41 citations · 71 across the 3 of their papers we have counts for
8 papers
Jet-powered supernovae of population III stars are observable by , , , and
Tatsuya Matsumoto, Daisuke Nakauchi, Kunihito Ioka +1
Supermassive black holes observed at high redshift could grow from direct collapse black holes (DCBHs) with mass , which result from the collapse o…
Can direct collapse black holes launch gamma-ray bursts and grow to supermassive black holes?
Tatsuya Matsumoto, Daisuke Nakauchi, Kunihito Ioka +2
The existence of black holes (BHs) of mass ~ 10^{9} M_sun at z > 6 is a big puzzle in astrophysics because even optimistic estimates of the accretion time are insufficient for stel…
Optical Synchrotron Precursors of Radio Hypernovae
Daisuke Nakauchi, Kazumi Kashiyama, Hiroki Nagakura +2
We examine the bright radio synchrotron counterparts of low-luminosity gamma-ray bursts (llGRBs) and relativistic supernovae (SNe) and find that they can be powered by spherical hy…
Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave
Tomoya Kinugawa, Kohei Inayoshi, Kenta Hotokezaka +2
We perform population synthesis simulations for Population III (Pop III) coalescing binary neutron stars (NS-NSs), neutron star - black hole binaries (NS-BHs), and binary black hol…
Soft X-ray Extended Emissions of Short Gamma-Ray Bursts as Electromagnetic Counterparts of Compact Binary Mergers; Possible Origin and Detectability
Takashi Nakamura, Kazumi Kashiyama, Daisuke Nakauchi +3
We investigate the possible origin of extended emissions (EEs) of short gamma-ray bursts with an isotropic energy of ~ 10^(50-51) erg and a duration of a few 10 s to ~ 100 s, based…
Blue Supergiant Model for Ultra-Long Gamma-Ray Burst with Superluminous-Supernova-Like Bump
Daisuke Nakauchi, Kazumi Kashiyama, Yudai Suwa +1
Long GRBs (LGRBs) have typical duration of ~ 30 s and some of them are associated with hypernovae, like Type Ic SN 1998bw. Wolf-Rayet stars are the most plausible LGRB progenitors,…