activity
20062009
most citedSecond and higher-order quasi-normal modes in binary black hole mergers

70 citations · 121 across the 5 of their papers we have counts for

collaborators

7 papers

gr-qc2009

Comparison of Post-Newtonian and Numerical Evolutions of Black-Hole Binaries

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

In this paper, we compare the waveforms from the post-Newtonian (PN) approach with the numerical simulations of generic black-hole binaries which have mass ratio , arbitr…

gr-qc20086 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-qc2008118 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-qc200815 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-qc200823 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…

astro-ph200770 cited

Second and higher-order quasi-normal modes in binary black hole mergers

Kunihito Ioka, Hiroyuki Nakano

Black hole (BH) oscillations known as quasi-normal modes (QNMs) are one of the most important gravitational wave (GW) sources. We propose that higher perturbative order of QNMs, ge…