output
19932026
most citedQCD Phenomenology based on a Chiral Effective Lagrangian

1.6k citations

Showing 2017Show all

8 papers · 1 filter

gr-qc2017★ 53 cited

The status of KAGRA underground cryogenic gravitational wave telescope

KAGRA Collaboration, T. Akutsu, M. Ando +146

KAGRA is a 3-km interferometric gravitational wave telescope located in the Kamioka mine in Japan. It is the first km-class gravitational wave telescope constructed underground to…

cond-mat.stat-mech2017★ 8 cited

Anomalous diffusion analysis of the lifting events in the event-chain Monte Carlo for the classical XY models

Kenji Kimura, Saburo Higuchi

We introduce a novel random walk model that emerges in the event-chain Monte Carlo (ECMC) of spin systems. In the ECMC, the lifting variable specifying the spin to be updated chang…

gr-qc2017★ 8 cited

Note on Accuracy of the Post-Newtonian Approximation for Extreme-Mass Ratio Inspirals: Retrograde Orbits

Ryuichi Fujita, Norichika Sago, Hiroyuki Nakano

The post-Newtonian approximation is useful to discuss gravitational waveforms for binary inspirals. In this note, for retrograde circular orbits in the equatorial plane, we discuss…

gr-qc2017

Extracting the orbital axis from gravitational waves of precessing binary systems

Kyohei Kawaguchi, Koutarou Kyutoku, Hiroyuki Nakano +1

We present a new method for extracting the instantaneous orbital axis only from gravitational wave strains of precessing binary systems observed from a particular observer directio…

gr-qc2017★ 21 cited

Estimation of starting times of quasinormal modes in ringdown gravitational waves with the Hilbert-Huang transform

Kazuki Sakai, Ken-ichi Oohara, Hiroyuki Nakano +2

It is known that a quasinormal mode (QNM) of a remnant black hole dominates a ringdown gravitational wave (GW) in a binary black hole (BBH) merger. To study properties of the QNMs,…

gr-qc2017★ 43 cited

Post-Newtonian templates for binary black-hole inspirals: the effect of the horizon fluxes and the secular change in the black-hole masses and spins

Soichiro Isoyama, Hiroyuki Nakano

Black holes (BHs) in an inspiraling compact binary system absorb the gravitational-wave (GW) energy and angular-momentum fluxes across their event horizons and this leads to the se…