中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Revisiting the event rate of short GRBs and estimating their detectable number within the Advanced LIGO horizon

文献类型:期刊论文

作者Liu, Hao-Yang; Yu, Yun-Wei
刊名Research in Astronomy and Astrophysics
出版日期2019
卷号19期号:8页码:118
ISSN号1674-4527
DOI10.1088/1674-4527/19/8/118
文献子类Journal article (JA)
英文摘要The redshift and luminosity distributions of 36 Swift short gamma-ray bursts (GRBs) are fitted by connecting their event rates with cosmic star formation rates using power-law distributed delay times , where a broken-power-law luminosity function is assumed and some empirical observational selection effects are taken into account. As a result, the most-likely model parameters are constrained to be , as power-law indices, with a break at erg s?1 for the luminosity function and Gyr for a typical gravitational wave decay timescale of the binary orbit. The corresponding local rate of short GRBs is found to be . With these parameters, the detectable numbers of short GRBs are estimated within the horizon of Advanced LIGO.
语种英语
源URL[http://ir.ihep.ac.cn/handle/311005/287856]  
专题引力波暴高能电磁对应体全天监测器(GECAM)
推荐引用方式
GB/T 7714
Liu, Hao-Yang,Yu, Yun-Wei. Revisiting the event rate of short GRBs and estimating their detectable number within the Advanced LIGO horizon[J]. Research in Astronomy and Astrophysics,2019,19(8):118.
APA Liu, Hao-Yang,&Yu, Yun-Wei.(2019).Revisiting the event rate of short GRBs and estimating their detectable number within the Advanced LIGO horizon.Research in Astronomy and Astrophysics,19(8),118.
MLA Liu, Hao-Yang,et al."Revisiting the event rate of short GRBs and estimating their detectable number within the Advanced LIGO horizon".Research in Astronomy and Astrophysics 19.8(2019):118.

入库方式: OAI收割

来源:高能物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。