Covariant power-counting renormalizable gravity: Lorentz symmetry breaking and accelerating early-time FRW universe

被引:322
作者
Nojiri, Shinichi [1 ,2 ]
Odintsov, Sergei D. [3 ,4 ]
机构
[1] Nagoya Univ, Dept Phys, Nagoya, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Univ, Nagoya, Aichi 4648602, Japan
[3] Inst Ciencies Espai IEEC CSIC, Fac Ciencias, E-08193 Bellaterra, Barcelona, Spain
[4] ICREA, E-08193 Bellaterra, Barcelona, Spain
来源
PHYSICAL REVIEW D | 2011年 / 83卷 / 02期
关键词
DARK ENERGY;
D O I
10.1103/PhysRevD.83.023001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We continue the study of covariant power-counting renormalizable gravity constrained by a scalar Lagrange multiplier. Lorentz-symmetry breaking is investigated in such a theory in comparison with the one in the ghost condensation model. Covariant power-counting renormalizable vector gravity which is invariant under U(1) gauge symmetry is proposed. Several forms of vector Lagrange multiplier in this theory are discussed. It is shown that the covariant scalar/vector gravity under consideration may have a power-law or de Sitter accelerating cosmological solution corresponding to an inflationary era. The simplest black hole solution is obtained and dispersion relations for graviton are presented.
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页数:10
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