activity
19972020
most citedConstruction of KAGRA: an Underground Gravitational Wave Observatory

86 citations · 665 across the 26 of their papers we have counts for

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12 papers · 1 filter

astro-ph2008★ 2 cited

Amplification of azimuthal modes with odd wave numbers during dynamical bar-mode growth in rotating stars

Yasufumi Kojima, Motoyuki Saijo

Nonlinear growth of the bar-mode deformation is studied for a differentially rotating star with supercritical rotational energy. In particular, the growth mechanism of some azimuth…

astro-ph2008★ 13 cited

Faraday resonance in dynamical bar instability of differentially rotating stars

Motoyuki Saijo, Yasufumi Kojima

We investigate the nonlinear behaviour of the dynamically unstable rotating star for the bar mode by three-dimensional hydrodynamics in Newtonian gravity. We find that an oscillati…

astro-ph2006★ 17 cited

Viscosity driven instability in rotating relativistic stars

Motoyuki Saijo, Eric Gourgoulhon

We investigate the viscosity driven instability in rotating relativistic stars by means of an iterative approach. We focus on polytropic rotating equilibrium stars and impose an m=…

astro-ph2006★ 2 cited

Low T/|W| dynamical instabilities in differentially rotating stars: Diagnosis with canonical angular momentum

Motoyuki Saijo, Shin'ichirou Yoshida

We study the nature of non-axisymmetric dynamical instabilities in differentially rotating stars with both linear eigenmode analysis and hydrodynamic simulations in Newtonian gravi…

astro-ph2005★ 13 cited

Dynamical bar instability in a relativistic rotational core collapse

Motoyuki Saijo

We investigate the rotational core collapse of a rapidly rotating relativistic star by means of a 3+1 hydrodynamical simulations in conformally flat spacetime of general relativity…

astro-ph2005★ 59 cited

Low T/|W| dynamical instability in differentially rotating stars: Diagnosis with canonical angular momentum

Motoyuki Saijo, Shin'ichirou Yoshida

We study the nature of non-axisymmetric dynamical instabilities in differentially rotating stars with both linear eigenmode analysis and hydrodynamic simulations in Newtonian gravi…

astro-ph2005

Dynamical One-Armed Spiral Instability in Differentially Rotating Stars

Motoyuki Saijo, Shin'ichirou Yoshida

We investigate the dynamical one-armed spiral instability in differentially rotating stars with both eigenmode analysis and hydrodynamic simulations in Newtonian gravity. We find t…

astro-ph2004★ 29 cited

The Collapse of Differentially Rotating Supermassive Stars: Conformally Flat Simulations

Motoyuki Saijo

We investigate the gravitational collapse of rapidly rotating relativistic supermassive stars by means of a 3+1 hydrodynamical simulations in conformally flat spacetime of general…

astro-ph2002★ 53 cited

Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Post-Newtonian Simulations

Motoyuki Saijo, Thomas W. Baumgarte, Stuart L. Shapiro +1

We study the gravitational collapse of a rotating supermassive star (SMS) by means of a (3+1) hydrodynamical simulation in a post-Newtonian (PN) approxi- mation of general relativi…

astro-ph2000★ 14 cited

Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals II : Spectra for various cases

Motoyuki Saijo, Takashi Nakamura

We compute the spectrum and the waveform of gravitational waves generated by the inspiral of a disk or a spherical like dust body into a Kerr black hole. We investigate the effect…

astro-ph2000★ 61 cited

Dynamical Bar Instability in Rotating Stars: Effect of General Relativity

Motoyuki Saijo, Masaru Shibata, Thomas W. Baumgarte +1

We study the dynamical stability against bar-mode deformation of rapidly and differentially rotating stars in the first post-Newtonian approximation of general relativity. We vary…

astro-ph2000★ 12 cited

Possible direct method to determine the radius of a star from the spectrum of gravitational wave signals

Motoyuki Saijo, Takashi Nakamura

We computed the spectrum of gravitational waves from a dust disk star of radius R inspiraling into a Kerr black hole of mass M and specific angular momentum a. We found that when R…