Gravitational collapse of dust with a cosmological constant

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 62, Issue 2, 2000, Pages 3-

  Lake, Kayll ^a  

^a QUEEN S UNIVERSITY   (Canada)

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EID: 18344386801     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.62.027301     Document Type: Article

References (16)

1. D. Markovic and S. L. Shapiro, Phys. Rev. D 61, 084029 (2000). This problem has also been considered by
2. K. Nakao, Gen. Relativ. Gravit. 24, 1069 (1992). See also
3. A. Ilha and J. P. S. Lemos, Phys. Rev. D 55, 1788 (1997);
4. A. Ilha, A. Kleber, J. P. S. Lemos, J. Math. Phys. 40, 3509 (1999).
5. See, for example, A. G. Riess, Astron. J. 116, 1009 (1998);
6. S. Perlmutter, Astrophys. J. 517, 565 (1999);
7. I. Zehavi and A. Dekel, Nature (London) 401, 252 (1999).
8. G. C. Omer, Proc. Natl. Acad. Sci. USA 53, 1 (1965).
9. D. M. Eardley and L. Smarr, Phys. Rev. D 19, 2239 (1979).
10. See, for example, K. Lake, Phys. Rev. Lett. 68, 3129 (1992).
11. Following Ruban (Formula presented)V. A. Ruban, Zh. Éksp. Teor. Fiz. 56, 1914 (1969) [Sov. Phys. JETP 29, 1027 (1969)](Formula presented), the case (Formula presented) can be examined as a limit of the subclass (Formula presented). In this case the junction conditions impose the restriction (Formula presented).
12. See, for example, W. B. Bonnor, in Recent Development in General Relativity (Pergamon, New York, 1962).
13. W. Israel, Phys. Rev. 164, 1776 (1967).
14. For an early independent construction, see K. Lake and R. C. Roeder, Phys. Rev. D 15, 3513 (1977).
15. See, for example, P. Musgrave and K. Lake, Class. Quantum Grav. 13, 1885 (1996).
16. K. Lake, Phys. Rev. D 20, 370 (1979).