Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters

	Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
	Chang Z(常哲); Wu FQ(吴锋泉); Zhang X(张鑫); Chang, Z; Wu, FQ; Zhang X
刊名	PHYSICS LETTERS B
	2006
卷号	633 期号:1 页码:#REF!
通讯作者	Zhang X (reprint author), Chinese Acad Sci, Inst High Energy Phys, POB 918 4, Beijing 100049, Peoples R China.
英文摘要	We use the Chandra measurements of the X-ray gas mass fraction of 26 rich clusters released by Allen et al. to perform constraints on the holographic dark energy model. The constraints are consistent with those from other cosmological tests, especially with the results of a joint analysis of supernovae, cosmic microwave background, and large scale structure data. From this test, the holographic dark energy also tends to behave as a quintom-type dark energy. (c) 2005 Elsevier B.V All rights reserved.
学科主题	Physics
类目[WOS]	Physics, Multidisciplinary
收录类别	SCI
WOS记录号	WOS:000235098400003
公开日期	2016-05-03
内容类型	期刊论文
源URL	[http://ir.ihep.ac.cn/handle/311005/225502]
专题	高能物理研究所_理论物理室
推荐引用方式 GB/T 7714	Chang Z,Wu FQ,Zhang X,et al. Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters[J]. PHYSICS LETTERS B,2006,633(1):#REF!.
APA	常哲,吴锋泉,张鑫,Chang, Z,Wu, FQ,&Zhang X.(2006).Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters.PHYSICS LETTERS B,633(1),#REF!.
MLA	常哲,et al."Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters".PHYSICS LETTERS B 633.1(2006):#REF!.