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 2013Show all

11 papers · 1 filter

astro-ph.HE2013★ 14 cited

Pre-merger localization of eccentric compact binary coalescences with second-generation gravitational-wave detector networks

Koutarou Kyutoku, Naoki Seto

We study the possibility of pre-merger localization of eccentric compact binary coalescences by second-generation gravitational-wave detector networks. Gravitational waves from ecc…

astro-ph.HE2013★ 132 cited

Radioactively Powered Emission from Black Hole-Neutron Star Mergers

Masaomi Tanaka, Kenta Hotokezaka, Koutarou Kyutoku +4

Detection of electromagnetic counterparts of gravitational wave (GW) sources is important to unveil the nature of compact binary coalescences. We perform three-dimensional, time-de…

astro-ph.HE2013★ 119 cited

Progenitor models of the electromagnetic transient associated with the short GRB 130603B

Kenta Hotokezaka, Koutarou Kyutoku, Masaomi Tanaka +4

An electromagnetic transient powered by the radioactive decay of r-process elements, a so-called kilonova/macronova, is one of the possible observable consequences of compact binar…

astro-ph.HE2013★ 47 cited

High-Energy Radiation from Remnants of Neutron Star Binary Mergers

Hajime Takami, Koutarou Kyutoku, Kunihito Ioka

We study high-energy emission from the mergers of neutron star binaries as electromagnetic counterparts to gravitational waves aside from short gamma-ray bursts. The mergers entail…

astro-ph.HE2013★ 324 cited

Remnant massive neutron stars of binary neutron star mergers: Evolution process and gravitational waveform

Kenta Hotokezaka, Kenta Kiuchi, Koutarou Kyutoku +4

Massive (hypermassive and supramassive) neutron stars are likely to be often formed after the merger of binary neutron stars. We explore the evolution process of the remnant massiv…

gr-qc2013★ 34 cited

Nonspinning black hole-neutron star mergers: a model for the amplitude of gravitational waveforms

Francesco Pannarale, Emanuele Berti, Koutarou Kyutoku +1

Black hole-neutron star binary mergers display a much richer phenomenology than black hole-black hole mergers, even in the relatively simple case - considered in this paper - in wh…