AN EXPANDING 4D UNIVERSE IN A 5D KALUZA-KLEIN COSMOLOGY WITH HIGHER DIMENSIONAL MATTER

被引:0
|
作者
Darabi, F. [1 ,2 ]
机构
[1] Azarbaijan Univ Tarbiat Moallem, Dept Phys, Tabriz 53714161, Iran
[2] Res Inst Astron & Astrophys Maraghaa, Maragha 5134441, Iran
关键词
Dark pressure; accelerating universe; non-compact Kaluza-Klein cosmology; PROBE WMAP OBSERVATIONS; MODIFIED GRAVITY; DARK ENERGY; INFLATIONARY COSMOLOGY; INVERSE POWERS; MODELS; QUINTESSENCE; EVOLUTION; EXPANSION; CONSTANT;
D O I
10.1142/S0217732310032743
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the framework of Kaluza-Klein theory, we investigate a (4 + 1)-dimensional universe consisting of a (4 + 1)-dimensional Robertson-Walker type metric coupled with a (4 + 1)dimensional energy-momentum tensor. The matter part consists of an energy density together with a pressure subject to 4D part of the (4 + 1)-dimensional energy-momentum tensor. The dark part consists of just a dark pressure (p) over bar, corresponding to the extra-dimension endowed by a scalar field, with no element of dark energy. It is shown that the reduced Einstein field equations are free of 4D pressure and are just affected by an effective pressure produced by the 4D energy density and dark pressure. It is then proposed that the expansion of the universe may be controlled by the equation of state in higher dimension rather than four dimensions. This may account for the current acceleration at the beginning or in the middle of matter dominant era.
引用
收藏
页码:1635 / 1646
页数:12
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