermassive black holes (SMBHs), via runaway stellar collisions for a wide range of star clu…

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