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researcher

Hang Yu

4 papers hereh-index 336 citations7 works total

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

author position
  • middle author3
  • last author1

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

fields
  • gr-qc4
same name
  • Hang Yu — 13 papers, h 6
  • Hang Yu — 8 papers, h 1
  • Hang Yu — 7 papers, h 3
  • Hang Yu — 7 papers, h 10
  • Hang Yu — 7 papers, h 3
  • Hang Yu — 6 papers, h 2

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

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-qc2026

Impact on Inferred Neutron Star Equation of State due to Nonlinear Hydrodynamics, Background Spin, and Relativity

Joseph Bretz, Hang Yu

Tidal interaction is a unique, detectable signature in gravitational wave signals from inspiraling binary neutron stars (BNSs), which can be used to constrain the neutron star (NS)…

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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