Bimetric structure formation: Non-Gaussian predictions

被引:27
作者
Magueijo, Joao [1 ]
Noller, Johannes [1 ]
Piazza, Federico [2 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BZ, England
[2] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 04期
基金
加拿大自然科学与工程研究理事会;
关键词
PRE-BIG-BANG; INFLATIONARY UNIVERSE; PERTURBATIONS; FLATNESS; SCENARIO; HORIZON; MODEL;
D O I
10.1103/PhysRevD.82.043521
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The minimal bimetric theory employing a disformal transformation between matter and gravity metrics is known to produce exactly scale-invariant fluctuations. It has a purely equilateral non-Gaussian signal, with an amplitude smaller than that of Dirac Born Infeld inflation (with opposite sign) but larger than standard inflation. We consider nonminimal bimetric models, where the coupling B appearing in the disformal transformation (g) over cap (mu nu) = g(mu nu) - B partial derivative(mu)phi partial derivative(nu)phi can run with phi. For power-law B(phi) these models predict tilted spectra. For each value of the spectral index, a distinctive distortion to the equilateral property can be found. The constraint between this distortion and the spectral index can be seen as a "consistency relation" for nonminimal bimetric models.
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页数:9
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