- R. Astron. 334, L27--L31 (2002) Dynamical instability differentially rotating stars
- Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity
- Black hole tidal problem in the Fermi normal coordinates Masaki Ishii,1
- Merger of binary neutron stars of unequal mass in full general relativity Masaru Shibata and Keisuke Taniguchi
- Stability and collapse of rapidly rotating, supramassive neutron stars: 3D simulations in general Masaru Shibata
- STABILITY RIGIDLY ROTATING RELATIVISTIC STARS WITH SOFT EQUATIONS STATE AGAINST GRAVITATIONAL COLLAPSE
- The Astrophysical Journal, 528:L29--L32, 2000 January 1 # 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- THE ASTROPHYSICAL JOURNAL, 542 : 453463, 2000 October 10 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction in rapidly rotating neutron stars
- Constraining Nuclear Equations State Using Gravitational Waves from Hypermassive Neutron Stars
- Merger of black hole and neutron star in general relativity: Tidal disruption, torus mass, and gravitational waves
- Collapse of Magnetized Hypermassive Neutron Stars in General Relativity Matthew D. Duez,1,* Yuk Tung Liu,1
- Progress of Theoretical Physics, Vol. 118, No. 2, August 2007 Magnetohydrodynamics of Neutrino-Cooled Accretion Tori around
- Merger of binary neutron stars with realistic equations of state in full general relativity Masaru Shibata,1
- THE ASTROPHYSICAL JOURNAL, 525 : 935949, 1999 November 10 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- Progress of Theoretical Physics, Vol. 107, No. 2, February 2002 Gravitational Waves from the Merger of Binary Neutron Stars
- Progress of Theoretical Physics, Vol. 117, No. 6, June 2007 A Formation Mechanism of Collapsar Black Hole
- THE ASTROPHYSICAL JOURNAL, 548 919931, 2001 February 20 ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- Fully general relativistic simulation of coalescing binary neutron stars: Preparatory tests Masaru Shibata
- COLLAPSE OF A ROTATING SUPERMASSIVE STAR TO A SUPERMASSIVE BLACK HOLE: POSTNEWTONIAN SIMULATIONS
- High-velocity collision of two black holes Masaru Shibata, Hirotada Okawa, and Tetsuro Yamamoto
- Thermodynamics of binary black holes and neutron stars John L. Friedman and Ko ji Uryu
- Gravitational waves from a spinning particle in circular orbits around a rotating black hole Takahiro Tanaka, Yasushi Mino, Misao Sasaki, and Masaru Shibata
- Progress of Theoretical Physics, Vol. 101, No. 6, June 1999 Fully General Relativistic Simulation of Merging Binary Clusters
- Progress of Theoretical Physics, Vol. 104, No. 2, August 2000 Axisymmetric Simulations of Rotating Stellar Collapse
- New criterion for direct black hole formation in rapidly rotating stellar collapse Yu-ichirou Sekiguchi and Masaru Shibata
- Axisymmetric collapse simulations of rotating massive stellar cores in full general relativity: Numerical study for prompt black hole formation
- Robustness of a high-resolution central scheme for hydrodynamic simulations in full general relativity
- Magnetized Hypermassive Neutron-Star Collapse: A Central Engine for Short Gamma-Ray Bursts
- Close-slow analysis for head-on collision of two black holes in higher dimensions: Bowen-York initial data
- Rotating black hole surrounded by self-gravitating torus in the puncture framework Masaru Shibata
- Nada: A new code for studying self-gravitating tori around black holes Pedro J. Montero,1
- Properties of general relativistic, irrotational binary neutron stars in close quasiequilibrium orbits: Polytropic equations of state
- Computing gravitational waves from slightly nonspherical stellar collapse to a black hole: Odd-parity perturbation
- Mon. Not. R. Astron. Soc. 343, 619626 (2003) Dynamical bar-mode instability of differentially rotating stars: effects
- IOP PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum Grav. 24 (2007) S125S137 doi:10.1088/0264-9381/24/12/S09
- COLLAPSE OF A ROTATING SUPERMASSIVE STAR TO A SUPERMASSIVE BLACK HOLE: ANALYTIC DETERMINATION OF THE BLACK HOLE MASS AND SPIN
- Simulating coalescing compact binaries by a new code (SACRA) Tetsuro Yamamoto and Masaru Shibata
- Computation of gravitational waves from inspiraling binary neutron stars in quasiequilibrium circular orbits: Formulation and calibration
- Magnetorotational collapse of massive stellar cores to neutron stars: Simulations in full general relativity
- Simulation of merging binary neutron stars in full general relativity: #2 case Masaru Shibata
- COLLAPSE OF ROTATING SUPRAMASSIVE NEUTRON STARS TO BLACK HOLES: FULLY GENERAL RELATIVISTIC SIMULATIONS
- Gravitational waves from black hole-neutron star binaries: Classification of waveforms Masaru Shibata,1
- Progress of Theoretical Physics, Vol. 101, No. 2, February 1999 3D Numerical Simulation of Black Hole Formation
- Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations
- Axisymmetric general relativistic hydrodynamics: Longterm evolution neutron stars stellar collapse neutron stars black holes
- Close-limit analysis for head-on collision of two black holes in higher dimensions: Brill-Lindquist initial data
- Merger of black hole-neutron star binaries: Nonspinning black hole case Masaru Shibata1
- Apparent horizon finder for general threedimensional spaces Masaru Shibata
- Deriving formulations for numerical computation binary neutron stars quasicircular orbits Masaru Shibata
- Evolution of neutron stars with toroidal magnetic fields: Axisymmetric simulation in full general relativity
- Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
- PHYSICAL REVIEW D VOLUME 53, NUMBER 2 15JANUARY 1996 Gravitational waves induced by a spinning particle falling into a rotating black hole
- Comparing the inspiral of irrotational and corotational binary neutron stars Matthew D. Duez, 1 Thomas W. Baumgarte, 1,2 Stuart L. Shapiro, 1,3 Masaru Shibata, 4 and Ko ji Uryu 5
- IOP PUBLISHING CLASSICAL AND QUANTUM GRAVITY Class. Quantum Grav. 24 (2007) S207S219 doi:10.1088/0264-9381/24/12/S14
- Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity
- Magnetohydrodynamics in full general relativity: Formulation and tests Masaru Shibata and Yu-ichirou Sekiguchi
- Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a rotating black hole: Up to O,,v8
- The Astrophysical Journal, 572:L39--L43, 2002 June 10 # 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
