CONSEQUENCES OF PROPAGATING TORSION IN CONNECTION-DYNAMIC THEORIES OF GRAVITY

被引:79
|
作者
CARROLL, SM
FIELD, GB
机构
[1] MIT,DEPT PHYS,CAMBRIDGE,MA 02139
[2] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138
来源
PHYSICAL REVIEW D | 1994年 / 50卷 / 06期
关键词
D O I
10.1103/PhysRevD.50.3867
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the possibility of constraining theories of gravity in which the connection is a fundamental variable by searching for observational consequences of the torsion degrees of freedom. In a wide class of models, the only modes of the torsion tenser which interact with matter are either a massive scalar or a massive spin-1 boson. Focusing on the scalar version, we study constraints on the two-dimensional parameter space characterizing the theory. For reasonable choices of these parameters the torsion decays quickly into matter fields, and no long-range fields are generated which could be discovered by ground-based or astrophysical experiments.
引用
收藏
页码:3867 / 3873
页数:7
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