Ghost-free massive gravity with a general reference metric

被引:309
作者
Hassan, S. F. [1 ,2 ]
Rosen, Rachel A. [3 ,4 ]
Schmidt-May, Angnis [1 ,2 ]
机构
[1] Stockholm Univ, AlbaNova Univ Ctr, Dept Phys, SE-10691 Stockholm, Sweden
[2] Stockholm Univ, AlbaNova Univ Ctr, Oskar Klein Ctr, SE-10691 Stockholm, Sweden
[3] Columbia Univ, Dept Phys, New York, NY 10027 USA
[4] Columbia Univ, Inst Strings Cosmol & Astroparticle Phys, New York, NY 10027 USA
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2012年 / 02期
基金
瑞典研究理事会;
关键词
Classical Theories of Gravity; Cosmology of Theories beyond the SM; VELTMAN-ZAKHAROV DISCONTINUITY; FINITE-RANGE; FIELD-THEORY; EQUATIONS; SPACE;
D O I
10.1007/JHEP02(2012)026
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
Theories of massive gravity inevitably include an auxiliary reference metric. Generically, they also contain an inconsistency known as the Boulware-Deser ghost. Recently, a family of non-linear massive gravity actions, formulated with a flat reference metric, were proposed and shown to be ghost free at the complete non-linear level. In this paper we consider these non-linear massive gravity actions but now formulated with a general reference metric. We extend the proof of the absence of the Boulware-Deser ghost to this case. The analysis is carried out in the ADM formalism at the complete non-linear level. We show that in these models there always exists a Hamiltonian constraint which, with an associated secondary constraint, eliminates the ghost. This result considerably extends the range of known consistent non-linear massive gravity theories. In addition, these theories can also be used to describe a massive spin-2 field in an arbitrary, fixed gravitational background. We also discuss the positivity of the Hamiltonian.
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页数:26
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