No de Sitter Invariant Vacuum in Massive Gravity Theory with Ghost

被引:17
作者
Izumi, Keisuke [1 ]
Tanaka, Takahiro [2 ]
机构
[1] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
[2] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
来源
PROGRESS OF THEORETICAL PHYSICS | 2009年 / 121卷 / 02期
关键词
FIELD-THEORY;
D O I
10.1143/PTP.121.419
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper, we point out that the massive gravity theory with a graviton ghost mode in the de Sitter background cannot possess a de Sitter invariant vacuum state. In order to avoid a negative norm state, we must associate the creation operator of the ghost mode with a negative-energy mode function instead of a positive-energy one as the mode function. Namely, we have to adopt a different procedure of quantization for a ghost. When a theory has a symmetry mixing a ghost mode with ordinary nonghost modes, the choice of a ghost mode is not unique. However, the quantization of a ghost is impossible without specifying a choice of ghost mode, which breaks the symmetry. For this reason, the vacuum state cannot respect the symmetry. In the massive gravity theory with a graviton ghost mode in the de Sitter background, the ghost is the helicity-0 mode of the graviton. This ghost mode is mixed with the other helicity graviton modes tinder the action of de Sitter symmetry. Therefore, there is no de Sitter invariant vacuum in such models. This leads to an interesting possibility that the non-covariant cutoff of the low-energy effective theory may naturally arise. As a result, the instability due to the pair production of a ghost and normal non-ghost particles gets much milder and that the model may escape from being rejected.
引用
收藏
页码:419 / 426
页数:8
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