The distance duality relation and the temperature profile of Galaxy Clusters
The distance duality relation and the temperature profile of Galaxy Clusters作者机构:Department of Astronomy Beijing Normal University Beijing 100875 China
出 版 物:《Science China(Physics,Mechanics & Astronomy)》 (中国科学:物理学、力学、天文学(英文版))
年 卷 期:2011年第54卷第12期
页 面:2260-2264页
核心收录:
学科分类:080903[工学-微电子学与固体电子学] 07[理学] 0809[工学-电子科学与技术(可授工学、理学学位)] 08[工学] 070104[理学-应用数学] 0805[工学-材料科学与工程(可授工学、理学学位)] 0704[理学-天文学] 0701[理学-数学]
基 金:supported by the National Natural Science Foundation of China under the Distinguished Young Scholar (Grant Nos.10825313 and 11073005) the Ministry of Science and Technology National Basic Science Program (Project 973) (Grant No.2012CB821804) the Fundamental Research Funds for the Central Universities Scientific Research Foundation of Beijing Normal University
主 题:X rays: galaxies: clusters (cosmology:) distance scale cosmology: miscellaneous
摘 要:The validity of distance duality relation, η = D L (z)(1 + z) 2 /D A (z) = 1, an exact result required by the Etherington reciprocity theorem, where D A (z) and D L (z) are the angular and luminosity distances, plays an essential part in cosmological observations and model constraints. In this paper, we investigate some consequences of such a relation by assuming η a constant or a function of the redshift. In order to constrain the parameters concerning η, we consider two groups of cluster gas mass fraction data including 52 X-ray luminous galaxy clusters observed by Chandra in the redshift range from 0.3 to 1.273 and temperature range T gas 4 keV, under the assumptions of two different temperature profiles. We find that the constant temperature profile is in relatively good agreement with no violation of the distance duality relation for both parameterizations of η, while the one with temperature gradient (the Vikhlinin et al. temperature profile) seems to be incompatible even at 99% CL.