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

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.HE2018★ 25 cited

How to detect the shortest-period binary pulsars in the era of LISA

Koutarou Kyutoku, Yuki Nishino, Naoki Seto

We discuss a multimessenger strategy to detect radio pulses from Galactic binary neutron stars in a very tight orbit with the period shorter than 10 min. On one hand, all-sky surve…

astro-ph.HE2018★ 18 cited

Discrepancy in tidal deformability of GW170817 between the Advanced LIGO twin detectors

Tatsuya Narikawa, Nami Uchikata, Kyohei Kawaguchi +4

We find that the Hanford and Livingston detectors of Advanced LIGO derive a distinct posterior probability distribution of binary tidal deformability tilde{Lambda} of the first bin…

astro-ph.CO2018★ 61 cited

Effect of Inhomogeneity on Primordial Black Hole Formation in the Matter Dominated Era

Takafumi Kokubu, Koutarou Kyutoku, Kazunori Kohri +1

We investigate the effect of inhomogeneity on primordial black hole formation in the matter dominated era. In the gravitational collapse of an inhomogeneous density distribution, a…

gr-qc2018★ 12 cited

Systematic effects from black hole-neutron star waveform model uncertainties on the neutron star equation of state

Kabir Chakravarti, Anuradha Gupta, Sukanta Bose +12

We identify various contributors of systematic effects in the measurement of the neutron star (NS) tidal deformability and quantify their magnitude for several types of neutron sta…

astro-ph.HE2018★ 37 cited

The origin of polarization in kilonovae and the case of the gravitational-wave counterpart AT 2017gfo

M. Bulla, S. Covino, K. Kyutoku +8

The Gravitational Wave (GW) event GW 170817 was generated by the coalescence of two neutron stars (NS) and produced an electromagnetic transient, labelled AT 2017gfo, that was targ…

gr-qc2018★ 77 cited

Frequency-domain gravitational waveform models for inspiraling binary neutron stars

Kyohei Kawaguchi, Kenta Kiuchi, Koutarou Kyutoku +3

We develop a model for frequency-domain gravitational waveforms from inspiraling binary neutron stars. Our waveform model is calibrated by comparison with hybrid waveforms construc…