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A population of dust-enshrouded objects orbiting the Galactic black hole 期刊论文
NATURE, 2020, 577 (7790) : 337-+
作者:  Witze, Alexandra
收藏  |  浏览/下载:8/0  |  提交时间:2020/07/03

The central 0.1 parsecs of the Milky Way host a supermassive black hole identified with the position of the radio and infrared source Sagittarius A* (refs.(1,2)), a cluster of young, massive stars (the S stars3) and various gaseous features(4,5). Recently, two unusual objects have been found to be closely orbiting Sagittarius A*: the so-called G sources, G1 and G2. These objects are unresolved (having a size of the order of 100 astronomical units, except at periapse, where the tidal interaction with the black hole stretches them along the orbit) and they show both thermal dust emission and line emission from ionized gas(6-10). G1 and G2 have generated attention because they appear to be tidally interacting with the supermassive Galactic black hole, possibly enhancing its accretion activity. No broad consensus has yet been reached concerning their nature: the G objects show the characteristics of gas and dust clouds but display the dynamical properties of stellar-mass objects. Here we report observations of four additional G objects, all lying within 0.04 parsecs of the black hole and forming a class that is probably unique to this environment. The widely varying orbits derived for the six G objects demonstrate that they were commonly but separately formed.


  
A cold, massive, rotating disk galaxy 1.5 billion years after the Big Bang 期刊论文
NATURE, 2020, 581 (7808) : 269-+
作者:  Poplawski, Gunnar H. D.;  Kawaguchi, Riki;  Van Niekerk, Erna;  Lu, Paul;  Mehta, Neil;  Canete, Philip;  Lie, Richard;  Dragatsis, Ioannis;  Meves, Jessica M.;  Zheng, Binhai;  Coppola, Giovanni;  Tuszynski, Mark H.
收藏  |  浏览/下载:59/0  |  提交时间:2020/07/03

Massive disk galaxies like the Milky Way are expected to form at late times in traditional models of galaxy formation(1,2), but recent numerical simulations suggest that such galaxies could form as early as a billion years after the Big Bang through the accretion of cold material and mergers(3,4). Observationally, it has been difficult to identify disk galaxies in emission at high redshift(5,6) in order to discern between competing models of galaxy formation. Here we report imaging, with a resolution of about 1.3 kiloparsecs, of the 158-micrometre emission line from singly ionized carbon, the far-infrared dust continuum and the near-ultraviolet continuum emission from a galaxy at a redshift of 4.2603, identified by detecting its absorption of quasar light. These observations show that the emission arises from gas inside a cold, dusty, rotating disk with a rotational velocity of about 272 kilometres per second. The detection of emission from carbon monoxide in the galaxy yields a molecular mass that is consistent with the estimate from the ionized carbon emission of about 72 billion solar masses. The existence of such a massive, rotationally supported, cold disk galaxy when the Universe was only 1.5 billion years old favours formation through either cold-mode accretion or mergers, although its large rotational velocity and large content of cold gas remain challenging to reproduce with most numerical simulations(7,8).


A massive rotating disk galaxy was formed a mere 1.5 billion years after the Big Bang, a surprisingly short time after the origin of the Universe.


  
APOE4 leads to blood-brain barrier dysfunction predicting cognitive decline 期刊论文
NATURE, 2020, 581 (7806) : 70-+
作者:  Doherty, Tiarnan A. S.;  Winchester, Andrew J.;  Macpherson, Stuart;  Johnstone, Duncan N.;  Pareek, Vivek;  Tennyson, Elizabeth M.;  Kosar, Sofiia;  Kosasih, Felix U.;  Anaya, Miguel;  Abdi-Jalebi, Mojtaba;  Andaji-Garmaroudi, Zahra;  Wong, E. Laine;  Madeo, Julien;  Chiang, Yu-Hsien;  Park, Ji-Sang;  Jung, Young-Kwang;  Petoukhoff, Christopher E.;  Divitini, Giorgio;  Man, Michael K. L.;  Ducati, Caterina;  Walsh, Aron;  Midgley, Paul A.;  Dani, Keshav M.;  Stranks, Samuel D.
收藏  |  浏览/下载:25/0  |  提交时间:2020/07/03

Breakdown of the blood-brain barrier in individuals carrying the epsilon 4 allele of the APOE gene, but not the epsilon 3 allele, increases with and predicts cognitive impairment and is independent of amyloid beta or tau pathology.


Vascular contributions to dementia and Alzheimer'  s disease are increasingly recognized(1-6). Recent studies have suggested that breakdown of the blood-brain barrier (BBB) is an early biomarker of human cognitive dysfunction(7), including the early clinical stages of Alzheimer'  s disease(5,8-10). The E4 variant of apolipoprotein E (APOE4), the main susceptibility gene for Alzheimer'  s disease(11-14), leads to accelerated breakdown of the BBB and degeneration of brain capillary pericytes(15-19), which maintain BBB integrity(20-22). It is unclear, however, whether the cerebrovascular effects of APOE4 contribute to cognitive impairment. Here we show that individuals bearing APOE4 (with the epsilon 3/epsilon 4 or epsilon 4/epsilon 4 alleles) are distinguished from those without APOE4 (epsilon 3/epsilon 3) by breakdown of the BBB in the hippocampus and medial temporal lobe. This finding is apparent in cognitively unimpaired APOE4 carriers and more severe in those with cognitive impairment, but is not related to amyloid-beta or tau pathology measured in cerebrospinal fluid or by positron emission tomography(23). High baseline levels of the BBB pericyte injury biomarker soluble PDGFR beta(7,8) in the cerebrospinal fluid predicted future cognitive decline in APOE4 carriers but not in non-carriers, even after controlling for amyloid-beta and tau status, and were correlated with increased activity of the BBB-degrading cyclophilin A-matrix metalloproteinase-9 pathway(19) in cerebrospinal fluid. Our findings suggest that breakdown of the BBB contributes to APOE4-associated cognitive decline independently of Alzheimer'  s disease pathology, and might be a therapeutic target in APOE4 carriers.


  
Control and single-shot readout of an ion embedded in a nanophotonic cavity 期刊论文
NATURE, 2020, 580 (7802) : 201-+
作者:  Rollie, Clare;  Chevallereau, Anne;  Watson, Bridget N. J.;  Chyou, Te-yuan;  Fradet, Olivier;  McLeod, Isobel;  Fineran, Peter C.;  Brown, Chris M.;  Gandon, Sylvain;  Westra, Edze R.
收藏  |  浏览/下载:22/0  |  提交时间:2020/07/03

Distributing entanglement over long distances using optical networks is an intriguing macroscopic quantum phenomenon with applications in quantum systems for advanced computing and secure communication(1,2). Building quantum networks requires scalable quantum light-matter interfaces(1) based on atoms(3), ions(4) or other optically addressable qubits. Solid-state emitters(5), such as quantum dots and defects in diamond or silicon carbide(6-10), have emerged as promising candidates for such interfaces. So far, it has not been possible to scale up these systems, motivating the development of alternative platforms. A central challenge is identifying emitters that exhibit coherent optical and spin transitions while coupled to photonic cavities that enhance the light-matter interaction and channel emission into optical fibres. Rare-earth ions in crystals are known to have highly coherent 4f-4f optical and spin transitions suited to quantum storage and transduction(11-15), but only recently have single rare-earth ions been isolated(16,17) and coupled to nanocavities(18,19). The crucial next steps towards using single rare-earth ions for quantum networks are realizing long spin coherence and single-shot readout in photonic resonators. Here we demonstrate spin initialization, coherent optical and spin manipulation, and high-fidelity single-shot optical readout of the hyperfine spin state of single Yb-171(3+) ions coupled to a nanophotonic cavity fabricated in an yttrium orthovanadate host crystal. These ions have optical and spin transitions that are first-order insensitive to magnetic field fluctuations, enabling optical linewidths of less than one megahertz and spin coherence times exceeding thirty milliseconds for cavity-coupled ions, even at temperatures greater than one kelvin. The cavity-enhanced optical emission rate facilitates efficient spin initialization and single-shot readout with conditional fidelity greater than 95 per cent. These results showcase a solid-state platform based on single coherent rare-earth ions for the future quantum internet.


Single ytterbium ion qubits in nanophotonic cavities have long coherence times and can be optically read out in a single shot, establishing them as excellent candidates for optical quantum networks.


  
Direct-bandgap emission from hexagonal Ge and SiGe alloys 期刊论文
NATURE, 2020, 580 (7802) : 205-+
作者:  Meiners, Thorsten;  Frolov, Timofey;  Rudd, Robert E.;  Dehm, Gerhard;  Liebscher, Christian H.
收藏  |  浏览/下载:28/0  |  提交时间:2020/07/03

Silicon crystallized in the usual cubic (diamond) lattice structure has dominated the electronics industry for more than half a century. However, cubic silicon (Si), germanium (Ge) and SiGe alloys are all indirect-bandgap semiconductors that cannot emit light efficiently. The goal(1) of achieving efficient light emission from group-IV materials in silicon technology has been elusive for decades(2-6). Here we demonstrate efficient light emission from direct-bandgap hexagonal Ge and SiGe alloys. We measure a sub-nanosecond, temperature-insensitive radiative recombination lifetime and observe an emission yield similar to that of direct-bandgap group-III-V semiconductors. Moreover, we demonstrate that, by controlling the composition of the hexagonal SiGe alloy, the emission wavelength can be continuously tuned over a broad range, while preserving the direct bandgap. Our experimental findings are in excellent quantitative agreement with ab initio theory. Hexagonal SiGe embodies an ideal material system in which to combine electronic and optoelectronic functionalities on a single chip, opening the way towards integrated device concepts and information-processing technologies.


A hexagonal (rather than cubic) alloy of silicon and germanium that has a direct (rather than indirect) bandgap emits light efficiently across a range of wavelengths, enabling electronic and optoelectronic functionalities to be combined on a single chip.


  
Electrically pumped topological laser with valley edge modes 期刊论文
NATURE, 2020, 578 (7794) : 246-+
作者:  Erickson, Peter;  van Asselt, Harro;  Koplow, Doug;  Lazarus, Michael;  Newell, Peter;  Oreskes, Naomi;  Supran, Geoffrey
收藏  |  浏览/下载:46/0  |  提交时间:2020/07/03

Quantum cascade lasers are compact, electrically pumped light sources in the technologically important mid-infrared and terahertz region of the electromagnetic spectrum(1,2). Recently, the concept of topology(3) has been expanded from condensed matter physics into photonics(4), giving rise to a new type of lasing(5-8) using topologically protected photonic modes that can efficiently bypass corners and defects(4). Previous demonstrations of topological lasers have required an external laser source for optical pumping and have operated in the conventional optical frequency regime(5-8). Here we demonstrate an electrically pumped terahertz quantum cascade laser based on topologically protected valley edge states(9-11). Unlike topological lasers that rely on large-scale features to impart topological protection, our compact design makes use of the valley degree of freedom in photonic crystals(10,11), analogous to two-dimensional gapped valleytronic materials(12). Lasing with regularly spaced emission peaks occurs in a sharp-cornered triangular cavity, even if perturbations are introduced into the underlying structure, owing to the existence of topologically protected valley edge states that circulate around the cavity without experiencing localization. We probe the properties of the topological lasing modes by adding different outcouplers to the topological cavity. The laser based on valley edge states may open routes to the practical use of topological protection in electrically driven laser sources.


  
Night-sky radiometry can revolutionize the characterization of light-pollution sources globally 期刊论文
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2019, 116 (16) : 7712-7717
作者:  Kocifaj, Miroslav;  Antonio Solano-Lamphar, Hector;  Videen, Gorden
收藏  |  浏览/下载:5/0  |  提交时间:2019/11/27
skyglow  night-sky radiometry  light-pollution sources  upward emission function  
Severe haze in northern China: A synergy of anthropogenic emissions and atmospheric processes 期刊论文
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2019, 116 (18) : 8657-8666
作者:  An, Zhisheng;  Huang, Ru-Jin;  Zhang, Renyi;  Tie, Xuexi;  Li, Guohui;  Cao, Junji;  Zhou, Weijian;  Shi, Zhengguo;  Han, Yongming;  Gu, Zhaolin;  Ji, Yuemeng
收藏  |  浏览/下载:11/0  |  提交时间:2019/11/27
severe haze  synergetic effects  anthropogenic emission  atmospheric chemistry  climate change  
Anthropogenic drivers of 2013-2017 trends in summer surface ozone in China 期刊论文
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2019, 116 (2) : 422-427
作者:  Li, Ke;  Jacob, Daniel J.;  Liao, Hong;  Shen, Lu;  Zhang, Qiang;  Bates, Kelvin H.
收藏  |  浏览/下载:48/0  |  提交时间:2019/11/27
surface ozone  China  aerosol chemistry  emission reductions  air quality  
Drivers of improved PM2.5 air quality in China from 2013 to 2017 期刊论文
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2019
作者:  Qiang Zhang;  Yixuan Zheng;  Dan Tong;  Min Shao;  Shuxiao Wang;  Yuanhang Zhang;  Xiangde Xu;  Jinnan Wang;  Hong He;  Wenqing Liu;  Yihui Ding;  Yu Lei;  Junhua Li;  Zifa Wang;  Xiaoye Zhang;  Yuesi Wang;  Jing Cheng;  Yang Liu;  Qinren Shi;  Liu Yan;  Guannan Geng;  Chaopeng Hong;  Meng Li;  Fei Liu;  Bo Zheng;  Junji Cao;  Aijun Ding;  Jian Gao;  Qingyan Fu;  Juntao Huo;  Baoxian Liu;  Zirui Liu;  Fumo Yang;  Kebin He;  and Jiming Hao
收藏  |  浏览/下载:12/0  |  提交时间:2019/11/27
clean air actions  PM  emission abatements  air quality improvements  health benefits