Dark energy： A brief review  

作　　者：Miao Li Xiao-Dong Li Shuang Wang Yi Wang 

机构地区：[1]Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China [2]Kavli Institute for Theoretical Physics, Key Laboratory of Frontiers in Theoretical Physics, Beijing 100190, China [3]Department of Modern Physics, University of Science and Technology of China, Heifei 230026, China [4]Interdisciplinary Center for Theoretical Study, University of Science and Technology of China, Hefei 230026, China [5]Department of Physics, College of Sciences, Northeastern University, Shenyang 110004, China [6]Homer L. Dodge Department of Physics Astronomy, Univ. of Oklahoma, W Brooks St., Norman, OK 73019, USA [7]Kavli Institute for the Physics and Mathematics of the Universe, Todai Institutes for Advanced Study, University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 27%8583, Japan [8]Department of Physics, McGill University, Montrdal, QC, H3A 2T8, Canada

出　　处：《Frontiers of physics》2013年第6期828-846,共19页物理学前沿（英文版）

基　　金：Acknowledgements This research was supported by the National Natural Science Foundation of China （Grant Nos. 10535060/A050207, 10975172, and 10821504） and Ministry of Science and Technology 973 Program under grant No. 2007CB815401. Yi Wang acknowledges support from grants from Kavli IPMU, McGill University, the Institute of Particle Physics （Canada） and the Foundational Questions Institute.

摘　　要：The problem of dark energy is briefly reviewed in both theoretical and observational aspects. In the theoretical aspect, dark energy scenarios are classified into symmetry, anthropie principle, tuning mechanism, modified gravity, quantum cosmology, holographic principle, back-reaction and phenomenologieal types. In the observational aspect, we introduce cosmic probes, dark energy related projects, observational constraints on theoretical models and model independent reconstructions.

关 键 词：dark energy THEORY OBSERVATION 

分 类 号：P145.9[天文地球—天体物理] P159.2[天文地球—天文学]