activity
20092026
most citedProduction of all the r-process nuclides in the dynamical ejecta of neutron star mergers

624 citations · 9k across the 85 of their papers we have counts for

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Showing 2020Show all

7 papers · 1 filter

astro-ph.HE2020★ 29 cited

Properties of the remnant disk and the dynamical ejecta produced in low-mass black hole-neutron star mergers

Kota Hayashi, Kyohei Kawaguchi, Kenta Kiuchi +2

We systematically perform numerical-relativity simulations for low-mass black hole-neutron star mergers for the models with seven mass ratios ranging from…

astro-ph.HE2020★ 53 cited

Viscous evolution of a massive disk surrounding stellar-mass black holes in full general relativity

Sho Fujibayashi, Masaru Shibata, Shinya Wanajo +3

Long-term viscous neutrino-radiation hydrodynamics simulations in full general relativity are performed for a massive disk surrounding spinning stellar-mass black holes with mass $…

astro-ph.HE2020★ 24 cited

Polarized kilonovae from black hole-neutron star mergers

M. Bulla, K. Kyutoku, M. Tanaka +6

We predict linear polarization for a radioactively-powered kilonova following the merger of a black hole and a neutron star. Specifically, we perform 3-D Monte Carlo radiative tran…

gr-qc2020★ 3 cited

Reducing orbital eccentricity in initial data of black hole--neutron star binaries in the puncture framework

Koutarou Kyutoku, Kyohei Kawaguchi, Kenta Kiuchi +2

We develop a method to compute low-eccentricity initial data of black hole--neutron star binaries in the puncture framework extending previous work on other types of compact binari…

astro-ph.HE2020★ 99 cited

Post-merger Mass Ejection of Low-mass Binary Neutron Stars

Sho Fujibayashi, Shinya Wanajo, Kenta Kiuchi +3

We study the post-merger mass ejection of low-mass binary neutron stars (NSs) with the system mass of , and subsequent nucleosynthesis by performing general-relativi…

astro-ph.HE2020★ 66 cited

On the possibility of GW190425 being a black hole--neutron star binary merger

Koutarou Kyutoku, Sho Fujibayashi, Kota Hayashi +4

We argue that the kilonova/macronova associated with the gravitational-wave event GW190425 could have been bright enough to be detected if it was caused by the merger of a low-mass…