Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters
文献类型：期刊论文
| 作者 | Chang Z(常哲) ; Wu FQ(吴锋泉); Zhang X(张鑫); Chang, Z; Wu, FQ; Zhang X
|
| 刊名 | PHYSICS LETTERS B
 |
| 出版日期 | 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 |
| 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!. |
入库方式： OAI收割
来源：高能物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。