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Formation pathway of Population III coalescing binary black holes through stable mass transfer

Monthly notices of the Royal Astronomical Society, 2017-07, Vol.468 (4), p.5020-5032

2017

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Chirp mass and spin of binary black holes from first star remnants

Monthly notices of the Royal Astronomical Society, 2020-11, Vol.498 (3), p.3946-3963

2020

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Population III binary black holes: effects of convective overshooting on formation of GW190521

Monthly notices of the Royal Astronomical Society, 2021-08, Vol.505 (2), p.2170-2176

2021

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Impact of binary interactions on the diffuse supernova neutrino background

Physical review. D, 2021-02, Vol.103 (4), Article 043003

2021

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Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave

Monthly notices of the Royal Astronomical Society, 2014-08, Vol.442 (4), p.2963-2992

2014

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The detection rate of inspiral and quasi-normal modes of Population III binary black holes which can confirm or refute the general relativity in the strong gravity region

Monthly notices of the Royal Astronomical Society, 2016-02, Vol.456 (1), p.1093-1114

2016

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Merger Rate Density of Population III Binary Black Holes Below, Above, and in the Pair-instability Mass Gap

The Astrophysical journal, 2021-03, Vol.910 (1), p.30

2021

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Fitting formulae for evolution tracks of massive stars under extreme metal-poor environments for population synthesis calculations and star cluster simulations

Monthly notices of the Royal Astronomical Society, 2020-07, Vol.495 (4), p.4170-4191

2020

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Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data

The Astrophysical journal, 2023-04, Vol.946 (2), p.79

2023

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Merger Rate Density of Binary Black Holes through Isolated Population I, II, III and Extremely Metal-poor Binary Star Evolution

The Astrophysical journal, 2022-02, Vol.926 (1), p.83

2022

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Merger Conditions of Population III Protostar Binaries

The Astrophysical journal, 2023-06, Vol.950 (2), p.188

2023

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Probe for Type Ia Supernova Progenitor in Decihertz Gravitational Wave Astronomy

The Astrophysical journal, 2022-10, Vol.938 (1), p.52

2022

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Long Gamma-Ray Burst Rate at Very High Redshift

The Astrophysical journal, 2019-06, Vol.878 (2), p.128

2019

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

Monthly notices of the Royal Astronomical Society. Letters, 2021-07, Vol.505 (1), p.L69-L73

2021

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The Rate of iPTF 14gqr like Ultra-stripped Supernovae and Binary Evolution Leading to Double Neutron Star Formation

The Astrophysical journal, 2019-09, Vol.882 (2), p.93

2019

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Constraints on population I/II neutron star-black hole binary formation by gravitational wave and radio observations

Monthly notices of the Royal Astronomical Society. Letters, 2022-09, Vol.515 (1), p.L78-L83

2022

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Long Gamma-Ray Burst Rate in the Binary Merger Progenitor Model

Astrophysical journal. Letters, 2017-11, Vol.849 (2), p.L29

2017

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How to confirm the existence of population III stars by observations of gravitational waves

Physical review. D, 2017-09, Vol.96 (6), Article 064025

2017

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Formation of mass gap compact object and black hole binary from Population III stars

Progress of theoretical and experimental physics, 2021-02, Vol.2021 (2)

2021

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The possible existence of Pop III NS-BH binary and its detectability

Progress of theoretical and experimental physics, 2017-02, Vol.2017 (2)

2017

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Gravitational wave quasinormal mode from Population III massive black hole binaries in various models of population synthesis

Progress of theoretical and experimental physics, 2016-10, Vol.2016 (10), p.103

2016

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Mass ratio of binary black holes determined from LIGO/Virgo data restricted to small false alarm rate

Monthly notices of the Royal Astronomical Society, 2024-06, Vol.531 (4), p.4725-4733

2024

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Possible confirmation of the existence of the ergoregion by the Kerr quasinormal mode in gravitational waves from a Population III massive black hole binary

Progress of theoretical and experimental physics, 2016-03, Vol.2016 (3), p.31

2016

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Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than ∼20 M

Monthly notices of the Royal Astronomical Society. Letters, 2021-06, Vol.504 (1), p.L28-L33

2021

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Synthesis of Biladienone and Bilatrienone by Coupled Oxidation of Tetraarylporphyrins

Journal of organic chemistry, 2007-07, Vol.72 (14), p.5320-5326

2007

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Formation pathway of Population III coalescing binary black holes through stable mass transfer

Chirp mass and spin of binary black holes from first star remnants

Population III binary black holes: effects of convective overshooting on formation of GW190521

Impact of binary interactions on the diffuse supernova neutrino background

Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave

The detection rate of inspiral and quasi-normal modes of Population III binary black holes which can confirm or refute the general relativity in the strong gravity region

Merger Rate Density of Population III Binary Black Holes Below, Above, and in the Pair-instability Mass Gap

Fitting formulae for evolution tracks of massive stars under extreme metal-poor environments for population synthesis calculations and star cluster simulations

Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data

Merger Rate Density of Binary Black Holes through Isolated Population I, II, III and Extremely Metal-poor Binary Star Evolution

Merger Conditions of Population III Protostar Binaries

Probe for Type Ia Supernova Progenitor in Decihertz Gravitational Wave Astronomy

Long Gamma-Ray Burst Rate at Very High Redshift

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

The Rate of iPTF 14gqr like Ultra-stripped Supernovae and Binary Evolution Leading to Double Neutron Star Formation

Constraints on population I/II neutron star-black hole binary formation by gravitational wave and radio observations

Long Gamma-Ray Burst Rate in the Binary Merger Progenitor Model

How to confirm the existence of population III stars by observations of gravitational waves

Formation of mass gap compact object and black hole binary from Population III stars

The possible existence of Pop III NS-BH binary and its detectability

Gravitational wave quasinormal mode from Population III massive black hole binaries in various models of population synthesis

Mass ratio of binary black holes determined from LIGO/Virgo data restricted to small false alarm rate

Possible confirmation of the existence of the ergoregion by the Kerr quasinormal mode in gravitational waves from a Population III massive black hole binary

Gravitational waves from Population III binary black holes are consistent with LIGO/Virgo O3a data for the chirp mass larger than ∼20 M

Synthesis of Biladienone and Bilatrienone by Coupled Oxidation of Tetraarylporphyrins

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