THE STRUCTURE OF PERTURBATIVE QUANTUM-GRAVITY ON A DESITTER BACKGROUND

被引:143
作者
TSAMIS, NC [1 ]
WOODARD, RP [1 ]
机构
[1] UNIV FLORIDA,DEPT PHYS,GAINESVILLE,FL 32611
关键词
D O I
10.1007/BF02102015
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Classical gravitation on de Sitter space suffers from a linearization instability. One consequence is that the causal response to a spatially localized distribution of positive energy cannot be globally regular. We use this fact to show that no causal Green's function can give the correct linearized response to certain bilocalized distributions, even though these distributions obey the constraints of linearization stability. We avoid the problem by working on the open submanifold spanned by conformal coordinates. The retarded Green's function is first computed in a simple gauge, then the rest of the propagator is inferred by analyticity - up to the usual ambiguity about real, analytic and homogeneous terms. We show that the latter can be chosen so as to give a propagator which does not grow in any direction. The ghost propagator is also given and the interaction vertices are worked out.
引用
收藏
页码:217 / 248
页数:32
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