Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
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下一代设施对伽马射线暴物理和宇宙学的看法
DOI：
10.1007/s11214-016-0274-z
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发表时间：
2016-06
影响因子：
10.3
通讯作者：
Chen Zhang
中科院分区：
文献类型：
--
作者：
Weimin Yuan;Lorenzo Amati;John K. Cannizzo;Bertr;Cordier;Neil Gehrels;Giancarlo Ghirl;a;Diego Götz;Nicolas Produit;Yulei Qiu;Jianchao Sun;Nial R. Tanvir;Jianyan Wei;Chen Zhang
红移~6以上的高红移伽玛射线暴（GRB）是探测遥远早期宇宙的潜在有力工具。它们的大量探测和真正的高红移要求下一代高能宽场仪器具有前所未有的灵敏度，至少比目前轨道上的仪器高一个数量级。另一方面，对高红移伽玛暴的余辉进行后续观测并识别其宿主星系，这对于目前正在运行的望远镜来说是困难的，需要新的，非常大的多波长设施。本章介绍了未来的实验，预计将推进这一令人兴奋的领域，目前正在建设和正在提出。Swift的遗产将由SVOM继续，SVOM配备了一套天基多波长仪器以及地面部分，包括一个广角相机和两个后续望远镜。已建立的龙虾眼X射线聚焦光学系统为探测超远距离的微弱伽玛暴提供了一种很有前途的技术，在此基础上提出了THESEUS、Einstein探测器和其他使命概念。射电SKA、光学/近红外30 m级望远镜、光学/近红外/中红外WFIRST和JWST等大型装置将为后续再电离期的观测和探索提供条件，此外还介绍了X射线和γ射线偏振实验POLAR。
High-redshift Gamma-Ray Bursts (GRBs) beyond redshift ~6 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 γ-ray polarization experiment POLAR is also introduced.
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DOI：
10.1111/j.1365-2966.2008.13736.x
发表时间：
2007-11
影响因子：
4.8
作者：
E. Rossi;R. Perna;F. Daigne
通讯作者：
E. Rossi;R. Perna;F. Daigne
DOI：
10.1088/0004-637x/736/1/7
发表时间：
2011-05
期刊：
The Astrophysical Journal
影响因子：
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作者：
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通讯作者：
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DOI：
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发表时间：
2007
期刊：
--
影响因子：
--
作者：
通讯作者：
--
DOI：
10.1098/rsta.2006.1992
发表时间：
2007-01
期刊：
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
影响因子：
--
作者：
N. Tanvir;P. Jakobsson
通讯作者：
N. Tanvir;P. Jakobsson
DOI：
10.1117/12.2055507
发表时间：
2014-06
期刊：
--
影响因子：
--
作者：
O. Godet;G. Nasser;J. Atteia;B. Cordier;P. Mandrou;D. Barret;H. Triou;R. Pons;C. Amoros;S. Bordon;O. Gevin;F. Gonzalez;D. Gotz;A. Gros;B. Houret;C. Lachaud;K. Lacombe;W. Marty;K. Mercier;D. Rambaud;P. Ramon;G. Rouaix;S. Schanne;V. Waegebaert
通讯作者：
O. Godet;G. Nasser;J. Atteia;B. Cordier;P. Mandrou;D. Barret;H. Triou;R. Pons;C. Amoros;S. Bordon;O. Gevin;F. Gonzalez;D. Gotz;A. Gros;B. Houret;C. Lachaud;K. Lacombe;W. Marty;K. Mercier;D. Rambaud;P. Ramon;G. Rouaix;S. Schanne;V. Waegebaert