Solving the Darwin problem in the first post-Newtonian approximation of general relativity: Compressible model

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 56, Issue 2, 1997, Pages 811-825

  Shibata, Masaru ^a   Taniguchi, Keisuke ^b  

^a OSAKA UNIVERSITY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000175151     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.811     Document Type: Article

References (16)

1. K. Taniguchi and M. Shibata, preceding paper, Phys. Rev. D56, 798 (1997).
2. D. Lai, F. A. Rasio, and S. L. Shapiro, Astrophys. J. Suppl. Ser. 88, 205 (1993); APJSA2
3. Astrophys. J. 420, 811 (1994).
4. For example, S. L. Shapiro and S. A. Teukolsky, Black Holes, White Dwarfs, and Neutron Stars (Wiley, New York, 1983).
5. M. Shibata, Phys. Rev. D55, 6019 (1997);
6. Prog. Theor. Phys. 96, 317 (1996).
7. S. Chandrasekhar, Astrophys. J. 142, 1488 (1965).
8. S. Chandrasekhar, Astrophys. J. 148, 621 (1967); also see nice collection, Selected Papers, S. Chandrasekhar (The University of Chicago Press, Chicago, 1990), Vol. 5.
9. H. Asada and M. Shibata, Phys. Rev. D 54, 4944 (1996).
10. S. Chandrasekhar, Ellipsoidal Figures of Equilibrium (Yale University Press, New Haven, CT, 1969).
11. C. M. Will, Theory and Experiment in Gravitational Physics (Cambridge University Press, Cambridge, England, 1981), p. 146.
12. S. Chandrasekhar, Astrophys. J. 140, 417 (1964);
13. 142, 1519 (1965).
14. A. G. Wiseman, Report No. (unpublished).
15. D. Lai, Phys. Rev. Lett. 76, 4878 (1996): He showed that the Newtonian tidal effect acts to stabilize each star of binary.
16. J. R. Wilson, G. J. Mathews, and P. Marrinetti, Phys. Rev. D 54, 1317 (1996).