collaborators

11 papers

astro-ph.GA2026

Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. III. Mass Distribution of Hierarchical Mergers

Katherine L. Gonglewski, Amy Secunda, Mordecai-Mark Mac Low +3

Active galactic nucleus (AGN) disks are a promising location for the formation of binary black holes (BBHs) that will merge on relatively short timescales and be detected by LIGO-V…

gr-qc2026

Exact Mass Conservation in Binary Neutron Star Merger Simulations

Boris Daszuta, Sebastiano Bernuzzi, Joan Fontbuté +4

A long-standing problem in the simulation of neutron star spacetimes is the treatment of vacuum regions outside the stars. The use of an artificial low-density atmosphere is a comm…

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

A formation scenario of black hole-envelope systems --viscous hydrodynamics simulation in general relativity--

Alan Tsz Lok Lam, Masaru Shibata, Kenta Hotokezaka +1

By performing a viscous hydrodynamics simulation in general relativity for super-Eddington accretion flows onto massive black holes of mass --, we discuss a fo…

astro-ph.HE2026

Accretion-powered flares from black hole-disk collisions in galactic nuclei

Joaquin Pelle, Kyohei Kawaguchi, Masaru Shibata +1

Black hole impacts on accretion disks in galactic nuclei can power luminous transients, but predicting their observable signatures is challenging because the post-collision flow is…

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…