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Space-time distributions
Space-time distributions
Mihaela D. Iftime
8
9
9 31 Aug 98
1
t
c
O Abstract
8 The space-time foliation Σ compatible with the gravitational field
1 g on a 4-manifold M determines a fibration π of M , π : M −→ N is a
surjective submersion over the 1-dimensional leaves space N . M is then
1 written as a disjoint union of the leaves of Σ, which are 3-dimensional
v spacelike surfaces on M .
9 0
5 The decomposition, T M = Σ ⊕ T M , also implies that we can
0 define a lift of the curves on N to curves (non-spacelike) on M .
0 The stable causality condition M [2] coincides with Σ being a causal
1 space-time distribution, generated by an exact timelike 1-form ω0 = dt
8 where t is some real function on M . In this case M is written as a
9
/ disjoint union of a family of spacelike 3-surfaces of constant t, which
c cover D+ (S) of a initial 3-surface S of M .
q
-
r
g AMS Classification numbers:
: Primary: 83C99
v
i Secondary: 53B30 53C50 53C12 57R30
X
r Keywords: space-time distribution, 4-manifold
a
1
1 Introduction
Note: We will denote by small Latin indices a, b, . . . numbers ranging from
0 to 3 and the small Greek indices α, β, . . . numbers
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