Cosmology of generalized modified gravity models - art. no. 065313

被引:547
作者
Carroll, SM
De Felice, A
Duvvuri, V
Easson, DA
Trodden, M
Turner, MS
机构
[1] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 USA
[2] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[3] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA
[4] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA
[5] Fermilab Natl Accelerator Lab, NASA Fermilab Astrophys Ctr, Batavia, IL 60510 USA
来源
PHYSICAL REVIEW D | 2005年 / 71卷 / 06期
关键词
D O I
10.1103/PhysRevD.71.063513
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider general curvature-invariant modifications of the Einstein-Hilbert action that become important only in regions of extremely low space-time curvature. We investigate the far future evolution of the Universe in such models, examining the possibilities for cosmic acceleration and other ultimate destinies. The models generically possess de Sitter space as an unstable solution and exhibit an interesting set of attractor solutions which, in some cases, provide alternatives to dark energy models.
引用
收藏
页码:1 / 11
页数:11
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