The 2m ≤ r property of spherically symmetric static space-times

Physics Letters, Section A: General, Atomic and Solid State Physics

Volumn 218, Issue 3-6, 1996, Pages 147-150

  Mars, Marc ^a,c   Martín Prats, M Mercè ^b,c   Senovilla, José M M ^b,c  

^a QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^b UNIVERSITY OF BARCELONA   (Spain)

^c INSTITUT D ESTUDIS CATALANS   (Spain)

Author keywords

[No Author keywords available]

Indexed keywords

BLACK HOLES; ENERGY CONDITION; FINITE NUMBER; HYPER-SURFACES; PERFECT FLUID; SPACE TIME;

EID: 0042124896     PISSN: 03759601     EISSN: None     Source Type: Journal    
DOI: 10.1016/0375-9601(96)00391-X     Document Type: Article

References (7)

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2. A.D. Rendall and B.G. Schmidt, Class. Quantum Grav. 8 (1991) 985.
3. T. Zannias, Phys. Rev. D 41 (1990) 3252.
4. M. Mars and J.M.M Senovilla, Class. Quantum Grav. 10 (1993) 1865.
5. W.B. Bonnor and P.A. Vickers, Gen. Rel. Grav. 13 (1981) 29.
6. A. Lichnerowicz, Théories relativistes de la gravitation et de l'électromagnétisme (Masson, Paris, 1955).
7. S. Hawking and G.F.R. Ellis, The large scale structure of space-time (Cambridge Univ. Press, Cambridge, 1973).