Effective field theory of broken spatial diffeomorphisms

被引:23
作者
Lin, Chunshan [1 ,2 ]
Labun, Lance Z. [3 ,4 ,5 ]
机构
[1] Kyoto Univ, Yukawa Inst Theoret Phys, Sakyo Ku, Kitashirakawa Oiwakecho, Kyoto 6068502, Japan
[2] Univ Tokyo, Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan
[3] Univ Texas Austin, Dept Phys, 2515 Speedway,MS C1510, Austin, TX 78712 USA
[4] Natl Taiwan Univ, Dept Phys, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan
[5] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys LeCosPA, 1,Sec 4,Roosevelt Rd, Taipei 10617, Taiwan
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2016年 / 03期
关键词
Classical Theories of Gravity; Effective field theories; MASSIVE GRAVITY; SUPERNOVAE; INFLATION; UNIVERSE;
D O I
10.1007/JHEP03(2016)128
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the low energy effective theory describing gravity with broken spatial diffeomorphism invariance. In the unitary gauge, the Goldstone bosons associated with broken diffeomorphisms are eaten and the graviton becomes a massive spin-2 particle with 5 well-behaved degrees of freedom. In this gauge, the most general theory is built with the lowest dimension operators invariant under only temporal diffeomorphisms. Imposing the additional shift and SO(3) internal symmetries, we analyze the perturbations on a FRW background. At linear perturbation level, the observables of this theory are characterized by five parameters, including the usual cosmological parameters and one additional coupling constant for the symmetry-breaking scalars. In the de Sitter and Minkowski limit, the three Goldstone bosons are supermassive and can be integrated out, leaving two massive tensor modes as the only propagating degrees of freedom. We discuss several examples relevant to theories of massive gravity.
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页数:29
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