A late-accelerating universe with no dark energy - and a finite-temperature big bang

被引:67
作者
Brown, RA [1 ]
Maartens, R
Papantonopoulos, E
Zamarias, V
机构
[1] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
[2] Natl Tech Univ Athens, Dept Phys, GR-15773 Athens, Greece
关键词
cosmology with extra dimensions; string theory and cosmology; physics of the early universe;
D O I
10.1088/1475-7516/2005/11/008
中图分类号
P1 [天文学];
学科分类号
0704 [天文学];
摘要
Brane-world models off. er the possibility of explaining the late acceleration of the universe via infra-red modifications to general relativity, rather than a dark energy field. However, one also expects ultra-violet modifications to general relativity, when high-energy stringy effects in the early universe begin to grow. We generalize the DGP brane-world model via an ultra-violet modi. cation, in the form of a Gauss-Bonnet term in the bulk action. The combination of infrared and ultra-violet modifications produces an intriguing cosmology. The DGP feature of late-time acceleration without dark energy is preserved, but there is an entirely new feature-there is no infinite-temperature big bang in the early universe. The universe starts with finite density and pressure, from a 'quiet' and 'sudden' curvature singularity.
引用
收藏
页码:131 / 143
页数:13
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