检索结果-内蒙古大学图书馆

arXiv 2019年

作者： Han, Seunghwoi Ortmann, Lisa Kim, Hyunwoong Kim, Yong Woo Oka, Takashi Chacon, Alexis Doran, Brent Ciappina, Marcelo Lewenstein, Maciej Kim, Seung-Woo Kim, Seungchul Landsman, Alexandra S. 291 Daehak-ro Yuseong-gu34141 Korea Republic of Max Planck Institute for Physics of Complex Systems Noethnitzer Strasse 38 Dresden01187 Germany Max Planck Institute for Chemical Physics of Solids Noethnitzer Strasse 40 Dresden01187 Germany Center for Nonlinear Studies Physics and Chemistry of Materials T1-Division Los Alamos National Laboratory Los AlamosNM87545 United States Mathematical Institute University of Oxford Oxford United Kingdom Institute of Physics of ASCR ELI-Beamlines Na Slovance 2 Prague182 21 Czech Republic 08860 Spain ICREA Pg. Lluis Company 23 Barcelona08010 Spain Department of Optics and Mechatronics Engineering College of Nanoscience and Nanotechnology Pusan National University 2 Busandaehak-ro 63beon-gil Busan46241 Korea Republic of Institute for the Frontier of Attosecond Science and Technology CREOL and Department of Physics University of Central Florida OrlandoFL32816 United States

State-of-the-art experiments employ strong ultrafast optical fields to study the nonlinear response of electrons in solids on an attosecond time-scale1-13. Notably, a recent experiment1 retrieved a 3rd order nonlinear susceptibility by comparing the nonlinear response induced by a strong laser field to a linear response induced by the otherwise identical weak field. In parallel, experiments have demonstrated high harmonic generation (HHG) in solids2-11, a highly nonlinear process that until recently had only been observed in gases. The highly nonlinear nature of HHG has the potential to extract even higher order nonlinear susceptibility terms, and thereby characterize the entire response of the electronic system to strong field excitation. However, up till now, such characterization has been elusive due to a lack of direct correspondence between high harmonics and nonlinear susceptibilities. Here, we demonstrate a regime where such correspondence can be clearly made, extracting nonlinear susceptibilities (7th, 9th, and 11th) from sapphire of the same order as the measured high harmonics. The extracted high order susceptibilities show angular-resolved periodicities arising from variation in the band structure with crystal orientation. Nonlinear susceptibilities are key to ultrafast lightwave driven optoelectronics, allowing petahertz scaling manipulation of the signal1,14. Our results open a door to multi-channel signal processing, controlled by laser polarization. Copyright © 2019, The Authors. All rights reserved.

关键词： Crystal orientation

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基于离子和分子共存理论的炉渣氧化能力的表征

基于离子和分子共存理论的炉渣氧化能力的表征

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第十六届冶金反应工程学会议

作者： LI Peng-cheng 李鹏程 LI Jin-yan 李晋岩 ZHANG Meng 张盟 ZHANG Jian-liang 张建良 ZHANG Jian 张鉴 YANG Xue-min 杨学民北京科技大学冶金与生态工程学院北京100083 Beijing Metallurgical Equipment Research Design Institute Company Limited China Metallurgical Group Corporation Beijing 100029 P.R.China 北京中冶设备研究设计总院有限公司北京100029 School of Metallurgical and Ecological Engineering University of Science and Technology Beijing Beijing 100083 China 北京科技大学冶金与生态工程学院北京100083 State Key Laboratory of Multiphase Complex Systems Institute of Process Engineering Chinese Academy of Sciences Beijing 100190 China 中国科学院过程工程研究所多相复杂系统国家重点实验室北京100190 School of Metallurgical and Ecological Engineering University of Science and Technology Beijing Beijing 100083 China 中国科学院过程工程研究所多相复杂系统国家重点实验室北京100190 State Key Laboratory of Multiphase Complex Systems Institute of Process Engineering Chinese Academy of Sciences Beijing 100190 China

基于炉渣离子-分子共存理论(IMCT),本文计算了炉渣中铁氧化物的综合质量作用浓度NFe1o,并通过和传统冶金物理化学定义的活度αFe1O比较来验证综合质量作用浓度NFe1O的合理性。同时,本文在综合质量作用浓度NFe1O的基础上,建立了炉渣结构... 详细信息

基于炉渣离子-分子共存理论(IMCT),本文计算了炉渣中铁氧化物的综合质量作用浓度NFe1o,并通过和传统冶金物理化学定义的活度αFe1O比较来验证综合质量作用浓度NFe1O的合理性。同时,本文在综合质量作用浓度NFe1O的基础上,建立了炉渣结构单元和离子对的质量作用浓度模型,即CaO-SiO2-MgO-FeO-Fe2O3-MnO-Al2O3-P2O5渣系的IMCT-Ni模型。与实测值aFe1O相比,综合质量作用浓度NFe1O比实测值aFe1O的精确度高。

关键词：高炉炼铁炉渣氧化能力共存理论结构单元

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A ring-like accretion structure in M87 connecting its black hole and jet

arXiv

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arXiv 2023年

作者： Lu, Ru-Sen Asada, Keiichi Krichbaum, Thomas P. Park, Jongho Tazaki, Fumie Pu, Hung-Yi Nakamura, Masanori Lobanov, Andrei Hada, Kazuhiro Akiyama, Kazunori Kim, Jae-Young Marti-Vidal, Ivan Gómez, José L. Kawashima, Tomohisa Yuan, Feng Ros, Eduardo Alef, Walter Britzen, Silke Bremer, Michael Broderick, Avery E. Doi, Akihiro Giovannini, Gabriele Giroletti, Marcello Ho, Paul T.P. Honma, Mareki Hughes, David H. Inoue, Makoto Jiang, Wu Kino, Motoki Koyama, Shoko Lindqvist, Michael Liu, Jun Marscher, Alan P. Matsushita, Satoki Nagai, Hiroshi Rottmann, Helge Savolainen, Tuomas Schuster, Karl-Friedrich Shen, Zhi-Qiang de Vicente, Pablo Walker, R. Craig Yang, Hai Zensus, J. Anton Algaba, Juan Carlos Allardi, Alexander Bach, Uwe Berthold, Ryan Bintley, Dan Byun, Do-Young Casadio, Carolina Chang, Shu-Hao Chang, Chih-Cheng Chang, Song-Chu Chen, Chung-Chen Chen, Ming-Tang Chilson, Ryan Chuter, Tim C. Conway, John Crew, Geoffrey B. Dempsey, Jessica T. Dornbusch, Sven Faber, Aaron Friberg, Per García, Javier González Garrido, Miguel Gómez Han, Chih-Chiang Han, Kuo-Chang Hasegawa, Yutaka Herrero-Illana, Ruben Huang, Yau-De Huang, Chih-Wei L. Impellizzeri, Violette Jiang, Homin Jinchi, Hao Jung, Taehyun Kallunki, Juha Kirves, Petri Kimura, Kimihiro Koay, Jun Yi Koch, Patrick M. Kramer, Carsten Kraus, Alex Kubo, Derek Kuo, Cheng-Yu Li, Chao-Te Lin, Lupin Chun-Che Liu, Ching-Tang Liu, Kuan-Yu Lo, Wen-Ping Lu, Li-Ming MacDonald, Nicholas Martin-Cocher, Pierre Messias, Hugo Meyer-Zhao, Zheng Minter, Anthony Nair, Dhanya G. Nishioka, Hiroaki Norton, Timothy J. Nystrom, George Ogawa, Hideo Oshiro, Peter Patel, Nimesh A. Pen, Ue-Li Pidopryhora, Yurii Pradel, Nicolas Raffin, Philippe A. Rao, Ramprasad Ruiz, Ignacio Sanchez, Salvador Shaw, Paul Snow, William Sridharan, T.K. Srinivasan, Ranjani Tercero, Belén Torne, Pablo Traianou, Efthalia Wagner, Jan Walther, Craig Wei, Ta-Shun Yang, Jun Yu, Chen-Yu Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai China Key Laboratory of Radio Astronomy Chinese Academy of Sciences Nanjing China Max-Planck-Institut für Radioastronomie Bonn Germany Institute of Astronomy and Astrophysics Academia Sinica Taipei Taiwan Korea Astronomy and Space Science Institute Daejeon Korea Republic of Simulation Technology Development Department Tokyo Electron Technology Solutions Oshu Japan Mizusawa VLBI Observatory National Astronomical Observatory of Japan Oshu Japan Department of Physics National Taiwan Normal University Taipei Taiwan Center of Astronomy and Gravitation National Taiwan Normal University Taipei Taiwan Department of General Science and Education National Institute of Technology Hachinohe College Hachinohe City Japan Department of Astronomical Science The Graduate University for Advanced Studies SOKENDAI Mitaka Japan Black Hole Initiative Harvard University CambridgeMA United States Massachusetts Institute of Technology Haystack Observatory WestfordMA United States National Astronomical Observatory of Japan Mitaka Japan Department of Astronomy and Atmospheric Sciences Kyungpook National University Daegu Korea Republic of Departament d’Astronomia i Astrofísica Universitat de València Valencia Spain Observatori Astronòmic Universitat de València Valencia Spain Instituto de Astrofísica de Andalucía-CSIC Granada Spain Institute for Cosmic Ray Research The University of Tokyo Chiba Japan Key Laboratory for Research in Galaxies and Cosmology Chinese Academy of Sciences Shanghai China School of Astronomy and Space Sciences University of Chinese Academy of Sciences Beijing China Institut de Radioastronomie Millimétrique Saint Martin d’Hères France Department of Physics and Astronomy University of Waterloo WaterlooON Canada Waterloo Centre for Astrophysics University of Waterloo WaterlooON Canada Perimeter Institute for Theoretical Physics WaterlooON Canada Institute of Space and Astron

The nearby radio galaxy M87 is a prime target for studying black hole accretion and jet formation1,2. Event Horizon Telescope observations of M87 in 2017, at a wavelength of 1.3 mm, revealed a ring-like structure, which was interpreted as gravitationally lensed emission around a central black hole3. Here we report images of M87 obtained in 2018, at a wavelength of 3.5 mm, showing that the compact radio core is spatially resolved. High-resolution imaging shows a ring-like structure of 8. 4!1.1$0.5 Schwarzschild radii in diameter, approximately 50% larger than that seen at 1.3 mm. The outer edge at 3.5 mm is also larger than that at 1.3 mm. This larger and thicker ring indicates a substantial contribution from the accretion flow with absorption effects in addition to the gravitationally lensed ring-like emission. The images show that the edge–brightened jet connects to the accretion flow of the black hole. Close to the black hole, the emission profile of the jet-launching region is wider than the expected profile of a black -hole-driven jet, suggesting the possible presence of a wind associated with the accretion flow. © 2023, CC BY.

关键词： Galaxies

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An emission spectrum for WASP-121b measured across the 0.8-1.1 µm wavelength range using the Hubble Space Telescope

arXiv

引用

arXiv 2019年

作者： Mikal-Evans, Thomas Sing, David K. Goyal, Jayesh M. Drummond, Benjamin Carter, Aarynn L. Henry, Gregory W. Wakeford, Hannah R. Lewis, Nikole K. Marley, Mark S. Tremblin, Pascal Nikolov, Nikolay Kataria, Tiffany Deming, Drake Ballester, Gilda E. Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology 77 Massachusetts Avenue CambridgeMA02139 United States Department of Earth and Planetary Sciences Johns Hopkins University BaltimoreMD United States Department of Physics & Astronomy Johns Hopkins University BaltimoreMD United States Physics and Astronomy Stocker Road University of Exeter ExeterEX4 3RF United Kingdom Center of Excellence in Information Systems Tennessee State University NashvilleTN37209 United States Space Telescope Science Institute 3700 San Martin Drive BaltimoreMD21218 United States Department of Astronomy and Carl Sagan Institute Cornell University 122 Sciences Drive IthacaNY14853 United States NASA Ames Research Center Moffett FieldCA United States Maison de la Simulation CEA CNRS Univ Paris-Sud UVSQ Université Paris-Saclay Gif-sur-YvetteF-91191 France NASA Jet Propulsion Laboratory 4800 Oak Grove Drive PasadenaCA91109 United States Department of Astronomy University of Maryland at College Park College ParkMD20742 United States Lunar and Planetary Laboratory University of Arizona TucsonAZ85721 United States

WASP-121b is a transiting gas giant exoplanet orbiting close to its Roche limit, with an inflated radius nearly double that of Jupiter and a dayside temperature comparable to a late M dwarf photosphere. Secondary eclipse observations covering the 1.1-1.6 µm wavelength range have revealed an atmospheric thermal inversion on the dayside hemisphere, likely caused by high altitude absorption at optical wavelengths. Here we present secondary eclipse observations made with the Hubble Space Telescope Wide Field Camera 3 spectrograph that extend the wavelength coverage from 1.1 µm down to 0.8 µm. To determine the atmospheric properties from the measured eclipse spectrum, we performed a retrieval analysis assuming chemical equilibrium, with the effects of thermal dissociation and ionization included. Our best-fit model provides a good fit to the data with reduced χν2 = 1.04. The data diverge from a blackbody spectrum and instead exhibit emission due to H− shortward of 1.1 µm. The best-fit model does not reproduce a previously reported bump in the spectrum at 1.25µm, possibly indicating this feature is a statistical fluctuation in the data rather than a VO emission band as had been tentatively suggested. We estimate an atmospheric metallicity of [M/H] = 1.09+0.58/-0.69, and fit for the carbon and oxygen abundances separately, obtaining [C/H] = −0.29+0.61/-0.48 and [O/H] = 0.18+0.64/-0.60. The corresponding carbon-to-oxygen ratio is C/O = 0.49+0.65/-0.37, which encompasses the solar value of 0.54, but has a large uncertainty. Copyright © 2019, The Authors. All rights reserved.

关键词： Carbon

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The climate opportunities and risks of improving building envelopes across 1,677 Chinese cities

引用

Cell Reports Sustainability 2024年第12期1卷

作者： Zhang, Yufei Dang, Mengyuan Chu, Chunli Behrens, Paul Berrill, Peter Zhong, Xiaoyang Jing, Rui Lei, Nuoa Jia, Hongyuan Zhang, Lixiao Shao, Chaofeng Masanet, Eric Ju, Meiting Liu, Lirong Chen, Weiqiang Cao, Zhi College of Environmental Science and Engineering Nankai University 38 Tongyan Road Jinnan District Tianjin 300350 China Institute of Environmental Sciences (CML) Leiden University RA Leiden Leiden 2300 Netherlands Oxford Martin School University of Oxford 34 Broad Street Oxford OX1 3BD United Kingdom Sustainability Economics of Human Settlements Technische Universität Berlin Fasanenstr. 88 Berlin 10623 Germany Mercator Research Institute on Global Commons and Climate Change Berlin 10829 Germany International Institute of Applied Systems Analysis (IIASA) Schlossplatz 1 Laxenburg 2361 Austria College of Energy Xiamen University Xiamen 361005 China Energy Technologies Area Lawrence Berkeley National Laboratory Berkeley 94720 CA United States School of Civil Engineering and Architecture Chongqing University of Science and Technology Chongqing 401331 China SinBerBEST Berkeley Education Alliance for Research in Singapore Singapore 138602 Singapore State Key Joint Laboratory of Environmental Simulation and Pollution Control School of Environment Beijing Normal University Beijing 100875 China Bren School of Environmental Science and Management University of California Santa Barbara 93106 CA United States Department of Mechanical Engineering University of California Santa Barbara 93106 CA United States Centre for Environment and Sustainability University of Surrey Guildford GU2 7XH United Kingdom Institute of Urban Environment Chinese Academy of Sciences Xiamen 361021 China

The global building sector consumes approximately 30% of final energy, making it crucial for climate change mitigation and adaptation. International calls for enhancing building energy efficiencies are growing, focusing on strategies such as energy-efficient building envelopes through renovation and replacement of older structures, along with electrification and fuel switching. However, the energy-saving potential of these improvements remains uncertain due to the complex interplay of building stock characteristics and climatic conditions. Here, we diagnose the compound effects of envelope improvements and climate change on China's housing energy demand using a physics-based building energy model with fine spatial and temporal granularity, covering 1,677 sub-province-level cities. Our model shows that envelope improvements play very different roles in ameliorating climate change impacts on housing energy use across the country, highlighting the need for building climate-resilient energy supply and pursuing alternative energy efficiency strategies in less climate-resilient regions. © 2024 The Authors

关键词： building energy building envelopes climate change cooling demand heating demand stock dynamics surrogate modeling

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Exoplanet Biosignatures: Future Directions

arXiv

引用

arXiv 2017年

作者： Walker, Sara I. Bains, William Cronin, Leroy DasSarma, Shiladitya Danielache, Sebastian Domagal-Goldman, Shawn Kacar, Betul Kiang, Nancy Y. Lenardic, Adrian Reinhard, Christopher T. Moore, William Schwieterman, Edward W. Shkolnik, Evgenya L. Smith, Harrison B. School of Earth and Space Exploration Arizona State University TempeAZ United States Beyond Center for Fundamental Concepts in Science Arizona State University TempeAZ United States ASU-Santa Fe Institute Center for Biosocial Complex Systems Arizona State University TempeAZ United States Blue Marble Space Institute of Science SeattleWA United States MIT 77 Mass Ave CambridgeMA02139 United States School of Chemistry University of Glasgow GlasgowG12 8QQ United Kingdom Department of Microbiology and Immunology Institute of Marine and Environmental Technology University of Maryland School of Medicine BaltimoreMD United States Department of Materials and Life Science Faculty of Science and Technology Sophia University Tokyo Japan Earth Life Institute Tokyo Institute of Technology Tokyo Japan NASA Goddard Space Flight Center GreenbeltMD United States NASA Astrobiology Institute Virtual Planetary Laboratory Team University of Washington SeattleWA United States Organismic and Evolutionary Biology Harvard University CambridgeMA United States NASA Astrobiology Institute Reliving the Past Team University of Montana MissoulaMT United States University of Arizona Department of Molecular and Cell Biology and Astronomy Tucson AZ NASA Goddard Institute for Space Studies New YorkNY United States Department of Earth Science Rice University HoustonTX United States School of Earth and Atmospheric Sciences Georgia Institute of Technology AtlantaGA United States NASA Astrobiology Institute Alternative Earths Team University of California RiversideCA United States Department of Atmospheric and Planetary Sciences Hampton University HamptonVA United States National Institute of Aerospace HamptonVA United States Department of Earth Sciences University of California RiversideCA United States NASA Postdoctoral Program Universities Space Research Association ColumbiaMD United States School of Earth and Space Exploration Arizona State University PO Box

Exoplanet science promises a continued rapid accumulation of new observations in the near future, energizing a drive to understand and interpret the forthcoming wealth of data to identify signs of life beyond our Solar System. The large statistics of exoplanet samples, combined with the ambiguity of our understanding of universal properties of life and its signatures, necessitate a quantitative framework for biosignature assessment Here, we introduce a Bayesian framework for guiding future directions in life detection, which permits the possibility of generalizing our search strategy beyond biosignatures of known life. The Bayesian methodology provides a language to define quantitatively the conditional probabilities and confidence levels of future life detection and, importantly, may constrain the prior probability of life with or without positive detection. We describe empirical and theoretical work necessary to place constraints on the relevant likelihoods, including those emerging from stellar and planetary context, the contingencies of evolutionary history and the universalities of physics and chemistry. We discuss how the Bayesian framework can guide our search strategies, including determining observational wavelengths or deciding between targeted searches or larger, lower resolution surveys. Our goal is to provide a quantitative framework not entrained to specific definitions of life or its signatures, which integrates the diverse disciplinary perspectives necessary to confidently detect alien life. Copyright © 2017, The Authors. All rights reserved.

关键词： Extrasolar planets

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Publisher Correction: Polariton condensates for classical and quantum computing

Nature Reviews Physics

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Nature Reviews Physics 2022年 496页

作者： Alexey Kavokin Timothy C. H. Liew Christian Schneider Pavlos G. Lagoudakis Sebastian Klembt Sven Hoefling Key Laboratory for Quantum Materials of Zhejiang Province School of Science Westlake University Hangzhou China Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University Singapore Singapore Institute of Physics University of Oldenburg Oldenburg Germany Skolkovo Institute of Science and Technology Moscow Russia Department of Physics and Astronomy University of Southampton Southampton UK Technische Physik and Wilhelm-Conrad-Röntgen-Research Center for Complex Material Systems University of Würzburg Würzburg Germany Würzburg–Dresden Cluster of Excellence ct.qmat University of Würzburg Würzburg Germany

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Publisher Correction: Ozone pollution mitigation strategy informed by long-term trends of atmospheric oxidation capacity

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Nature Geoscience 2024年 172页

作者： Wenjie Wang Xin Li Ying Liu Sihua Lu Yusheng Wu Shiyi Chen Keding Lu Min Hu Limin Zeng Min Shao Yuanhang Zhang Hang Su Yafang Cheng Ruijing Ni Ulrich Pöschl Zhaofeng Tan Franz Rohrer Andreas Wahner David D. Parrish Cheng Huang Xudong Tian K. M. Leung Liangfu Chen Meng Fan Qiang Zhang State Key Joint Laboratory of Environmental Simulation and Pollution Control College of Environmental Sciences and Engineering Peking University Beijing China State Key Laboratory of Atmospheric Environment and Extreme Meteorology Institute of Atmospheric Physics Chinese Academy of Sciences Beijing China Max Planck Institute for Chemistry Mainz Germany International Joint Laboratory for Regional Pollution Control Ministry of Education Beijing China Collaborative Innovation Centre of Atmospheric Environment and Equipment Technology Nanjing University of Information Science & Technology Nanjing China Institute of Carbon Neutrality Peking University Beijing China Institute for Environmental and Climate Research Jinan University Guangzhou China State Environmental Protection Key Laboratory of Formation and Prevention of Urban Air Pollution Complex Shanghai Academy of Environmental Sciences Shanghai China Institut für Energie-und Klimaforschung: Troposphäre (IEK-8) Forschungszentrum Jülich Jülich Germany Key Laboratory of Ecological and Environmental Monitoring Forewarning and Quality Control of Zhejiang Zhejiang Ecological and Environmental Monitoring Center Hangzhou China Environmental Protection Department The Government of the Hong Kong Special Administrative Region Hong Kong China State Key Laboratory of Remote Sensing Science The Aerospace Information Research Institute Chinese Academy of Sciences Beijing China Department of Earth System Science Tsinghua University Beijing China

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Strong and Fragile Topological Dirac Semimetals with Higher-Order Fermi Arcs

arXiv

引用

arXiv 2019年

作者： Wieder, Benjamin J. Wang, Zhijun Cano, Jennifer Dai, Xi Schoop, Leslie M. Bradlyn, Barry Bernevig, B. Andrei Department of Physics Princeton University PrincetonNJ08544 United States Beijing National Laboratory for Condensed Matter Physics Institute of Physics Chinese Academy of Sciences Beijing100190 China University of Chinese Academy of Sciences Beijing100049 China Department of Physics and Astronomy Stony Brook University Stony BrookNY11974 United States Center for Computational Quantum Physics The Flatiron Institute New YorkNY10010 United States Physics Department Hong Kong University of Science and Technology Clear Water Bay Hong Kong Department of Chemistry Princeton University PrincetonNJ08544 United States Department of Physics Institute for Condensed Matter Theory University of Illinois at Urbana-Champaign UrbanaIL61801-3080 United States Donostia International Physics Center P. Manuel de Lardizabal 4 Donostia-San Sebastián20018 Spain Dahlem Center for Complex Quantum Systems and Fachbereich Physik Freie Universität Berlin Arnimallee 14 Berlin14195 Germany Max Planck Institute of Microstructure Physics Halle06120 Germany

Dirac and Weyl semimetals both exhibit arc-like surface states. However, whereas the surface Fermi arcs in Weyl semimetals are topological consequences of the Weyl points themselves, the surface Fermi arcs in Dirac semimetals are not directly related to the bulk Dirac points, raising the question of whether there exists a topological bulk-boundary correspondence for Dirac semimetals. In this work, we discover that strong and fragile topological Dirac semimetals exhibit 1D higher-order hinge Fermi arcs (HOFAs) as universal, direct consequences of their bulk 3D Dirac points. To predict HOFAs coexisting with topological surface states in solid-state Dirac semimetals, we introduce and layer a spinful model of an s − d-hybridized quadrupole insulator (QI). We develop a rigorous nested Jackiw-Rebbi formulation of QIs and HOFA states. Employing ab initio calculations, we demonstrate HOFAs in both the room- (α) and intermediate-temperature (α′′) phases of Cd3As2, KMgBi, and rutile-structure (β′-) PtO2. Copyright © 2019, The Authors. All rights reserved.

关键词： Topology

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Preface

Lecture Notes in Networks and Systems

引用

Lecture Notes in Networks and systems 2023年 729 LNNS卷 v-vi页

作者： Vasant, Pandian Weber, Gerhard-Wilhelm Arefin, Mohammad Shamsul Rodriguez-Aguilar, Roman Panchenko, Vladimir Munapo, Elias Thomas, J. Joshua Faculty of Electrical and Electronics Engineering Modeling Evolutionary Algorithms Simulation and Artificial Intelligence Ton Duc Thang University Ho Chi Minh City Viet Nam Department of Computer Science Chittagong University of Engineering and Technology Chittagong Bangladesh Laboratory of Non-traditional Energy Systems Department of Theoretical and Applied Mechanics Federal Scientific Agroengineering Center VIM Russian University of Transport Moscow Russia Department of Computer Science UOW Malaysia KDU Penang University College George Town Malaysia Faculty of Engineering Management Poznań University of Technology Poznan Poland School of Economics and Decision Sciences North West University Mmabatho South Africa Facultad de Ciencias Económicas y Empresariales School of Economic and Business Sciences Universidad Panamericana Mexico City Mexico

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