THE FRAGILITY AND RIGIDITY OF COSMOLOGICAL THEORIES

被引:13
作者
LIDSEY, JE
机构
[1] Theoretical Astronomy Unit, School of Mathematical Sciences, Queen Mary and Westfield, London, E1 4NS, Mile End Road
关键词
D O I
10.1007/BF00757120
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The concepts of fragility and rigidity in theories containing a minimally coupled, self-interacting scalar field are introduced and defined for an arbitrary space-time dimension, D, by using the field as the dynamical variable. It is proved that inflation is rigid and the case of an exponential self-interaction is studied. The fragility of higher-order, scalar-tensor and Kaluza-Klein gravity theories is investigated by using their conformal equivalence to general relativity plus a scalar field. Whilst most higher-order theories are rigid, the conditions for Kaluza-Klein theories to become fragile depend strongly on D.
引用
收藏
页码:399 / 407
页数:9
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