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arXiv 2024年

作者： Yalçınkaya, S. Esmer, E.M. Baştürk, Ö. Muhaymin, A. Kutluay, A.C. Silistre, D.I. Akar, F. Southworth, J. Mancini, L. Davoudi, F. Karamanlı, E. Tezcan, F. Demir, E. Yılmaz, D. Güleroglu, E. Tekin, M. Taşkın, I. Aladag, Y. Sertkan, E. Kurt, U.Y. Fişek, S. Kaptan, S. Aliş, S. Aksaker, N. Yelkenci, F.K. Tezcan, C.T. Kaya, A. Oglakkaya, D. Aydın, Z.S. Yeşilyaprak, C. Department of Astronomy & Space Sciences Faculty of Science Ankara University AnkaraTR-06100 Turkey Incek Blvd. Ahlatlıbel AnkaraTR-06837 Turkey Bilkent University Faculty of Science Department of Physics AnkaraTR-06800 Turkey Middle East Technical University Science Faculty Physics Department Ankara Turkey Astrophysics Group Keele University StaffordshireST5 5BG United Kingdom Department of Physics University of Rome "Tor Vergata" Via della Ricerca Scientifica 1 RomaI-00133 Italy INAF Turin Astrophysical Observatory Via Osservatorio 20 Pino TorineseI-10025 Italy Max Planck Institute for Astronomy Königstuhl 17 HeidelbergD-69117 Germany Astrobiology Research Unit Universitè de Liège Allèe du 6 Aôut 19C LiègeB-4000 Belgium Atatürk University Science Faculty Department of Astronomy and Space Sciences Erzurum25240 Turkey University of Çukurova Adana01330 Turkey Department of Astronomy and Space Sciences Faculty of Science Istanbul University Istanbul34119 Turkey Astronomy and Space Sciences Program Institute of Graduate Studies in Sciences Istanbul University Istanbul34116 Turkey Adana Organised Industrial Zones Vocational School of Technical Science University of Çukurova Adana01410 Turkey Yakutiye Erzurum25240 Turkey

We update the ephemerides of 16 transiting exoplanets using our ground-based observations, new TESS data, and previously published observations including those of amateur astronomers. All these light curves were modeled by making use of a set of quantitative criteria with the exofast code to obtain mid-transit times. We searched for statistically significant secular and/or periodic trends in the mid-transit times. We found that the timing data are well modeled by a linear ephemeris for all systems except for XO-2 b, for which we detect an orbital decay with the rate of -12.95 1.85 ms/yr that can be confirmed with future observations. We also detect a hint of potential periodic variations in the TTV data of HAT-P-13 b which also requires confirmation with further precise observations. © 2024, CC BY-NC-ND.

关键词： Orbits

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Code Comparison for Fast Flavor Instability Simulation

arXiv

引用

arXiv 2022年

作者： Richers, Sherwood Duan, Huaiyu Wu, Meng-Ru Bhattacharyya, Soumya Zaizen, Masamichi George, Manu Lin, Chun-Yu Xiong, Zewei Department of Physics University of California BerkeleyCA94720 United States Department of Physics & Astronomy University of New Mexico AlbuquerqueNM87131 United States Institute of Physics Academia Sinica Taipei11529 Taiwan Institute of Astronomy and Astrophysics Academia Sinica Taipei10617 Taiwan Tata Institute of Fundamental Research Homi Bhabha Road Mumbai400005 India Faculty of Science and Engineering Waseda University Tokyo169-8555 Japan Department of Astronomy Graduate School of Science University of Tokyo Tokyo113-0033 Japan National Center for High-performance Computing National Applied Research Laboratories Hsinchu Science Park Hsinchu City30076 Taiwan GSI Helmholtzzentrum für Schwerionenforschung Planckstraße 1 Darmstadt64291 Germany

The fast flavor instability (FFI) is expected to be ubiquitous in core-collapse supernovae and neutron star mergers. It rapidly shuffles neutrino flavor in a way that could impact the explosion mechanism, neutrino signals, mass outflows, and nucleosynthesis. The variety of initial conditions and simulation methods employed in simulations of the FFI prevent an apples-to-apples comparison of the results. We simulate a standardized test problem using five independent codes and verify that they are all faithfully simulating the underlying quantum kinetic equations under the assumptions of axial symmetry and homogeneity in two directions. We quantify the amount of numerical error in each method and demonstrate that each method is superior in at least one metric of this error. We make the results publicly available to serve as a benchmark. © 2022, CC BY.

关键词： Fruits

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Logarithmic Entanglement Growth from Disorder-Free Localization in the Two-Leg Compass Ladder

引用

Physical Review Letters 2021年第22期126卷 227202-227202页

作者： Oliver Hart Sarang Gopalakrishnan Claudio Castelnovo T.C.M. Group Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE United Kingdom Physics Program and Initiative for the Theoretical Sciences Graduate Center CUNY New York New York 10016 USA Physics and Astronomy College of Staten Island Staten Island New York 10314 USA Department of Physics The Pennsylvania State University University Park Pennsylvania 16802 USA

We explore the finite-temperature dynamics of the quasi-1D orbital compass and plaquette Ising models. We map these systems onto a model of free fermions coupled to strictly localized spin-1/2 degrees of freedom. At finite temperature, the localized degrees of freedom act as emergent disorder and localize the fermions. Although the model can be analyzed using free-fermion techniques, it has dynamical signatures in common with typical many-body localized systems: Starting from generic initial states, entanglement grows logarithmically; in addition, equilibrium dynamical correlation functions decay with an exponent that varies continuously with temperature and model parameters. These quasi-1D models offer an experimentally realizable setting in which natural dynamical probes show signatures of disorder-free many-body localization.

关键词： Anderson localization Entanglement entropy Localization Many-body localization Nonequilibrium statistical mechanics Integrable systems Spin ladders

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Experimental Realization of a Protected Superconducting Circuit Derived from the 0–π Qubit

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PRX Quantum 2021年第1期2卷 010339-010339页

作者： András Gyenis Pranav S. Mundada Agustin Di Paolo Thomas M. Hazard Xinyuan You David I. Schuster Jens Koch Alexandre Blais Andrew A. Houck Department of Electrical Engineering Princeton University Princeton New Jersey 08544 USA Institut quantique & Département de Physique Université de Sherbrooke Sherbrooke Quebec J1K 2R1 Canada Graduate Program in Applied Physics Northwestern University Evanston Illinois 60208 USA The James Franck Institute and Department of Physics University of Chicago Chicago Illinois 60637 USA Department of Physics and Astronomy Northwestern University Evanston Illinois 60208 USA Canadian Institute for Advanced Research Toronto Ontario M5G 1M1 Canada

Encoding a qubit in logical quantum states with wave functions characterized by disjoint support and robust energies can offer simultaneous protection against relaxation and pure dephasing. One of the most promising candidates for such a fully protected superconducting qubit is the 0–π circuit [Brooks et al., Phys. Rev. A 87, 052306 (2013)]. Here we realize the proposed circuit topology in an experimentally obtainable parameter regime, where the ground-state degeneracy is lifted but the qubit is still largely noise protected. More precisely, the logical states of this qubit feature disjoint support and are exponentially protected against relaxation and exponentially (first order) protected against dephasing due to charge (flux) noise. We name the resultant device the “soft 0–π qubit.” Multitone spectroscopy measurements reveal the energy-level structure of the system, which can be precisely described by a simple two-mode Hamiltonian. Using a Raman-type protocol, we exploit a higher-lying charge-insensitive energy level of the device to realize coherent population transfer and logical operations. The measured relaxation (T1=1.6 ms) and dephasing (TR=9μs, T2E=25μs) times demonstrate that the soft 0–π circuit not only broadens the family of superconducting qubits but also constitutes an important step toward quantum computing with intrinsically protected superconducting qubits.

关键词： Quantum computation Quantum information with solid state qubits

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Camera Calibration of the CTA-LST prototype 37

Camera Calibration of the CTA-LST prototype

引用

37th International Cosmic Ray Conference, ICRC 2021

作者： Kobayashi, Yukiho Okumura, Akira Cassol, Franca Katagiri, Hideaki Sitarek, Julian Gliwny, Pawel Nozaki, Seiya Nogami, Yuto Abe, H. Aguasca, A. Agudo, I. Antonelli, L.A. Aramo, C. Armstrong, T. Artero, M. Asano, K. Ashkar, H. Aubert, P. Baktash, A. Bamba, A. Baquero Larriva, A. Baroncelli, L. Barres de Almeida, U. Barrio, J.A. Batkovic, I. Becerra Gonzalez, J. Bernardos, M.I. Berti, A. Biederbeck, N. Bigongiari, C. Blanch, O. Bonnoli, G. Bordas, P. Bose, D. Bulgarelli, A. Burelli, I. Buscemi, M. Cardillo, M. Caroff, S. Carosi, A. Cerruti, M. Chai, Y. Cheng, K. Chikawa, M. Chytka, L. Contreras, J.L. Cortina, J. Costantini, H. Dalchenko, M. De Angelis, A. de Bony de Lavergne, M. Deleglise, G. Delgado, C. Delgado Mengual, J. della Volpe, D. Depaoli, D. Di Pierro, F. Di Venere, L. Daaz, C. Dominik, R.M. Dominis Prester, D. Donini, A. Dorner, D. Doro, M. Elsaasser, D. Emery, G. Escudero, J. Fiasson, A. Foffano, L. Fonseca, M.V. Freixas Coromina, L. Fukami, S. Fukazawa, Y. Garcia, E. Garcia Lapez, R. Giglietto, N. Giordano, F. Godinovic, N. Green, D. Grespan, P. Gunji, S. Hackfeld, J. Hadasch, D. Hahn, A. Hassan, T. Hayashi, K. Heckmann, L. Heller, M. Herrera Llorente, J. Hirotani, K. Hoffmann, D. Horns, D. Houles, J. Hrabovsky, M. Hrupec, D. Hui, D. HÃŒtten, M. Inada, T. Inome, Y. Iori, M. Ishio, K. Iwamura, Y. Jacquemont, M. Jimenez Martinez, I. Jouvin, L. Jurysek, J. Kagaya, M. Karas, V. Kataoka, J. Kerszberg, D. Kong, A. Kubo, H. Kushida, J. Lamanna, G. Lamastra, A. Le Flour, T. Longo, F. Lapez-Coto, R. Lapez-Moya, M. Lapez-Oramas, A. Luque-Escamilla, P.L. Majumdar, P. Makariev, M. Mandat, D. Manganaro, M. Mannheim, K. Mariotti, M. Marquez, P. Marsella, G. Marta, J. Martinez, O. MartÃnez, G. MartÃnez, M. Marusevec, P. Mas, A. Maurin, G. Mazin, D. Mestre Guillen, E. Micanovic, S. Miceli, D. Miener, T. Miranda, J.M. Miranda, L.D.M. Mirzoyan, R. Mizuno, T. Molina, E. Montaruli, T. Monteiro, I. Moralejo, A. Morcuende, D. Moretti, E. Morselli, A. Mrakovcic, K. Institute for Cosmic Ray Research The University of Tokyo Chiba Japan Institute for Space-Earth Environmental Research Kobayashi-Maskawa Institute for the Origin of Particles and the Universe Nagoya University Nagoya Japan Aix Marseille Univ CNRS IN2P3 CPPM Marseille France College of Science Ibaraki University Ibaraki Japan Faculty of Physics and Applied Informatics University of Lodz ul. Pomorska 149/153 Lódz90-236 Poland Department of Physics Kyoto University Kyoto606-8502 Japan Institute for Cosmic Ray Research University of Tokyo Japan Departament de Fasica Quantica i Astrofasica Institut de Ciancies del Cosmos Universitat de Barcelona IEEC-UB Spain Instituto de Astrofasica de Andalucaa-CSIC Spain INAF - Osservatorio Astronomico di Roma Italy INFN Sezione di Napoli Italy Aix Marseille Univ CNRS IN2P3 CPPM France The Barcelona Institute of Science and Technology Spain IRFU CEA Universita© Paris-Saclay France LAPP Univ. Grenoble Alpes Univ. Savoie Mont Blanc CNRS-IN2P3 Annecy France Universitaat Hamburg Institut faer Experimentalphysik Germany Graduate School of Science University of Tokyo Japan EMFTEL Department IPARCOS Universidad Complutense de Madrid Spain INAF - Osservatorio di Astrofisica e Scienza dello Spazio di Bologna Italy Centro Brasileiro de Pesquisas Fasicas Brazil INFN Sezione di Padova Universita degli Studi di Padova Italy Instituto de Astrofasica de Canarias Departamento de Astrofasica Universidad de La Laguna Spain Max-Planck-Institut faer Physik Germany Department of Physics TU Dortmund University Germany Saha Institute of Nuclear Physics India INFN Sezione di Trieste Universita degli Studi di Udine Italy INFN Sezione di Catania Italy Italy University of Geneva Da©partement de Physique Nucla©aire et Corpusculaire Switzerland Palacky University Olomouc Faculty of Science Czech Republic CIEMAT Spain Port d'Informacia Cientafica Spain INFN Sezione di Torino Italy Dipartimento di Fisica Universita degli Studi di Tori

The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory that is expected to reach one order of magnitude better sensitivity than that of current telescope arrays. The Large-Sized Telescopes (LSTs) have an essential role in extending the energy range down to 20 GeV. The prototype LST (LST-1) proposed for CTA was built in La Palma, the northern site of CTA, in 2018. LST-1 is currently in its commissioning phase and moving towards scientific observations. The LST-1 camera consists of 1855 photomultiplier tubes (PMTs) which are sensitive to Cherenkov light. PMT signals are recorded as waveforms sampled at 1 GHz rate with Domino Ring Sampler version 4 (DRS4) chips. Fast sampling is essential to achieve a low energy threshold by minimizing the integration of background light from the night sky. Absolute charge calibration can be performed by the so-called F-factor method, which allows calibration constants to be monitored even during observations. A calibration pipeline of the camera readout has been developed as part of the LST analysis chain. The pipeline performs DRS4 pedestal and timing corrections, as well as the extraction and calibration of charge and time of pulses for subsequent higher-level analysis. The performance of each calibration step is examined, and especially charge and time resolution of the camera readout are evaluated and compared to CTA requirements. We report on the current status of the calibration pipeline, including the performance of each step through to signal reconstruction, and the consistency with Monte Carlo simulations. © 2022 Sissa Medialab Srl. All rights reserved.

关键词： Calibration

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Addressing challenges for operating electrochemical solar fuels technologies under variable and diurnal conditions

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Frontiers in Energy Research 2024年 12卷

作者： Yap, Kyra M. K. Lee, Sol A. Kistler, Tobias A. Collins, Darci K. Warren, Emily L. Atwater, Harry A. Jaramillo, Thomas F. Xiang, Chengxiang Nielander, Adam C. Department of Chemical Engineering Stanford University StanfordCA United States SUNCAT Center for Interface Science and Catalysis SLAC National Accelerator Laboratory Menlo ParkCA United States Department of Applied Physics and Materials Science California Institute of Technology PasadenaCA United States Chemical Sciences Division Lawrence Berkeley National Laboratory BerkeleyCA United States Chemistry and Nanoscience Center National Renewable Energy Laboratory GoldenCO United States Advanced Energy Systems Graduate Program Colorado School of Mines GoldenCO United States

The outdoor operation of electrochemical solar fuels devices must contend with challenges presented by the cycles of solar irradiance, temperature, and other meteorological factors. Herein, we discuss challenges associated with these fluctuations presented over three timescales, including the effects of diurnal cycling over the course of many days, a single diurnal cycle over the course of hours, and meteorological phenomena that cause fluctuations on the order of seconds to minutes. We also highlight both reaction-independent and reaction-specific effects of variable conditions for the hydrogen evolution reaction and CO2 reduction reaction. We identify key areas of research for advancing the outdoor operation of solar fuels technology and highlight the need for metrics and benchmarks to enable the comparison of diurnal studies across systems and geographical locations. Copyright © 2024 Yap, Lee, Kistler, Collins, Warren, Atwater, Jaramillo, Xiang and Nielander.

关键词： Hydrogen fuels

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The ALMA-QUARKS Survey.Ⅰ.Survey Description and Data Reduction

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Research in astronomy and Astrophysics 2024年第2期24卷 104-124页

作者：刘训川 Tie Liu Lei Zhu Guido Garay Hong-Li Liu Paul Goldsmith Neal Evans Kee-Tae Kim Sheng-Yuan Liu Fengwei Xu Xing Lu Anandmayee Tej Xiaofeng Mai Leonardo Bronfman Shanghuo Li Diego Mardones Amelia Stutz Ken'ichi Tatematsu Ke Wang Qizhou Zhang Sheng-Li Qin Jianwen Zhou Qiuyi Luo Siju Zhang Yu Cheng Jinhua He Qilao Gu Ziyang Li Zhenying Zhang Suinan Zhang Anindya Saha Lokesh Dewangan Patricio Sanhueza Zhiqiang Shen Shanghai Astronomical Observatory Chinese Academy of SciencesShanghai 200030China Chinese Academy of Sciences South America Center for Astronomy National Astronomical ObservatoriesChinese Academy of SciencesBeijing 100101China Departamento de Astronomía Universidad de ChileLas Condes7591245 SantiagoChile School of Physics and Astronomy Yunnan UniversityKunming 650091China Jet Propulsion Laboratory California Institute of Technology4800 Oak Grove DrivePasadena CA 91109USA Department of Astronomy The University of Texas at AustinTX 78712-1205USA Korea Astronomy and Space Science Institute 776 Daedeokdae-roYuseong-guDaejeon 34055Republic of Korea Institute of Astronomy and Astrophysics Academia SinicaRoosevelt RoadTaipei 10617China Kavli Institute for Astronomy and Astrophysics Peking UniversityBeijing 100871China Department of Astronomy School of PhysicsPeking UniversityBeijing 100871China Indian Institute of Space Science and Technology Thiruvananthapuram 695547KeralaIndia Max Planck Institute for Astronomy Königstuhl 17D-69117 HeidelbergGermany Departamento de Astronomía Universidad de ConcepciónCasilla 160-CConcepciónChile Nobeyama Radio Observatory National Astronomical Observatory of JapanNational Institutes of Natural Sciences462-2 NobeyamaMinamimakiMinamisakuNagano 384-1305Japan Center for Astrophysics∣Harvard&Smithsonian 60 Garden StreetCambridgeMA 02138USA Max-Planck-Institut für Radioastronomie Auf dem Hügel 69D-53125 BonnGermany School of Astronomy and Space Sciences University of Chinese Academy of SciencesBeijing 100049China National Astronomical Observatory of Japan 2-21-1 OsawaMitakaTokyo181-8588Japan Yunnan Observatories Chinese Academy of SciencesKunming 650216China Physical Research Laboratory NavrangpuraAhmedabad-380009India Astronomical Science Program The Graduate University for Advanced StudiesSOKENDAI2-21-1 OsawaMitakaTokyo 181-8588Japan University of Science and Technology Korea(UST)217 Gajeong-roYuseong-guDaejeon 34113Republic o

This paper presents an overview of the QUARKS survey,which stands for Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures."The QUARKS survey is observing139 massive clumps covered by 156 pointings at Atacama Large Millimeter/submillimeter Array(ALMA)Band 6(λ~1.3 mm).In conjunction with data obtained from the ALMA-ATOMS survey at Band 3(λ~3 mm),QUARKS aims to carry out an unbiased statistical investigation of massive star formation process within protoclusters down to a scale of 1000 *** overview paper describes the observations and data reduction of the QUARKS survey,and gives a first look at an exemplar source,the mini-starburst Sgr B2(M).The wide-b and width(7.5 GHz)and high-angular-resolution(~0."3)observations of the QUARKS survey allow for the resolution of much more compact cores than those could be done by the ATOMS survey,and to detect previously unrevealed fainter filamentary *** spectral windows cover transitions of species including CO,SO,N_(2)D^(+),SiO,H_(30)α,H_(2)CO,CH_(3)CN,and many other complex organic molecules,tracing gas components with different temperatures and spatial *** aims to deepen our understanding of several scientific topics of massive star formation,such as the mass transport within protoclusters by(hub-)filamentary structures,the existence of massive starless cores,the physical and chemical properties of dense cores within protoclusters,and the feedback from already formed high-mass young protostars.

关键词： stars formation-stars kinematics and dynamics-ISM clouds-ISM molecules

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Low-Velocity-Favored Transition Radiation

引用

Physical Review Letters 2023年第11期131卷 113002-113002页

作者： Jialin Chen Ruoxi Chen Fuyang Tay Zheng Gong Hao Hu Yi Yang Xinyan Zhang Chan Wang Ido Kaminer Hongsheng Chen Baile Zhang Xiao Lin Interdisciplinary Center for Quantum Information State Key Laboratory of Extreme Photonics and Instrumentation ZJU-Hangzhou Global Scientific and Technological Innovation Center College of Information Science & Electronic Engineering Zhejiang University Hangzhou 310027 China International Joint Innovation Center the Electromagnetics Academy at Zhejiang University Zhejiang University Haining 314400 China Department of Electrical and Computer Engineering Technion-Israel Institute of Technology Haifa 32000 Israel Department of Electrical and Computer Engineering Rice University Houston Texas 77005 USA Applied Physics Graduate Program Smalley-Curl Institute Rice University Houston Texas 77005 USA School of Electrical and Electronic Engineering Nanyang Technological University Singapore 639798 Singapore Department of Physics University of Hong Kong Hong Kong 999077 China Key Lab of Advanced Micro/Nano Electronic Devices & Smart Systems of Zhejiang Jinhua Institute of Zhejiang University Zhejiang University Jinhua 321099 China Shaoxing Institute of Zhejiang University Zhejiang University Shaoxing 312000 China Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University Singapore 637371 Singapore Centre for Disruptive Photonic Technologies Nanyang Technological University Singapore 637371 Singapore

When a charged particle penetrates through an optical interface, photon emissions emerge—a phenomenon known as transition radiation. Being paramount to fundamental physics, transition radiation has enabled many applications from high-energy particle identification to novel light sources. A rule of thumb in transition radiation is that the radiation intensity generally decreases with the decrease of particle velocity v; as a result, low-energy particles are not favored in practice. Here, we find that there exist situations where transition radiation from particles with extremely low velocities (e.g., v/c<10−3) exhibits comparable intensity as that from high-energy particles (e.g., v/c=0.999), where c is the light speed in free space. The comparable radiation intensity implies an extremely high photon extraction efficiency from low-energy particles, up to 8 orders of magnitude larger than that from high-energy particles. This exotic phenomenon of low-velocity-favored transition radiation originates from the interference of the excited Ferrell-Berreman modes in an ultrathin epsilon-near-zero slab. Our findings may provide a promising route toward the design of integrated light sources based on low-energy electrons and specialized detectors for beyond-standard-model particles.

关键词： Atom or molecule scattering from surfaces Atomic & molecular collisions Cherenkov radiation Crystal optics Electron beams & optics Light-matter interaction Optical sources & detectors Optical transient phenomena Plasmonics

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Nearly Room-Temperature Ferromagnetism in a Pressure-Induced Correlated Metallic State of the van der Waals Insulator CrGeTe3

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Physical Review Letters 2021年第21期127卷 217203-217203页

作者： Dilip Bhoi Jun Gouchi Naoka Hiraoka Yufeng Zhang Norio Ogita Takumi Hasegawa Kentaro Kitagawa Hidenori Takagi Kee Hoon Kim Yoshiya Uwatoko The Institute for Solid State Physics University of Tokyo Kashiwa Chiba 277-8581 Japan Department of Physics Graduate School of Sciences University of Tokyo Tokyo 113-0033 Japan School of Physics Southeast University Nanjing 211189 China Graduate School of Integrated Arts and Sciences Hiroshima University Higashi-Hiroshima Hiroshima 739-8521 Japan Institute for Functional Matter and Quantum Technologies University of Stuttgart 70569 Stuttgart Germany Max Planck Institute for Solid State Research Heisenbergstraße 1 70569 Stuttgart Germany Department of Physics and Astronomy CeNSCMR Seoul National University Seoul 151-747 Republic of Korea Institute of Applied Physics Seoul National University Seoul 151-747 Republic of Korea

A complex interplay of different energy scales involving Coulomb repulsion, spin-orbit coupling, and Hund’s coupling energy in 2D van der Waals (vdW) material produces a novel emerging physical state. For instance, ferromagnetism in vdW charge transfer insulator CrGeTe3 provides a promising platform to simultaneously manipulate the magnetic and electrical properties for potential device implementation using few nanometers thick materials. Here, we show a continuous tuning of magnetic and electrical properties of a CrGeTe3 single crystal using pressure. With application of pressure, CrGeTe3 transforms from a ferromagnetic insulator with Curie temperature TC∼66 K at ambient condition to a correlated 2D Fermi metal with TC exceeding ∼250 K. Notably, absence of an accompanying structural distortion across the insulator-metal transition (IMT) suggests that the pressure induced modification of electronic ground states is driven by electronic correlation furnishing a rare example of bandwidth-controlled IMT in a vdW material.

关键词： Electrical conductivity Exchange interaction Ferromagnetism Hopping transport Magnetic susceptibility Second order phase transitions Spin-orbit coupling

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Polarization entanglement enabled by orthogonally stacked van der Waals NbOCl2 crystals

arXiv

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arXiv 2024年

作者： Guo, Qiangbing Wu, Yun-Kun Zhang, Di Zhang, Qiuhong Guo, Guang-Can Alù, Andrea Ren, Xi-Feng Qiu, Cheng-Wei Department of Electrical and Computer Engineering National University of Singapore Singapore Singapore Centre for Advanced 2D Materials Graphene Research Centre National University of Singapore Singapore Singapore CAS Key Laboratory of Quantum Information CAS Synergetic Innovation Center of Quantum Information & Quantum Physics University of Science and Technology of China Hefei China Hefei National Laboratory University of Science and Technology of China Hefei China Photonics Initiative Advanced Science Research Center City University of New York New York United States Physics Program Graduate Center City University of New York New York United States The Key Laboratory of Weak-Light Nonlinear Photonics Ministry of Education School of Physics TEDA Applied Physics Institute Nankai University Tianjin China School of Chemistry and Materials Science Hangzhou Institute for Advanced Study University of Chinese Academy of Sciences Hangzhou China

Polarization entanglement holds significant importance for photonic quantum technologies. Recently emerging subwavelength nonlinear quantum light sources, e.g., GaP and LiNbO3 thin films, benefiting from the relaxed phase-matching constraints and volume confinement, has shown intriguing properties, such as high-dimensional hyperentanglement and robust entanglement anti-degradation. Van der Waals (vdW) NbOCl2 crystal, renowned for its superior optical nonlinearities, has emerged as one of ideal candidates for ultrathin quantum light sources [Nature 613, 53 (2023)]. However, polarization-entanglement is inaccessible in NbOCl2 crystal due to its unfavorable nonlinear susceptibility tensor. Here, by leveraging the twist-stacking degree of freedom inherently in vdW systems, we showcase the preparation of tunable polarization entanglement and quantum Bell states. Our work not only provides a new and tunable polarization-entangled vdW photon-pair source, but also introduces a new knob in engineering the entanglement state of quantum light at the nanoscale. © 2024, CC BY-NC-ND.

关键词： Van der Waals forces

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