collaborators

10 papers

gr-qc2026

Celephais: efficient spectral initial data code for precessing compact binaries

Hao-Jui Kuan

Large numerical-relativity surveys require compact-binary initial data that are both spectrally accurate and inexpensive to construct, including for systems with unequal masses and…

gr-qc2026

Donutization Inside Neutron Stars: Shell-Localized Scalar Fields

Hao-Jui Kuan, Alan Tsz-Lok Lam, Jacquelyn Noronha-Hostler +1

Heavy scalar fields ( eV) in scalar-tensor gravity are expected to be hidden from neutron-star observations because their Compton wavelength is sub-stellar. We…

astro-ph.HE2026

Nonradial oscillations of stratified neutron stars with solid crusts: Mode characterization and tidal resonances in coalescing binaries

Yong Gao, Hao-Jui Kuan, Cheng-Jun Xia +2

Dynamical tides of neutron stars in the late stages of binary inspirals provide a viable probe into dense matter through gravitational waves, and potentially trigger electromagneti…

astro-ph.HE2026

Convective stability analysis of massive neutron stars formed in binary mergers

Yong Gao, Kota Hayashi, Kenta Kiuchi +3

We perform fully general-relativistic hydrodynamics simulations of binary neutron star mergers over post-merger to investigate the dynamics of remnant massive neutron…

gr-qc2025

Difference between quark stars and neutron stars in universal relations and their effect on gravitational waves

Duanyuan Gao, Hao-Jui Kuan, Yurui Zhou +4

We calculate the -mode frequency and tidal overlap of quark stars using the full general relativity method. We verify the universal relations obtained from conventional neutron…

hep-ph2025

Tidal Resonance in Binary Neutron Star Inspirals: A High-Precision Study in Numerical Relativity

Hao-Jui Kuan, Kenta Kiuchi, Masaru Shibata

We investigate the tidal resonance of the fundamental (-)mode in spinning neutron stars, robustly tracing the onset of the excitation to its saturation, using numerical relativi…