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Redshift evolution of the Amati relation: Calibrated results from the Hubble diagram of quasars at high redshifts

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成果类型:
期刊论文
作者:
Dai, Yan;Zheng, Xiao-Gang;Li, Zheng-Xiang;Gao, He;Zhu, Zong-Hong
作者机构:
[Dai, Yan; Li, Zheng-Xiang; Gao, He; Zhu, Zong-Hong] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China.
[Dai, Yan] Beijing Planetarium, Beijing 100044, Peoples R China.
[Zheng, Xiao-Gang] Wuhan Polytech Univ, Sch Elect & Elect Engn, Wuhan 430023, Peoples R China.
语种:
英文
关键词:
gravitational waves;stars: neutron;stars: oscillations;quasars: general
期刊:
ASTRONOMY AND ASTROPHYSICS
ISSN:
0004-6361
年:
2021
卷:
651
基金类别:
National Natural Science Foundation of ChinaNational Natural Science Foundation of China (NSFC) [11633001, 11920101003, 12021003, 11690024]; Strategic Priority Research Program of the Chinese Academy of SciencesChinese Academy of Sciences [XDB23000000]; Interdiscipline Research Funds of Beijing Normal University
机构署名:
本校为其他机构
院系归属:
电气与电子工程学院
摘要:
Gamma-ray bursts (GRBs) have long been proposed as a complementary probe to type Ia supernovae (SNe Ia) and the cosmic microwave background to explore the expansion history of the high-redshift universe, mainly because they are bright enough to be detected at greater distances. Although they lack definite physical explanations, many empirical correlations between GRB isotropic energy or luminosity and some directly detectable spectral or temporal properties have been proposed to make GRBs standard candles. Since the observed GRB rate falls off ...

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