Extra dimensions present a new flatness problem

被引:29
作者
Chung, DJH [1 ]
Kolb, EW
Riotto, A
机构
[1] Univ Michigan, Randall Lab Phys, Ann Arbor, MI 48109 USA
[2] NASA, Fermilab Astrophys Ctr, Fermi Natl Accelerator Lab, Batavia, IL 60510 USA
[3] Univ Chicago, Enrico Fermi Inst, Dept Astron & Astrophys, Chicago, IL 60637 USA
[4] Scuola Normale Super Pisa, I-56126 Pisa, Italy
[5] Ist Nazl Fis Nucl, I-56127 Pisa, Italy
来源
PHYSICAL REVIEW D | 2002年 / 65卷 / 08期
关键词
D O I
10.1103/PhysRevD.65.083516
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
There is no known fundamental reason to demand as a cosmological initial condition that the bulk possess an SO(3,1) isometry. On the contrary, one expects bulk curvature terms that violate the SO(3,1) isometry at early epochs, leading to a violation of Lorentz invariance on our brane. Demanding that the Lorentz noninvariant terms are small leads to a new "flatness" problem, not solved by the usual formulation of inflation for a class of braneworld solutions. Furthermore, unlike in four dimensions, the Lorentz violations induced from the bulk curvature cannot always be removed as the infrared cutoff is taken arbitrarily large. This means that the equivalence principle in higher dimensions does not guarantee the equivalence principle in dimensionally reduced theories. Near-future experiments are expected to severely constrain these Lorentz-violating "signatures" of extra dimensions.
引用
收藏
页码:835161 / 835169
页数:9
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