Healthy degenerate theories with higher derivatives

被引:145
|
作者
Motohashi, Hayato [1 ]
Noui, Karim [2 ,3 ]
Suyama, Teruaki [4 ]
Yamaguchi, Masahide [5 ]
Langlois, David [3 ]
机构
[1] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[2] Univ Tours, Lab Math & Phys Theor, Parc Grandmont, F-37200 Tours, France
[3] Univ Paris 07, Lab APC Astroparticule & Cosmol, F-75013 Paris, France
[4] Univ Tokyo, Grad Sch Sci, RESCEU, Tokyo 1130033, Japan
[5] Tokyo Inst Technol, Dept Phys, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528551, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2016年 / 07期
基金
日本学术振兴会;
关键词
modified gravity; dark energy theory; inflation;
D O I
10.1088/1475-7516/2016/07/033
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the context of classical mechanics, we study the conditions under which higher-order derivative theories can evade the so-called Ostrogradsky instability. More precisely, we consider general Lagrangians with second order time derivatives, of the form L(phi(a), phi(a), phi(a); q(i), q(j)) with a = 1,..., n and i = 1,...., m. For n = 1, assuming that the q(i,) s form a nondegenerate subsystem, we confirm that the degeneracy of the kinetic matrix eliminates the Ostrogradsky instability. The degeneracy implies, in the Hamiltonian formulation of the theory, the existence of a primary constraint, which generates a secondary constraint, thus eliminating the Ostrogradsky ghost. For n > 1, we show that, in addition to the degeneracy of the kinetic matrix, one needs to impose extra conditions to ensure the presence of a sufficient number of secondary constraints that can eliminate all the Ostrogradsky ghosts. When these conditions that ensure the disappearance of the Ostrogradsky instability are satisfied, we show that the Euler-Lagrange equations, which involve a priori higher order derivatives, can be reduced to a second order system.
引用
收藏
页数:28
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