activity
20002023
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 4.9k across the 104 of their papers we have counts for

collaborators

104 papers

gr-qc2023

Mass Ratio of Binary Black Holes Determined from LIGO/Virgo Data Restricted to Small False Alarm Rate

Tomoya Kinugawa, Takashi Nakamura, Hiroyuki Nakano

We focus on gravitational-wave events of binary black-hole mergers up to the third observing run with the minimum false alarm rate smaller than . These even…

gr-qc2023★ 1 cited

Stability of relativistic tidal response against small potential modification

Takuya Katagiri, Hiroyuki Nakano, Kazuyuki Omukai

The tidal response of compact objects in an inspiraling binary system is measured by a set of tidal Love and dissipation numbers imprinted in the gravitational waveforms. While a f…

gr-qc2022★ 40 cited

Vanishing Love of Black Holes in General Relativity: From Spacetime Conformal Symmetry of a Two-dimensional Reduced Geometry

Takuya Katagiri, Masashi Kimura, Hiroyuki Nakano +1

We study the underlying structure of the vanishing of the Love numbers of both Schwarzschild and Kerr black holes in terms of spacetime conformal symmetry in a unified manner for t…

gr-qc2022★ 11 cited

Eccentricity estimation from initial data for Numerical Relativity Simulations

Alessandro Ciarfella, James Healy, Carlos O. Lousto +1

We describe and study an instantaneous definition of eccentricity to be applied at the initial moment of full numerical simulations of binary black holes. The method consists of ev…

astro-ph.HE2022★ 2 cited

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

Tomoya Kinugawa, Takashi Nakamura, Hiroyuki Nakano

Two neutron star (NS)-black hole (BH) binaries, GW200105 and GW200115 found in the LIGO/Virgo O3b run have smaller BH mass of 6--9\, which is consistent with Population…

gr-qc2021★ 78 cited

Adiabatic waveforms from extreme-mass-ratio inspirals: an analytical approach

Soichiro Isoyama, Ryuichi Fujita, Alvin J. K. Chua +3

Scientific analysis for the gravitational-wave detector LISA will require theoretical waveforms from extreme-mass-ratio inspirals (EMRIs) that extensively cover all possible orbita…