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20002023
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

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

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Showing 2008Show all

6 papers · 1 filter

gr-qc2008★ 6 cited

Perturbations of Spacetime around a Stationary Rotating Cosmic String

Kouji Ogawa, Hideki Ishihara, Hiroshi Kozaki +1

We consider the metric perturbations around a stationary rotating Nambu-Goto string in Minkowski spacetime. By solving the linearized Einstein equations, we study the effects of az…

gr-qc2008★ 118 cited

Comparison of Numerical and Post-Newtonian Waveforms for Generic Precessing Black-Hole Binaries

Manuela Campanelli, Carlos O. Lousto, Hiroyuki Nakano +1

We compare waveforms and orbital dynamics from the first long-term, fully non-linear, numerical simulations of a generic black-hole binary configuration with post-Newtonian predict…

gr-qc2008★ 15 cited

Regular second order perturbations of binary black holes: The extreme mass ratio regime

Carlos O. Lousto, Hiroyuki Nakano

In order to derive the precise gravitational waveforms for extreme mass ratio inspirals (EMRI), we develop a formulation for the second order metric perturbations produced by a poi…

gr-qc2008★ 23 cited

Stationary Rotating Strings as Relativistic Particle Mechanics

Kouji Ogawa, Hideki Ishihara, Hiroshi Kozaki +2

Stationary rotating strings can be viewed as geodesic motions in appropriate metrics on a two-dimensional space. We obtain all solutions describing stationary rotating strings in f…

gr-qc2008★ 11 cited

A new method to integrate (2+1)-wave equations with Dirac's delta functions as sources

Carlos O. Lousto, Hiroyuki Nakano

Unlike in the Schwarzschild black hole background, gravitational perturbations in a Kerr black hole background can not be decomposed into simple tensor harmonics in the time domain…

gr-qc2008

New method to integrate 2+1 wave equations with Dirac's delta functions as sources

Hiroyuki Nakano, Carlos O. Lousto

Gravitational perturbations in a Kerr black hole background can not be decomposed into simple tensor harmonics in the time domain. Here, we make the mode decomposition only in the…