IHEP OpenIR  > 粒子天体物理中心
Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
Yuan, WM; Amati, L; Cannizzo, JK; Cordier, B; Gehrels, N; Ghirlanda, G; Gotz, D; Produit, N; Qiu, YL; Sun, JC; Tanvir, NR; Wei, JY; Zhang, C; Sun JC(孙建超)
2016
发表期刊SPACE SCIENCE REVIEWS
页码1-43
通讯作者孙建超
摘要High-redshift Gamma-Ray Bursts (GRBs) beyond redshift are potentially powerful tools to probe the distant early Universe. Their detections in large numbers and at truly high redshifts call for the next generation of high-energy wide-field instruments with unprecedented sensitivity at least one order of magnitude higher than the ones currently in orbit. On the other hand, follow-up observations of the afterglows of high-redshift GRBs and identification of their host galaxies, which would be difficult for the currently operating telescopes, require new, extremely large facilities of at multi-wavelengths. This chapter describes future experiments that are expected to advance this exciting field, both being currently built and being proposed. The legacy of Swift will be continued by SVOM, which is equipped with a set of space-based multi-wavelength instruments as well as and a ground segment including a wide angle camera and two follow-up telescopes. The established Lobster-eye X-ray focusing optics provides a promising technology for the detection of faint GRBs at very large distances, based on which the THESEUS, Einstein Probe and other mission concepts have been proposed. Follow-up observations and exploration of the reionization era will be enabled by large facilities such as SKA in the radio, the 30 m class telescopes in the optical/near-IR, and the space-borne WFIRST and JWST in the optical/near-IR/mid-IR. In addition, the X-ray and -ray polarization experiment POLAR is also introduced.
文章类型Review
关键词Gamma-ray bursts High-redshift Gamma-ray X-ray Instrumentation
DOI10.1007/s11214-016-0274-z
关键词[WOS]28 FEBRUARY 1997 ; HIGH-REDSHIFT ; GRB 130427A ; OPTICAL AFTERGLOWS ; RADIO AFTERGLOW ; COMPLETE SAMPLE ; REVERSE-SHOCK ; EMISSION ; CALORIMETRY ; POPULATION
语种英语
WOS记录号WOS:000388982800010
引用统计
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/260694
专题粒子天体物理中心
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Yuan, WM,Amati, L,Cannizzo, JK,et al. Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities[J]. SPACE SCIENCE REVIEWS,2016:1-43.
APA Yuan, WM.,Amati, L.,Cannizzo, JK.,Cordier, B.,Gehrels, N.,...&孙建超.(2016).Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities.SPACE SCIENCE REVIEWS,1-43.
MLA Yuan, WM,et al."Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities".SPACE SCIENCE REVIEWS (2016):1-43.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
20160713.pdf(6514KB)期刊论文作者接受稿限制开放CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Yuan, WM]的文章
[Amati, L]的文章
[Cannizzo, JK]的文章
百度学术
百度学术中相似的文章
[Yuan, WM]的文章
[Amati, L]的文章
[Cannizzo, JK]的文章
必应学术
必应学术中相似的文章
[Yuan, WM]的文章
[Amati, L]的文章
[Cannizzo, JK]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

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。