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S. W. Hawking, Commun. Math. Phys. 25, 152 (1972); S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, 1973), p. 329.
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Hawking, S.W.1
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33744571220
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Cambridge University Press, Cambridge
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S. W. Hawking, Commun. Math. Phys. 25, 152 (1972); S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge University Press, Cambridge, 1973), p. 329.
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Ellis, G.F.R.2
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B. Carter, Commun. Math. Phys. 17, 233 (1970); B. Carter, in Black Hole Physics, Les Houches 1972, edited by, C. DeWitt, and, B. S. DeWitt, (Gordon and Breach, New York, 1978).
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Carter, B.1
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13
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13644255715
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2 T* with the vector field K ε Χ(M).
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2 T* with the vector field K ε Χ(M).
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14
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0000016294
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R. Geroch, E. H. Kronheimer, and R. Penrose, Proc. R. Soc. London, Ser. A 327, 545 (1972).
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Geroch, R.1
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Penrose, R.3
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15
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13644249544
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A point p in (M,g) is called a future end point of a causal curve γ:F→M, if for every neighborhood U of p there is a t̃ ∈F such that γ(t)∈U for all t∈F, with t>t̃. The definition of past endless and past end point is analogous.
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A point p in (M,g) is called a future end point of a causal curve γ:F→M, if for every neighborhood U of p there is a t̃ ∈F such that γ(t)∈U for all t∈F, with t>t̃. The definition of past endless and past end point is analogous.
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16
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13644254246
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A set S- is said to be a past-set if S- ⊂ I- (S-), or if S- is the chronological past of some set.
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A set S- is said to be a past-set if S- ⊂ I- (S-), or if S- is the chronological past of some set.
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17
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0004057466
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University of Chicago Press, Chicago
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R. M. Wald, General Relativity (University of Chicago Press, Chicago, 1984), pp. 434-436.
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Wald, R.M.1
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