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科学家采用新的联合成像技术分析陨石以探究地球水的来源 快报文章
地球科学快报,2022年第22期
作者:  张树良
Microsoft Word(15Kb)  |  收藏  |  浏览/下载:696/0  |  提交时间:2022/11/25
combining neutrons and X-ray imaging  meteorite  Earth evolution  water  
Synthesis and properties of free-standing monolayer amorphous carbon 期刊论文
NATURE, 2020, 577 (7789) : 199-+
作者:  Toh, Chee-Tat;  Zhang, Hongji;  Lin, Junhao;  Mayorov, Alexander S.;  Wang, Yun-Peng;  Orofeo, Carlo M.;  Ferry, Darim Badur;  Andersen, Henrik;  Kakenov, Nurbek;  Guo, Zenglong;  Abidi, Irfan Haider;  Sims, Hunter;  Suenaga, Kazu;  Pantelides, Sokrates T.;  Ozyilmaz, Barbaros
收藏  |  浏览/下载:21/0  |  提交时间:2020/07/03

Bulk amorphous materials have been studied extensively and are widely used, yet their atomic arrangement remains an open issue. Although they are generally believed to be Zachariasen continuous random networks(1), recent experimental evidence favours the competing crystallite model in the case of amorphous silicon(2-4). In two-dimensional materials, however, the corresponding questions remain unanswered. Here we report the synthesis, by laser-assisted chemical vapour deposition(5), of centimetre-scale, free-standing, continuous and stable monolayer amorphous carbon, topologically distinct from disordered graphene. Unlike in bulk materials, the structure of monolayer amorphous carbon can be determined by atomic-resolution imaging. Extensive characterization by Raman and X-ray spectroscopy and transmission electron microscopy reveals the complete absence of long-range periodicity and a threefold-coordinated structure with a wide distribution of bond lengths, bond angles, and five-, six-, seven- and eight-member rings. The ring distribution is not a Zachariasen continuous random network, but resembles the competing (nano)crystallite model(6). We construct a corresponding model that enables density-functional-theory calculations of the properties of monolayer amorphous carbon, in accordance with observations. Direct measurements confirm that it is insulating, with resistivity values similar to those of boron nitride grown by chemical vapour deposition. Free-standing monolayer amorphous carbon is surprisingly stable and deforms to a high breaking strength, without crack propagation from the point of fracture. The excellent physical properties of this stable, free-standing monolayer amorphous carbon could prove useful for permeation and diffusion barriers in applications such as magnetic recording devices and flexible electronics.


  
Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2 期刊论文
NATURE, 2020, 577 (7788) : 39-+
作者:  Willis, J. P.;  Canning, R. E. A.;  Noordeh, E. S.;  Allen, S. W.;  King, A. L.;  Mantz, A.;  Morris, R. G.;  Stanford, S. A.;  Brammer, G.
收藏  |  浏览/下载:36/0  |  提交时间:2020/07/03

Galaxy clusters are the most massive virialized structures in the Universe and are formed through the gravitational accretion of matter over cosmic time(1). The discovery(2) of an evolved galaxy cluster at redshift z = 2, corresponding to a look-back time of 10.4 billion years, provides an opportunity to study its properties. The galaxy cluster XLSSC 122 was originally detected as a faint, extended X-ray source in the XMM Large Scale Structure survey and was revealed to be coincident with a compact over-density of galaxies(2) with photometric redshifts of 1.9 +/- 0.2. Subsequent observations3 at millimetre wavelengths detected a Sunyaev-Zel'  dovich decrement along the line of sight to XLSSC 122, thus confirming the existence of hot intracluster gas, while deep imaging spectroscopy from the European Space Agency'  s X-ray Multi-Mirror Mission (XMM-Newton) revealed(4) an extended, X-ray-bright gaseous atmosphere with a virial temperature of 60 million Kelvin, enriched with metals to the same extent as are local clusters. Here we report optical spectroscopic observations of XLSSC 122 and identify 37 member galaxies at a mean redshift of 1.98, corresponding to a look-back time of 10.4 billion years. We use photometry to determine a mean, dust-free stellar age of 2.98 billion years, indicating that star formation commenced in these galaxies at a mean redshift of 12, when the Universe was only 370 million years old. The full range of inferred formation redshifts, including the effects of dust, covers the interval from 7 to 13. These observations confirm that XLSSC 122 is a remarkably mature galaxy cluster with both evolved stellar populations in the member galaxies and a hot, metal-rich gas composing the intracluster medium.


  
Rock Characterization Using Gray-Level Co-Occurrence Matrix: An Objective Perspective of Digital Rock Statistics 期刊论文
WATER RESOURCES RESEARCH, 2019, 55 (3) : 1912-1927
作者:  Singh, Ankita;  Armstrong, Ryan T.;  Regenauer-Lieb, Klaus;  Mostaghimi, Peyman
收藏  |  浏览/下载:14/0  |  提交时间:2019/11/26
porous media  rock characterization  GLCM  image processing  X-ray imaging  computer vision  
Tracking CO2 Plumes in Clay-Rich Rock by Distributed Fiber Optic Strain Sensing (DFOSS): A Laboratory Demonstration 期刊论文
WATER RESOURCES RESEARCH, 2019, 55 (1) : 856-867
作者:  Zhang, Yi;  Xue, Ziqiu;  Park, Hyuck;  Shi, Ji-Quan;  Kiyama, Tamotsu;  Lei, Xinglin;  Sun, Yankun;  Liang, Yunfeng
收藏  |  浏览/下载:22/0  |  提交时间:2019/04/09
CO2 storage  deformation  strain  optical fiber strain sensing  X-ray CT imaging  reservoir monitoring