Published Papers in Journal (2003--2004, in Tokyo)

64. M. Shibata, Phys. Rev. D 67(2003), 024033-1--24

Axisymmetric general relativistic hydrodynamics: Longterm evolution of neutron stars and collapse to neutron stars and black holes (ps file: /ps) (pdf file: /pdf)

65. M. Shibata, S. Karino and Y. Eriguchi, MNRAS 343 (2003), 619--626

Dynamical bar-mode instability of differentially rotating stars : Study for a wide parameter space (pdf file: /pdf)

66. T. Harada, H. Iguchi and M. Shibata, Phys. Rev. D 68 (2003), 024002-1--21

Computing gravitational waves from slightly nonspherical stellar collapse to black hole: Odd-parity perturbation (pdf file: /pdf)

67. M. Shibata, Astrophys. J. 595 (2003), 992--999

Collapse of Rotating Supramassive Neutron Stars to Black Holes: Fully General Relativistic Simulations (ps file: /ps) (pdf file: /pdf)

68. M. Shibata, K. Taniguchi, and K. Uryu, Phys. Rev. D 68 (2003), 084020-1--24

Merger of binary neutron stars of unequal mass in full general relativity (ps file: /ps)

69. M. Shibata and Y. Sekiguchi, Phys. Rev. D 68 (2003), 104020-1--14

Gravitational waves from axisymmetrically oscillating neutron stars in general relativistic simulations (ps file: /ps)

70. M. Shibata, Astrophys. J. 605 (2004), 350--359

Stability of rigidly rotating relativistic stars with soft equations of state against gravitational collapse (ps file: /ps)

71. M. Shibata and Y. Sekiguchi, Phys. Rev. D 69 (2004), 084024-1--16

Gravitational waves from axisymmetric rotating stellar core collapse to a neutron star in full general relativity (pdf file: /pdf)

72. M. Shibata, K. Uryu, and J. L. Friedman, Phys. Rev. D 70 (2004), 044044-1--18

Deriving formulations for numerical computation of binary neutron stars in quasicircular orbits (ps file: /ps)

73. Y. Sekiguchi and M. Shibata, Phys. Rev. D 70 (2004), 084005-1--14

New Criterion for direct black hole formation in rapidly rotating stellar collapse (pdf file: /pdf)

74. M. Ishii and M. Shibata, Prog. Theor. Phys. 112 (2004), 399--413

Numerical Study for the Tidal Disruption of Neutron Stars moving around a Black Hole: Compressible Jeans and Roche problems

75. M. Shibata and S. Karino, Phys. Rev. D 70 (2004), 084022-1--15

Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction (pdf file: /pdf)