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A highly conserved core bacterial microbiota with nitrogen-fixation capacity inhabits the xylem sap in maize plants 期刊论文
Nature Communications, 2022
作者:  Zhang, Liyu;  Zhang, Meiling;  Huang, Shuyu;  Li, Lujun;  Gao, Qiang;  Wang, Yin;  Zhang, Shuiqing;  Huang, Shaomin;  Yuan, Liang;  Wen, Yanchen;  Liu, Kailou;  Yu, Xichu;  Li, Dongchu;  Zhang, Lu;  Xu, Xinpeng;  Wei, Hailei;  He, Ping;  Zhou, Wei;  Philippot, Laurent;  Ai, Chao
收藏  |  浏览/下载:15/0  |  提交时间:2022/06/24
Nonlinear interactions of land carbon cycle feedbacks in Earth System Models 期刊论文
Global Change Biology, 2021
作者:  Yuanyuan Huang;  Ying-Ping Wang;  Tilo Ziehn
收藏  |  浏览/下载:11/0  |  提交时间:2021/11/15
Global health effects of future atmospheric mercury emissions 期刊论文
Nature Communications, 2021
作者:  Yanxu Zhang;  Zhengcheng Song;  Shaojian Huang;  Peng Zhang;  Yiming Peng;  Peipei Wu;  Jing Gu;  Stephanie Dutkiewicz;  Huanxin Zhang;  Shiliang Wu;  Feiyue Wang;  Long Chen;  Shuxiao Wang;  Ping Li
收藏  |  浏览/下载:7/0  |  提交时间:2021/06/07
A small climate-amplifying effect of climate-carbon cycle feedback 期刊论文
Nature Communications, 2021
作者:  Xuanze Zhang;  Ying-Ping Wang;  Peter J. Rayner;  Philippe Ciais;  Kun Huang;  Yiqi Luo;  Shilong Piao;  Zhonglei Wang;  Jianyang Xia;  Wei Zhao;  Xiaogu Zheng;  Jing Tian;  Yongqiang Zhang
收藏  |  浏览/下载:14/0  |  提交时间:2021/06/07
Transferring hydrologic data across continents ‐‐ leveraging data‐rich regions to improve hydrologic prediction in data‐sparse regions 期刊论文
Water Resources Research, 2021
作者:  Kai Ma;  Dapeng Feng;  Kathryn Lawson;  Wen‐;  Ping Tsai;  Chuan Liang;  Xiaorong Huang;  Ashutosh Sharma;  Chaopeng Shen
收藏  |  浏览/下载:17/0  |  提交时间:2021/04/06
Stabilizing black-phase formamidinium perovskite formation at room temperature and high humidity 期刊论文
Science, 2021
作者:  Wei Hui;  Lingfeng Chao;  Hui Lu;  Fei Xia;  Qi Wei;  Zhenhuang Su;  Tingting Niu;  Lei Tao;  Bin Du;  Deli Li;  Yue Wang;  He Dong;  Shouwei Zuo;  Bixin Li;  Wei Shi;  Xueqin Ran;  Ping Li;  Hui Zhang;  Zhongbin Wu;  Chenxin Ran;  Lin Song;  Guichuan Xing;  Xingyu Gao;  Jing Zhang;  Yingdong Xia;  Yonghua Chen;  Wei Huang
收藏  |  浏览/下载:21/0  |  提交时间:2021/04/06
Network-based screen in iPSC-derived cells reveals therapeutic candidate for heart valve disease 期刊论文
Science, 2021
作者:  Christina V. Theodoris;  Ping Zhou;  Lei Liu;  Yu Zhang;  Tomohiro Nishino;  Yu Huang;  Aleksandra Kostina;  Sanjeev S. Ranade;  Casey A. Gifford;  Vladimir Uspenskiy;  Anna Malashicheva;  Sheng Ding;  Deepak Srivastava
收藏  |  浏览/下载:9/0  |  提交时间:2021/02/17
Simulation of Hubbard model physics in WSe2/WS2 moire superlattices 期刊论文
NATURE, 2020, 579 (7799) : 353-+
作者:  Stein, Reed M.;  Kang, Hye Jin;  McCorvy, John D.;  Glatfelter, Grant C.;  Jones, Anthony J.;  Che, Tao;  Slocum, Samuel;  Huang, Xi-Ping;  Savych, Olena;  Moroz, Yurii S.;  Stauch, Benjamin;  Johansson, Linda C.;  Cherezov, Vadim;  Kenakin, Terry;  Irwin, John J.;  Shoichet, Brian K.;  Roth, Bryan L.;  Dubocovich, Margarita L.
收藏  |  浏览/下载:8/0  |  提交时间:2020/07/03

Study of WSe2/WS2 moire superlattices reveals the phase diagram of the triangular-lattice Hubbard model, including a Mott insulating state at half-filling and a possible magnetic quantum phase transition near 0.6 filling.


The Hubbard model, formulated by physicist John Hubbard in the 1960s(1), is a simple theoretical model of interacting quantum particles in a lattice. The model is thought to capture the essential physics of high-temperature superconductors, magnetic insulators and other complex quantum many-body ground states(2,3). Although the Hubbard model provides a greatly simplified representation of most real materials, it is nevertheless difficult to solve accurately except in the one-dimensional case(2,3). Therefore, the physical realization of the Hubbard model in two or three dimensions, which can act as an analogue quantum simulator (that is, it can mimic the model and simulate its phase diagram and dynamics(4,5)), has a vital role in solving the strong-correlation puzzle, namely, revealing the physics of a large number of strongly interacting quantum particles. Here we obtain the phase diagram of the two-dimensional triangular-lattice Hubbard model by studying angle-aligned WSe2/WS2 bilayers, which form moire superlattices(6) because of the difference between the lattice constants of the two materials. We probe the charge and magnetic properties of the system by measuring the dependence of its optical response on an out-of-plane magnetic field and on the gate-tuned carrier density. At half-filling of the first hole moire superlattice band, we observe a Mott insulating state with antiferromagnetic Curie-Weiss behaviour, as expected for a Hubbard model in the strong-interaction regime(2,3,7-9). Above half-filling, our experiment suggests a possible quantum phase transition from an antiferromagnetic to a weak ferromagnetic state at filling factors near 0.6. Our results establish a new solid-state platform based on moire superlattices that can be used to simulate problems in strong-correlation physics that are described by triangular-lattice Hubbard models.


  
A lysosomal switch triggers proteostasis renewal in the immortal C. elegans germ lineage (vol 551, pg 629, 2017) 期刊论文
NATURE, 2020, 580 (7802) : E5-E5
作者:  Lu, Zhihao;  Zou, Jianling;  Li, Shuang;  Topper, Michael J.;  Tao, Yong;  Zhang, Hao;  Jiao, Xi;  Xie, Wenbing;  Kong, Xiangqian;  Vaz, Michelle;  Li, Huili;  Cai, Yi;  Xia, Limin;  Huang, Peng;  Rodgers, Kristen;  Lee, Beverly;  Riemer, Joanne B.;  Day, Chi-Ping;  Yen, Ray-Whay Chiu;  Cui, Ying;  Wang, Yujiao;  Wang, Yanni;  Zhang, Weiqiang;  Easwaran, Hariharan;  Hulbert, Alicia;  Kim, KiBem;  Juergens, Rosalyn A.;  Yang, Stephen C.;  Battafarano, Richard J.;  Bush, Errol L.;  Broderick, Stephen R.;  Cattaneo, Stephen M.;  Brahmer, Julie R.;  Rudin, Charles M.;  Wrangle, John;  Mei, Yuping;  Kim, Young J.;  Zhang, Bin;  Wang, Ken Kang-Hsin;  Forde, Patrick M.;  Margolick, Joseph B.;  Nelkin, Barry D.;  Zahnow, Cynthia A.;  Pardoll, Drew M.;  Housseau, Franck;  Baylin, Stephen B.;  Shen, Lin;  Brock, Malcolm V.
收藏  |  浏览/下载:26/0  |  提交时间:2020/07/03
Nightside condensation of iron in an ultrahot giant exoplanet 期刊论文
NATURE, 2020, 580 (7805) : 597-+
作者:  Lu, Zhihao;  Zou, Jianling;  Li, Shuang;  Topper, Michael J.;  Tao, Yong;  Zhang, Hao;  Jiao, Xi;  Xie, Wenbing;  Kong, Xiangqian;  Vaz, Michelle;  Li, Huili;  Cai, Yi;  Xia, Limin;  Huang, Peng;  Rodgers, Kristen;  Lee, Beverly;  Riemer, Joanne B.;  Day, Chi-Ping;  Yen, Ray-Whay Chiu;  Cui, Ying;  Wang, Yujiao;  Wang, Yanni;  Zhang, Weiqiang;  Easwaran, Hariharan;  Hulbert, Alicia;  Kim, KiBem;  Juergens, Rosalyn A.;  Yang, Stephen C.;  Battafarano, Richard J.;  Bush, Errol L.;  Broderick, Stephen R.;  Cattaneo, Stephen M.;  Brahmer, Julie R.;  Rudin, Charles M.;  Wrangle, John;  Mei, Yuping;  Kim, Young J.;  Zhang, Bin;  Wang, Ken Kang-Hsin;  Forde, Patrick M.;  Margolick, Joseph B.;  Nelkin, Barry D.;  Zahnow, Cynthia A.;  Pardoll, Drew M.;  Housseau, Franck;  Baylin, Stephen B.;  Shen, Lin;  Brock, Malcolm V.
收藏  |  浏览/下载:57/0  |  提交时间:2020/07/03

Ultrahot giant exoplanets receive thousands of times Earth'  s insolation(1,2). Their high-temperature atmospheres (greater than 2,000 kelvin) are ideal laboratories for studying extreme planetary climates and chemistry(3-5). Daysides are predicted to be cloud-free, dominated by atomic species(6) and much hotter than nightsides(5,7,8). Atoms are expected to recombine into molecules over the nightside(9), resulting in different day and night chemistries. Although metallic elements and a large temperature contrast have been observed(10-14), no chemical gradient has been measured across the surface of such an exoplanet. Different atmospheric chemistry between the day-to-night ('  evening'  ) and night-to-day ('  morning'  ) terminators could, however, be revealed as an asymmetric absorption signature during transit(4,7,15). Here we report the detection of an asymmetric atmospheric signature in the ultrahot exoplanet WASP-76b. We spectrally and temporally resolve this signature using a combination of high-dispersion spectroscopy with a large photon-collecting area. The absorption signal, attributed to neutral iron, is blueshifted by -11 +/- 0.7 kilometres per second on the trailing limb, which can be explained by a combination of planetary rotation and wind blowing from the hot dayside(16). In contrast, no signal arises from the nightside close to the morning terminator, showing that atomic iron is not absorbing starlight there. We conclude that iron must therefore condense during its journey across the nightside.


Absorption lines of iron in the dayside atmosphere of an ultrahot giant exoplanet disappear after travelling across the nightside, showing that the iron has condensed during its travel.