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刘宏亚

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期刊论文

Three Components Evolution in a Simple Big Bounce Cosmological Model

刘宏亚Lixin XuHongya Liu

September 11, 2007 11:24 WSPC/INSTRUCTION FILE IJMPD,-0001,():

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摘要/描述

We consider a five-dimensional Ricci flat Bouncing cosmology and assume that the four-dimensional universe is permeated smoothly by three minimally coupled matter compo-nents:CDM+baryons ρm, radiation ρr and dark energy ρx.Evolutions of these three components are studied and it is found that dark energy dominates before the bounce,and pulls the universe contracting. In this process,dark energy decreases while radi-ation and the matter increase.After the bounce, the radiation and matter dominates alternatively and then decrease with the expansion of the universe.At present,the dark energy dominates again and pushes the universe accelerating. In this model,we also obtain that the equation of state (EOS) of dark energy at present time is wx0≈−1.05 and the redshift of the transition from decelerated expansion to accelerated expansion is zT≈0.37,which are compatible with the current observations.

【免责声明】以下全部内容由[刘宏亚]上传于[2007年09月12日 15时37分26秒],版权归原创者所有。本文仅代表作者本人观点,与本网站无关。本网站对文中陈述、观点判断保持中立,不对所包含内容的准确性、可靠性或完整性提供任何明示或暗示的保证。请读者仅作参考,并请自行承担全部责任。

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