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researcher

K. Kwon

4 papers hereh-index 210 citations11 works total

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

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • gr-qc4
same name
  • K. Kwon — 7 papers, h 6
  • K. Kwon — 3 papers, h 1
  • K. Kwon — 2 papers, h 4
  • K. Kwon — 1 paper, h 0
  • K. Kwon — 1 paper, h 3
  • K. Kwon — 1 paper, h 4

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

collaborators

4 papers

gr-qc2026

Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions

Hang Yu, Giorgio Nicolini, Shu Yan Lau +6

We study tides during the inspiral of a binary neutron star system, including nonlinear hydrodynamical interactions. Using an affine approximation that treats the perturbed neutron…

gr-qc2026

Relativistic and Dynamical Love

Abhishek Hegade K. R., K. J. Kwon, Tejaswi Venumadhav +2

Gravitational waves emitted in the late inspiral of binary neutron stars are affected by their tidal deformation. We study the tidal dynamics in full general relativity through mat…

gr-qc2025

Resonance Locking of Anharmonic g-Modes in Coalescing Neutron Star Binaries

K. J. Kwon, Hang Yu, Tejaswi Venumadhav

Neutron stars in coalescing binaries deform due to the tidal gravitational fields generated by their companions. During the inspiral phase, the tidal deformation is dominated by th…

gr-qc2025

Resonance locking: radian-level phase shifts due to nonlinear hydrodynamics of g-modes in merging neutron star binaries

K. J. Kwon, Hang Yu, Tejaswi Venumadhav

A neutron star (NS) in a binary system deforms due to the companion's tidal gravitational field. As the binary inspirals due to gravitational wave (GW) emission, the NS's deformati…

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