Published Papers in Journal (1996--1997, in Osaka)
- 17. Y.Mino, M.Shibata and T.Tanaka,
Phys. Rev. D 53 (1996), 622-634; Err. D 59 (1999), 047502
Gravitational waves induced by a spinning particle falling into a
rotating black hole
(pdf file: /pdf)
- 18. H.Tagoshi, M.Shibata, T.Tanaka and M.Sasaki
Phys. Rev. D 54 (1996), 1439-1459
Post-Newtonian Expansion of Gravitational Waves from a Particle
in Circular Orbits around a Rotating Black Hole: Up to $O(^{8})$
beyond the Quadrupole Formula
(pdf file: /pdf)
- 19. T.Tanaka, Y.Mino, M.Sasaki and M.Shibata,
Phys. Rev. D 54 (1996), 3762-3777
Gravitational waves by a spinning particle in circular orbits
around a rotating black hole
(pdf file: /pdf)
- 20. H.Asada, M.Shibata and T.Futamase,
Prog. Theor. Phys. 96 (1996), 81-112
Post-Newtonian hydrodynamic equations using the (3+1) formalism in
general relativity
(ps file: /ps)
- 21. M.Shibata,
Prog. Theor. Phys. 96 (1996), 317-325
Instability of synchronized binary neutron stars in the first
post-Newtonian approximation of general relativity
(pdf file: /pdf)
- 22. H.Asada and M.Shibata,
Phys. Rev. D 54 (1996), 4944-4954
Formulation for non-axisymmetric uniformly rotating equilibrium
configurations in the second post-Newtonian order
- 23. M.Shibata,
Phys. Rev. D 55 (1997), 2002-2013
Apparent horizon finder for a special family of spacetimes in 3D numerical relativity
(ps file: /ps)
- 24. M.Shibata,
Prog. Theor. Phys. 96 (1996), 917-932
Relativistic Roche-Riemann Problems around a Black Hole
(pdf file: /pdf)
- 25. M.Shibata,
Phys. Rev. D 55 (1997), 6019-6029
Numerical Study of Synchronized Binary Neutron Stars in Post-Newtonian
Approximation of General Relativity
- 26. M.Shibata,
Phys. Rev. D 55 (1997), 7529-7537
Time Symmetric Initial Conditions of Gravitational Waves for 3D
Numerical Relativity
- 27. K.Taniguchi and M.Shibata,
Phys. Rev. D 56 (1997), 798-810
Solving the Darwin Problem in the First Post-Newtonian Approximation
of General Relativity
- 28. M.Shibata and K.Taniguchi
Phys. Rev. D 56 (1997), 811-825
Solving the Darwin Problem in the First Post-Newtonian Approximation
of General Relativity : Compressive Model
- 29. M.Shibata, K.Oohara and T.Nakamura
Prog. Theor. Phys. 98 (1997), 1081-1098
Numerical Study on the Hydrodynamic Instability of Binary Stars
in the First Post Newtonian Approximation of General Relativity
- 30. Y.Mino, M.Sasaki, M.Shibata, H.Tagoshi and T.Tanaka
Prog. Theor. Phys.(Supplement) 128 (1997), Chapter 1(pp.1)
- 31. K.Oohara, T.Nakamura and M.Shibata
Prog. Theor. Phys.(Supplement) 128 (1997), Chapter 3(pp.183)
A Way to 3D Numerical Relativity
- 32. M.Shibata, K.Taniguchi and T.Nakamura
Prog. Theor. Phys.(Supplement) 128 (1997), Chapter 5(pp.295)
Location of the Innermost Stable Circular Orbit of Binary Neutron Stars in the
Post Newtonian Approximations of General Relativity