Forecast of cosmological constraints with superluminous supernovae from the Chinese Space Station Telescope

被引：1

作者：

Jia, Xuan-Dong ^{[1
]}

Hu, Jian-Ping ^{[1
]}

Wang, Fa-Yin ^{[1
,2
]}

Dai, Zi-Gao ^{[3
]}

机构：

[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China

[2] Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Peoples R China

[3] Univ Sci & Technol China, Dept Astron, Hefei 230026, Peoples R China

来源：

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2024年 / 67卷 / 10期

基金：

中国国家自然科学基金;

关键词：

supernovae; cosmology; cosmological constant; GAMMA-RAY BURSTS; LIGHT CURVES; HUBBLE CONSTANT; LOCAL VALUE; REDSHIFT; TRANSITION; SIGNATURE; GALAXIES; UNIVERSE; QUASARS;

D O I：

10.1007/s11433-024-2425-8

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Superluminous supernovae (SLSNe) are a class of intense celestial events that can be standardized for measuring cosmological parameters, bridging the gap between type Ia supernovae and the cosmic microwave background. In this work, we discuss the cosmological applications of SLSNe from the Chinese Space Station Telescope (CSST). Our estimation suggests that SLSNe rate is biased tracing the cosmic star formation rate, exhibiting a factor of (1 + z)1.2. We futher predict that CSST is poised to observe similar to 360 SLSNe in the 10 square degrees ultra-deep field survey within a span of 2.5 years. A stringent constraint on cosmological parameters can be derived from their peak-color relationship. CSST is anticipated to uncover a substantial number of SLSNe, contributing to a deeper understanding of their central engines and shedding light on the nature of dark energy at high redshifts.

引用

页数：11

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