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Keisuke Taniguchi

Researcher at University of the Ryukyus

Publications -  80
Citations -  7335

Keisuke Taniguchi is an academic researcher from University of the Ryukyus. The author has contributed to research in topics: Neutron star & Black hole. The author has an hindex of 41, co-authored 77 publications receiving 6387 citations. Previous affiliations of Keisuke Taniguchi include University of Illinois at Urbana–Champaign & University of Wisconsin–Milwaukee.

Papers
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The Japanese space gravitational wave antenna DECIGO

Seiji Kawamura, +144 more
Journal ArticleDOI

Mass ejection from the merger of binary neutron stars

TL;DR: In this paper, numerical simulations for the merger of binary neutron stars are performed for a variety of equations of state (EOSs) and for a plausible range of the neutron star mass, focusing primarily on the properties of the material ejected from the system.
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Coalescence of Black Hole-Neutron Star Binaries

TL;DR: The current status of general relativistic studies for the coalescence of black hole-neutron star (BH-NS) binaries is reviewed and understanding for the merger and/or tidal disruption processes, the criterion for tidal disruption, and the properties of the remnant formed after the tidal disruption are summarized.
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The Japanese space gravitational wave antenna?DECIGO

Seiji Kawamura, +131 more
TL;DR: DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) as discussed by the authors is the future Japanese space gravitational wave antenna, which aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy.
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Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing

TL;DR: In this paper, three-dimensional simulations for the merger of binary neutron stars are performed in the framework of full general relativity, with particular attention to the black hole formation case and to the resulting mass of the surrounding disk for exploring the possibility for formation of the central engine of short-duration gamma-ray bursts (SGRBs).