Gravitational collapse with a cosmological constant

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 61, Issue 8, 2000, Pages

  Shapiro, Stuart L ^a  

^a University of Illinois at Urbana Champaign   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17044376185     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.084029     Document Type: Article

References (14)

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4. J. R. Oppenheimer and H. Snyder, Phys. Rev. 56, 455 (1939).
5. J. Morrow-Jones, Ph.D. thesis, University of California, Santa Barbara, 1988.
6. F. Kottler, Ann. Phys. (Leipzig) 56, 410 (1918).
7. W. Israel, Nuovo Cimento B 44B, 1 (1966).
8. Vacuum region E in Fig. 44.
9. Vacuum regions A and D in Fig. 44.
10. Vacuum regions B and C in Fig. 44.
11. E. Schrödinger, Expanding Universes (Oxford University Press, Oxford, England, 1956).
12. S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, England, 1973).
13. The critical mass satisfies (Formula presented), where recent Type Ia supernovae measurements give (Formula presented) of order, but just below, unity 12. Here (Formula presented) is Hubble’s constant.
14. A related analysis using a different approach and focusing on the exterior spacetime in the context of the cosmic “no hair” conjecture has been provided by K. Nakao, Gen. Relativ. Gravit. 24, 1069 (1992).