中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Natural Explanation for 21 cm Absorption Signals via Axion-Induced Cooling

文献类型:期刊论文

作者Houston, Nick1; Li, Chuang1,2; Li, Tianjun1,2; Yang, Qiaoli3; Zhang, Xin4,5
刊名PHYSICAL REVIEW LETTERS
出版日期2018-09-13
卷号121期号:11页码:6
ISSN号0031-9007
DOI10.1103/PhysRevLett.121.111301
英文摘要The EDGES Collaboration has reported an anomalously strong 21 cm absorption feature corresponding to the era of first star formation, which may indirectly betray the influence of dark matter during this epoch. We demonstrate that, by virtue of the ability to mediate cooling processes while in the condensed phase, a small amount of axion dark matter can explain these observations within the context of standard models of axions and axionlike particles. The EDGES best-fit result favors an axionlike particle mass in the (10, 450) meV range, which can be compressed for the QCD axion to (100, 450) meV in the absence of fine tuning. Future experiments and large scale surveys, particularly the International Axion Observatory (IAXO) and EUCLID, should have the capability to directly test this scenario.
WOS关键词CP INVARIANCE ; PARTICLES
资助项目CAS President's International Fellowship ; National Natural Science Foundation of China[11475238] ; National Natural Science Foundation of China[11647601] ; National Natural Science Foundation of China[11875062] ; National Natural Science Foundation of China[11875148] ; Key Research Program of Frontier Science, CAS
WOS研究方向Physics
语种英语
WOS记录号WOS:000444614800004
出版者AMER PHYSICAL SOC
资助机构CAS President's International Fellowship ; CAS President's International Fellowship ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of Frontier Science, CAS ; Key Research Program of Frontier Science, CAS ; CAS President's International Fellowship ; CAS President's International Fellowship ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of Frontier Science, CAS ; Key Research Program of Frontier Science, CAS ; CAS President's International Fellowship ; CAS President's International Fellowship ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of Frontier Science, CAS ; Key Research Program of Frontier Science, CAS ; CAS President's International Fellowship ; CAS President's International Fellowship ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of Frontier Science, CAS ; Key Research Program of Frontier Science, CAS
源URL[http://ir.bao.ac.cn/handle/114a11/22746]  
专题中国科学院国家天文台
通讯作者Houston, Nick; Li, Chuang; Li, Tianjun; Yang, Qiaoli; Zhang, Xin
作者单位1.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
2.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China
3.Jinan Univ, Phys Dept, Siyuan Lab, Guangzhou 510632, Guangdong, Peoples R China
4.Chinese Acad Sci, Natl Astron Observ, Key Lab Computat Astrophys, 20A Datun Rd, Beijing 100012, Peoples R China
5.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
推荐引用方式
GB/T 7714
Houston, Nick,Li, Chuang,Li, Tianjun,et al. Natural Explanation for 21 cm Absorption Signals via Axion-Induced Cooling[J]. PHYSICAL REVIEW LETTERS,2018,121(11):6.
APA Houston, Nick,Li, Chuang,Li, Tianjun,Yang, Qiaoli,&Zhang, Xin.(2018).Natural Explanation for 21 cm Absorption Signals via Axion-Induced Cooling.PHYSICAL REVIEW LETTERS,121(11),6.
MLA Houston, Nick,et al."Natural Explanation for 21 cm Absorption Signals via Axion-Induced Cooling".PHYSICAL REVIEW LETTERS 121.11(2018):6.

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来源:国家天文台

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