activity
20162023
most citedChirp Mass and Spin of Binary Black Holes from First Star Remnants

59 citations · 182 across the 9 of their papers we have counts for

collaborators

20 papers

astro-ph.HE20221 cited

On the population III binary black hole mergers with intermediate mass black holes: dependence on common envelope parameter

Kotaro Hijikawa, Tomoya Kinugawa, Ataru Tanikawa +2

The current gravitational wave (GW) detectors have successfully observed many binary compact objects, and the third generation ground-based GW detectors such as Einstein telescope…

astro-ph.HE202216 cited

Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?

Ataru Tanikawa, Gen Chiaki, Tomoya Kinugawa +2

Population (Pop) III stars, first stars, or metal-free stars are made of primordial gas. We have examined if they can be dominant origins of merging binary black holes (BHs) and ex…

astro-ph.HE202128 cited

On the population III binary black hole mergers beyond the pair-instability mass gap

Kotaro Hijikawa, Ataru Tanikawa, Tomoya Kinugawa +2

We perform a binary population synthesis calculation incorporating very massive population (Pop.) III stars up to 1500 , and investigate the nature of binary black hole (B…

astro-ph.HE2021

Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than

Tomoya Kinugawa, Takashi Nakamura, Hiroyuki Nakano

The probability number distribution function of binary black hole mergers observed by LIGO/Virgo O3a has double peaks as a function of chirp mass , total mass , primary b…

astro-ph.HE202141 cited

Impact of binary interactions on the diffuse supernova neutrino background

Shunsaku Horiuchi, Tomoya Kinugawa, Tomoya Takiwaki +2

Binary interactions, especially mass transfer and mergers, can strongly influence the evolution of massive stars and change their final properties and the occurrence of supernovae.…

astro-ph.HE2020

Formation of Binary Black Holes Similar to GW190521 with a Total Mass of from Population III Binary Star Evolution

Tomoya Kinugawa, Takashi Nakamura, Hiroyuki Nakano

In the case of zero-metal (population III or Pop III) stars, we show that the total mass of binary black holes from binary Pop III star evolution can be , whi…