Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
文献类型：期刊论文
| 作者 | Yuan, Weimin1 ; Amati, Lorenzo2; Cannizzo, John K.3; Cordier, Bertrand4; Gehrels, Neil5; Ghirlanda, Giancarlo6; Gotz, Diego4; Produit, Nicolas7; Qiu, Yulei1; Sun, Jianchao8
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| 刊名 | SPACE SCIENCE REVIEWS
 |
| 出版日期 | 2016-12-01 |
| 卷号 | 202期号:1-4页码:235-277 |
| 关键词 | Gamma-ray bursts High-redshift Gamma-ray X-ray Instrumentation |
| 英文摘要 | 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. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | 28 FEBRUARY 1997 ; HIGH-REDSHIFT ; GRB 130427A ; OPTICAL AFTERGLOWS ; RADIO AFTERGLOW ; COMPLETE SAMPLE ; REVERSE-SHOCK ; EMISSION ; CALORIMETRY ; POPULATION |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000388982800010 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6834]  |
| 专题 | 国家天文台_空间科学研究部 |
| 作者单位 | 1.Chinese Acad Sci, Key Lab Space Astron & Technol, Natl Astron Observ, Datun Rd 20A, Beijing 100012, Peoples R China 2.INAF IASF Bologna, Via P Gobetti 101, I-40129 Bologna, Italy 3.Univ Maryland Baltimore Cty, CRESST Joint Ctr Astrophys, Baltimore, MD 21250 USA 4.CEA Irfu, Serv Astrophys, F-91191 Gif Sur Yvette, France 5.NASA, Goddard Space Flight Ctr, Div Astrophys, Greenbelt, MD 20771 USA 6.Ist Nazl Astrofis INAF, Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, LC, Italy 7.ISDC, Chemin Ecogia 16, CH-1290 Versoix, Switzerland 8.Chinese Acad Sci, Inst High Energy Phys, Yuquan Lu 19B, Beijing, Peoples R China 9.Univ Leicester, Dept Phys & Astron, Univ Rd, Leicester LE1 7RH, Leics, England |
| 推荐引用方式 GB/T 7714 | Yuan, Weimin,Amati, Lorenzo,Cannizzo, John K.,et al. Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities[J]. SPACE SCIENCE REVIEWS,2016,202(1-4):235-277. |
| APA | Yuan, Weimin.,Amati, Lorenzo.,Cannizzo, John K..,Cordier, Bertrand.,Gehrels, Neil.,...&Zhang, Chen.(2016).Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities.SPACE SCIENCE REVIEWS,202(1-4),235-277. |
| MLA | Yuan, Weimin,et al."Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities".SPACE SCIENCE REVIEWS 202.1-4(2016):235-277. |
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来源：国家天文台
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