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18th IEEE International Conference on Machine Learning and Applications, ICMLA 2019

作者： Day, Rosemarie J. Salehi, Hassan Javadi, Mahsa Data Science Program Worcester Polytechnic Institute WorcesterMA United States Department of Electrical and Computer Engineering California State University Chico ChicoCA United States Division of Genetic Research University of Connecticut Health Center FarmingtonCT United States

ISBN: (纸本)9781728145495

Everyday migraines are affecting more than one billion people worldwide. This headache disorder is classified as the sixth most disabling disease in the world. Migraines are just one chronic illness affected by environmental triggers due to changes that occur inside the home. Migraines share this characteristic with sinus headaches and thus are often misdiagnosed. In this research work, an iOS-based environmental analyzer was designed, implemented and evaluated for migraine sufferers with the use of sensors. After the data collection and cleaning, five machine learning model were used to estimate prediction accuracy of migraines in terms of the environment. The data was evaluated against the models using K-Fold cross validation. The algorithm accuracy comparison showed that Linear Discriminant Analysis (LDA) produced highest accuracy for the testing data at a mean of 0.938. Preliminary results demonstrate the feasibility of using machine learning algorithms to perform the automated recognition of migraine trigger areas in the environment. © 2019 IEEE.

关键词： Internet of things

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A fully inkjet-printed disposable glucose sensor on paper

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npj Flexible Electronics 2018年第1期2卷 263-270页

作者： Eloïse Bihar Shofarul Wustoni Anna Maria Pappa Khaled N.Salama Derya Baran Sahika Inal Division of Biological and Environmental Science and Engineering King Abdullah University of Science and Technology(KAUST)Thuwal 23955Saudi Arabia Division of Physical Science and Engineering KAUST Solar CenterKAUSTThuwal 23955Saudi Arabia Department of Chemical Engineering and Biotechnology University of CambridgePhilippa Fawcett DriveCambridge CB30ASUK Division of Computer Electrical and Mathematical Sciences and EngineeringAdvanced Membranes and Porous Materials CenterKAUSTThuwal 23955Saudi Arabia

Inexpensive and easy-to-use diagnostic tools for fast health screening are imperative,especially in the developing world,where portability and affordability are a *** monitoring of metabolite levels can provide useful information regarding key metabolic activities of the body and detect the concomitant irregularities such as in the case of diabetes,a worldwide chronic ***,the majority of daily glucose monitoring tools rely on piercing the skin to draw *** pain and discomfort associated with finger pricking have created a global need to develop non-invasive,portable glucose *** this work,we develop a disposable analytical device which can measure physiologically relevant glucose concentrations in human saliva based on enzymatic electrochemical *** use inkjet-printing technology for the rapid and low-cost deposition of all the components of this glucose sensor,from the electronics to the biorecognition elements,on commercially available paper *** only electronic component of the sensor is the conducting polymer poly(3,4 ethylenedioxythiophene)doped with polystyrene sulfonate(PEDOT:PSS),while the biorecognition element comprises of the enzyme glucose oxidase coupled with an electron *** demonstrate that one month after its fabrication and storage in air-free environment,the sensor maintains its function with only minor performance *** fully printed,all-polymer biosensor with its ease of fabrication,accuracy,sensitivity and compatibility with easy-to-obtain biofluids such as saliva aids in the development of next generation low-cost,noninvasive,eco-friendly,and disposable diagnostic tools.

关键词： maintain sensor printing

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Magnetic Control of Soft Chiral Phonons in PbTe

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physical Review Letters 2022年第7期128卷 075901-075901页

作者： Andrey Baydin Felix G. G. Hernandez Martin Rodriguez-Vega Anderson K. Okazaki Fuyang Tay G. Timothy Noe, II Ikufumi Katayama Jun Takeda Hiroyuki Nojiri Paulo H. O. Rappl Eduardo Abramof Gregory A. Fiete Junichiro Kono Department of Electrical and Computer Engineering Rice University Houston Texas 77005 USA Smalley-Curl Institute Rice University Houston Texas 77005 USA Instituto de Física Universidade de São Paulo São Paulo São Paulo 05508-090 Brazil Theoretical Division Los Alamos National Laboratory Los Alamos New Mexico 87545 USA Laboratório Associado de Sensores e Materiais Instituto Nacional de Pesquisas Espaciais São José dos Campos São Paulo 12201-970 Brazil Applied Physics Graduate Program Smalley-Curl Institute Rice University Houston Texas 77005 USA Department of Physics Graduate School of Engineering Science Yokohama National University Yokohama 240-8501 Japan Institute for Materials Research Tohoku University Sendai 980-8577 Japan Department of Physics Northeastern University Boston Massachusetts 02115 USA Department of Physics Massachusetts Institute of Technology Cambridge Massachusetts 02139 USA Department of Physics and Astronomy Rice University Houston Texas 77005 USA Department of Material Science and NanoEngineering Rice University Houston Texas 77005 USA

PbTe crystals have a soft transverse optical phonon mode in the terahertz frequency range, which is known to efficiently decay into heat-carrying acoustic phonons, resulting in anomalously low thermal conductivity. Here, we studied this phonon via polarization-dependent terahertz spectroscopy. We observed softening of this mode with decreasing temperature, indicative of incipient ferroelectricity, which we explain through a model including strong anharmonicity with a quartic displacement term. In magnetic fields up to 25 T, the phonon mode splits into two modes with opposite handedness, exhibiting circular dichroism. Their frequencies display Zeeman splitting together with an overall diamagnetic shift with increasing magnetic field. Using a group-theoretical approach, we demonstrate that these observations are the result of magnetic field-induced morphic changes in the crystal symmetries through the Lorentz force exerted on the lattice ions. Thus, our Letter reveals a novel process of controlling phonon properties in a soft ionic lattice by a strong magnetic field.

关键词： Chirality Diamagnetism Magneto-dielectric effect Optical phonons Thermal conductivity Zeeman effect Terahertz time-domain spectroscopy

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Ultrahigh green and red optical gain cross-sections from solutions of colloidal quantum well heterostructures

arXiv

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arXiv 2020年

作者： Delikanli, Savas Erdem, Onur Isik, Furkan Baruj, Hameed Dehghanpour Shabani, Farzan Yagcı, Huseyin Bilge Demir, Hilmi Volkan Luminous! Center of Excellence for Semiconductor Lighting and Displays School of Electrical and Electronic Engineering Nanyang Technological University 50 Nanyang Avenue Singapore639798 Singapore Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University 21 Nanyang Link Singapore639798 Singapore Department of Electrical and Electronics Engineering Department of Physics UNAM Institute of Materials Science and Nanotechnology Bilkent University Ankara06800 Turkey

Optical gain in solution, which provides high photostability as a result of continuous regeneration of the gain medium, is extremely attractive for optoelectronic applications. Here, we propose and demonstrate amplified spontaneous emission (ASE) in solution with ultralow thresholds of 30 µJ/cm2 in red and of 44 µJ/cm2 in green from engineered colloidal quantum well (CQW) heterostructures. For this purpose, CdSe/CdS core/crown CQWs, designed to hit the green region, and CdSe/CdS@CdxZn1-xS core/crown@gradient-alloyed shell CQWs, further tuned to reach the red region by shell alloying, were employed to achieve high-performance ASE in the visible. The net modal gain of these CQWs reaches 530 cm-1 for the green and 201 cm-1 for the red, two orders of magnitude larger than those of colloidal quantum dots (QDs) in solution owing to intrinsically larger gain cross-sections of these CQWs. To explain the root cause for ultrahigh gain coefficient in solution, we show that for the first time that the gain cross-sections of these CQWs is ≥3.3×10-14 cm2 in the green and ≥1.3×10-14 cm2 in the red which are two orders magnitude larger compared to those of CQDs. These findings confirm the extraordinary prospects of these solution-processed CQWs as solution-based optical gain media in lasing applications. Copyright © 2020, The Authors. All rights reserved.

关键词： Optical gain

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High-energy gamma-ray observations above 10 GeV with CALET on the International Space Station

High-energy gamma-ray observations above 10 GeV with CALET o...

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37th International Cosmic Ray Conference, ICRC 2021

作者： Adriani, O. Akaike, Y. Asano, K. Asaoka, Y. Berti, E. Bigongiari, G. Binns, W.R. Bongi, M. Brogi, P. Bruno, A. Buckley, J.H. Cannady, N. Castellini, G. Checchia, C. Cherry, M.L. Collazuol, G. Ebisawa, K. Ficklin, A.W. Fuke, H. Gonzi, S. Guzik, T.G. Hams, T. Hibino, K. Ichimura, M. Ioka, K. Ishizaki, W. Israel, M.H. Kasahara, K. Kataoka, J. Kataoka, R. Katayose, Y. Kato, C. Kawanaka, N. Kawakubo, Y. Kobayashi, K. Kohri, K. Krawczynski, H.S. Krizmanic, J.F. Maestro, P. Marrocchesi, P.S. Messineo, A.M. Mitchell, J.W. Miyake, S. Moiseev, A.A. Mori, Masaki Mori, N. Motz, H.M. Munakata, K. Nakahira, S. Nishimura, J. de Nolfo, G.A. Okuno, S. Ormes, J.F. Ospina, N. Ozawa, S. Pacini, L. Papini, P. Rauch, B.F. Ricciarini, S.B. Sakai, K. Sakamoto, T. Sasaki, M. Shimizu, Y. Shiomi, A. Spillantini, P. Stolzi, F. Sugita, S. Sulaj, A. Takita, M. Tamura, T. Terasawa, T. Torii, S. Tsunesada, Y. Uchihori, Y. Vannuccini, E. Wefel, J.P. Yamaoka, K. Yanagita, S. Yoshida, A. Yoshida, K. Zober, W.V. Department of Physics University of Florence Via Sansone 1 Sesto Fiorentino 50019 Italy INFN Sezione di Florence Via Sansone 1 Sesto Fiorentino 50019 Italy Waseda Research Institute for Science and Engineering Waseda University 17 Kikuicho Shinjuku Tokyo162-0044 Japan JEM Utilization Center Human Spaceflight Technology Directorate Japan Aerospace Exploration Agency 2-1-1 Sengen Ibaraki Tsukuba305-8505 Japan Institute for Cosmic Ray Research The University of Tokyo 5-1-5 Kashiwa-no-Ha Chiba Kashiwa277-8582 Japan Department of Physical Sciences Earth and Environment University of Siena via Roma 56 Siena53100 Italy INFN Sezione di Pisa Polo Fibonacci Largo B. Pontecorvo 3 Pisa56127 Italy Department of Physics McDonnell Center for the Space Sciences Washington University One Brookings Drive St. LouisMO63130-4899 United States Heliospheric Physics Laboratory NASA/GSFC GreenbeltMD20771 United States Department of Physics Catholic University of America WashingtonDC20064 United States Center for Space Sciences and Technology University of Maryland Baltimore County 1000 Hilltop Circle BaltimoreMD21250 United States Astroparticle Physics Laboratory NASA/GSFC GreenbeltMD20771 United States Center for Research and Exploration in Space Sciences and Technology NASA/GSFC GreenbeltMD20771 United States Via Madonna del Piano 10 Sesto Fiorentino 50019 Italy Department of Physics and Astronomy Louisiana State University 202 Nicholson Hall Baton RougeLA70803 United States Department of Physics and Astronomy University of Padova Via Marzolo 8 Padova35131 Italy INFN Sezione di Padova Via Marzolo 8 Padova35131 Italy Institute of Space and Astronautical Science Japan Aerospace Exploration Agency 3-1-1 Yoshinodai Chuo Kanagawa Sagamihara252-5210 Japan Kanagawa University 3-27-1 Rokkakubashi Kanagawa Kanagawa Yokohama221-8686 Japan Faculty of Science and Technology Graduate School of Science and Technology Hirosaki Universi

Since the deployment of the CALorimetric Electron Telescope (CALET) on the exposure facility of the Japanese Experiment Module (JEM) 'Kibo' of the International Space Station in 2015, CALET is accumulating cosmic ray data steadily without any serious faults up to now. Although CALET is basically a high-energy cosmic-ray detector, its composite and thick detector structure allow us to separate gamma rays from charged cosmic rays clearly up the TeV energy region. In this paper, analysis of gamma-ray events above 10 GeV obtained by the 'high-energy' triggers, which is the basic trigger mode of CALET for cosmic-ray observations and is always effective regardless of the ISS position in orbit, are reported. Especially, good energy resolution (less than 3% at 10 GeV) of CALET enables us to search for spectral features in the gamma-ray energy spectrum such as lines possibly caused by annihilation of dark matter particles. Gamma-ray events above 10 GeV observed during five years of CALET operation have been analyzed to search for possible line signals in the energy spectra assuming various region-of-interests of the sky depending on the proposed Galactic density profile models. We found no hint of line signals and preliminary upper limits on parameters of the DM annihilation and decay models have been obtained. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

关键词： Gamma rays

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Comparative Analysis of Vee Antenna for Space Instrumentation

Comparative Analysis of Vee Antenna for Space Instrumentatio...

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TEQIP III Sponsored International Conference on Microwave Integrated Circuits, Photonics and Wireless Networks (IMICPW)

作者： V R Dinesh Kumar Jayesh P. Pabari Sonam Jitarwal Kinsuk Acharyya Department of Electrical and Electronics Engineering BITS Pilani Hyderabad Campus Hyderabad India Planetary Science Division Physical Research Laboratory Ahmedabad India

ISBN: (纸本)9781728118826

Most planetary missions contain instruments capable of recording radio emissions. The antenna is one such useful tool to detect electric field of radio emissions. Characterising the antenna is essential to better understand the signals observed and also to design front end and back end electronics. In this work, we analyse different Vee antenna configurations and present an empirical formula of induced voltage across antenna terminal for each case. A comparison of their suitability for space application is also presented.

关键词： Helical antennas Electric fields Lightning Dipole antennas Dynamic range Satellite broadcasting

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Performance of joint gamma-ray observations with MAGIC and LST-1 telescopes 38

Performance of joint gamma-ray observations with MAGIC and L...

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38th International Cosmic Ray Conference, ICRC 2023

作者： Di Pierro, F. Berti, A. de Menezes, R. Jobst, E. Ohtani, Y. Sitarek, J. Suda, Y. Visentin, E. Abe, H. Abe, K. Abe, S. Abhir, J. Acciari, V.A. Aguasca-Cabot, A. Agudo, I. Alvarez Crespo, N. Aniello, T. Ansoldi, S. Antonelli, L.A. Aramo, C. Arbet-Engels, A. Cornelia, A. Artero, M. Asano, K. Aubert, P. Baack, D. Babić, A. Baktash, A. Bamba, A. Baquero Larriva, A. Baroncelli, L. Barres de Almeida, U. Barrio, J.A. Batkovic, I. Baxter, J. Becerra González, J. Bednarek, W. Bernardini, E. Bernardos, M.I. Bernete Medrano, J. Besenrieder, J. Bhattacharjee, P. Biederbeck, N. Bigongiari, C. Biland, A. Bissaldi, E. Blanch, O. Bonnoli, G. Bordas, P. Bošnjak, Ž. Bulgarelli, A. Burelli, I. Burmistrov, L. Buscemi, M. Busetto, G. Campoy-Ordaz, A. Cardillo, M. Caroff, S. Carosi, A. Carosi, R. Carrasco, M.S. Carretero-Castrillo, M. Cassol, F. Castro-Tirado, A.J. Cauz, D. Cerasole, D. Ceribella, G. Chai, Y. Cheng, K. Chiavassa, A. Chikawa, M. Chilingarian, A. Chytka, L. Cifuentes, A. Cikota, S. Colombo, E. Contreras, J.L. Cortina, J. Costantini, H. Covino, S. D’Amico, G. Dalchenko, M. D’Elia, V. Da Vela, P. Dazzi, F. De Angelis, A. de Bony de Lavergne, M. De Lotto, B. De Lucia, M. de Menezes, R. Del Peral, L. Deleglise, G. Delfino, M. Delgado, C. Delgado Mengual, J. della Volpe, D. Dellaiera, M. Del Popolo, A. Depaoli, D. Di Piano, A. Di Pierro, F. Di Pilato, A. Di Tria, R. Di Venere, L. Díaz, C. Dominik, R.M. Dominis Prester, D. Donini, A. Dorner, D. Doro, M. Eisenberger, L. Elsässer, D. Emery, G. Escudero, J. Fallah Ramazani, V. Fariña, L. Fattorini, A. Ferrara, G. Ferrarotto, F. Fiasson, A. Foffano, L. Font, L. Freixas Coromina, L. Fröse, S. Fukami, S. Fukazawa, Y. Garcia, E. Garcia López, R. Garczarczyk, M. Gasbarra, C. Gasparrini, D. Gasparyan, S. Gaug, M. Geyer, D. Giesbrecht Paiva, J. Giglietto, N. Giordano, F. Gliwny, P. Godinovic, N. Grau, R. Green, J. Green, D. Gunji, S. Günther, P. Hackfeld, J. Hadasch, D. Hahn, A. Hashiyama, K. Hassan, T. Hayashi, K. INFN Torino Via P. Giuria 1 Torino Italy Max-Planck-Institut für Physik Föhringer Ring 6 München Germany Università degli Studi di Torino Dipartimento di Fisica Via P. Giuria 1 Torino Italy University of Tokyo Institute for Cosmic Ray Research 5-1-5 Kashiwa-no-ha Chiba Kashiwa277-8582 Japan University of Lodz Faculty of Physics and Applied Informatics ul. Pomorska 149-153 Lodz Poland Hiroshima University Physics Program Graduate School of Advanced Science and Engineering Hiroshima739-8526 Japan Department of Physics Tokai University Japan ETH Zürich Switzerland Instituto de Astrofísica de Canarias Departamento de Astrofísica Universidad de La Laguna Spain Departament de Física Quàntica i Astrofísica Institut de Ciències del Cosmos Universitat de Barcelona IEEC-UB Spain Instituto de Astrofísica de Andalucía-CSIC Spain EMFTEL department IPARCOS Universidad Complutense de Madrid Spain Italy INFN Sezione di Trieste Università degli Studi di Udine Italy Italy INAF - Osservatorio Astronomico di Roma Italy INFN Sezione di Napoli Italy INFN Sezione di Padova Università degli Studi di Padova Italy The Barcelona Institute of Science and Technology Spain LAPP Univ. Grenoble Alpes Univ. Savoie Mont Blanc CNRS-IN2P3 Annecy France Department of Physics TU Dortmund University Germany Croatia Universität Hamburg Institut für Experimentalphysik Germany Graduate School of Science University of Tokyo Japan Universidad del Azuay Ecuador INAF - Osservatorio di Astrofisica e Scienza dello spazio di Bologna Italy Centro Brasileiro de Pesquisas Físicas Brazil CIEMAT Spain INFN Sezione di Bari Politecnico di Bari Italy INAF - Osservatorio Astronomico di Brera Italy University of Geneva Département de physique nucléaire et corpusculaire Switzerland INFN Sezione di Catania Italy Departament de Física CERES-IEEC Universitat Autónoma de Barcelona Spain Italy Università di Pisa INFN Pisa Italy Aix Marseille Univ CNRS IN2P3 CPPM France INFN Sezione di Bari

The prototype Large-Sized Telescope (LST-1) of the Cherenkov Telescope Array Observatory (CTAO) is in commissioning phase at the Observatorio del Roque de Los Muchachos at 2200 m a.s.l. in La Palma (Canary Islands, Spain). LST-1 is a 23-m diameter telescope and is the first of four that will compose the LST part of the CTAO Northern array. The LST subarray is optimized to provide the best sensitivity for gamma rays in the 20 GeV - 200 GeV energy range. The MAGIC telescopes, which are located approximately 100 m from the LST-1, is operating as a two 17-m telescope stereoscopic system for more than 14 years. LST-1 and MAGIC routinely perform joint observations of gamma-ray sources to exploit the potential of the three-telescope system. This contribution describes the analysis pipeline and evaluates the performance of the system using Monte Carlo simulations and data on the Crab Nebula. The sensitivity achieved during joint observations with MAGIC and LST-1 is about 30% higher than that of MAGIC alone. © Copyright owned by the author(s) under the terms of the Creative Commons.

关键词： Stereo image processing

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Toggling near-field directionality via polarization control of surface waves

arXiv

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arXiv 2021年

作者： Zhong, Yuhan Lin, Xiao Jiang, Jing Yang, Yi Liu, Gui-Geng Xue, Haoran Low, Tony Chen, Hongsheng Zhang, Baile Interdisciplinary Center for Quantum Information State Key Laboratory of Modern Optical Instrumentation ZJU-Hangzhou Global Science and Technology Innovation Center College of Information Science and Electronic Engineering Zhejiang University Hangzhou310027 China International Joint Innovation Center ZJU-UIUC Institute Zhejiang University Haining314400 China School of Applied Science Beijing Information Science and Technology University Beijing100192 China Research Laboratory of Electronics Department of Physics Massachusetts Institute of Technology CambridgeMA02139 United States Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University Singapore637371 Singapore Department of Electrical and Computer Engineering University of Minnesota MinneapolisMN55455 United States Centre for Disruptive Photonic Technologies Nanyang Technological University Singapore637371 Singapore

Directional excitation of guidance modes is central to many applications ranging from light harvesting, optical information processing to quantum optical technology. Of paramount interest, especially, the active control of near-field directionality provides a new paradigm for the real-time on-chip manipulation of light. Here we find that for a given dipolar source, its near-field directionality can be toggled efficiently via tailoring the polarization of surface waves that are excited, for example, via tuning the chemical potential of graphene in a graphene-metasurface waveguide. This finding enables a feasible scheme for the active near-field directionality. Counterintuitively, we reveal that this scheme can transform a circular electric/magnetic dipole into a Huygens dipole in the near-field coupling. Moreover, for Janus dipoles, this scheme enables us to actively flip their near-field coupling and non-coupling faces. © 2021, CC BY.

关键词： Surface waves

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Complications in the ALMA detection of phosphine at Venus

arXiv

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arXiv 2021年

作者： Akins, Alex B. Lincowski, Andrew P. Meadows, Victoria S. Steffes, Paul G. Jet Propulsion Laboratory California Institute of Technology Instruments Division PasadenaCA91011 United States Department of Astronomy and Astrobiology Program University of Washington Box 351580 SeattleWA98195 United States NASA Nexus for Exoplanet System Science Virtual Planetary Laboratory Team University of Washington Box 351580 SeattleWA98195 United States School of Electrical and Computer Engineering Georgia Institute of Technology AtlantaGA30308 United States

Recently published ALMA observations suggest the presence of 20 ppb PH3 in the upper clouds of Venus. This is an unexpected result, as PH3 does not have a readily apparent source and should be rapidly photochemically destroyed according to our current understanding of Venus atmospheric chemistry. While the reported PH3 spectral line at 266.94 GHz is nearly co-located with an SO2 spectral line, the non-detection of stronger SO2 lines in the wideband ALMA data is used to rule out SO2 as the origin of the feature. We present a reassessment of wideband and narrowband datasets derived from these ALMA observations. The ALMA observations are re-reduced following both the initial and revised calibration procedures discussed by the authors of the original study. We also investigate the phenomenon of apparent spectral line dilution over varying spatial scales resulting from the ALMA antenna configuration. A 266.94 GHz spectral feature is apparent in the narrowband data using the initial calibration procedures, but this same feature can not be identified following calibration revisions. The feature is also not reproduced in the wideband data. While the SO2 spectral line is not observed at 257.54 GHz in the ALMA wideband data, our dilution simulations suggest that SO2 abundances greater than the previously suggested 10 ppb limit would also not be detected by ALMA. Additional millimeter, sub-millimeter, and infrared observations of Venus should be undertaken to further investigate the possibility of PH3 in the Venus atmosphere. © 2021, CC BY-NC-SA.

关键词： Antennas

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Observation of ferromagnetic phase in the second moiré band of twisted MoTe2

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Nature Communications 2025年第1期16卷 1-7页

作者： An, Liheng Pan, Haiyang Qiu, Wen-Xuan Wang, Naizhou Ru, Shihao Tan, Qinghai Dai, Xuran Cai, Xiangbin Shang, Qiuyu Lu, Xiufang Jiang, Hao Lyu, Xiaodan Yang, Shunshun Watanabe, Kenji Taniguchi, Takashi Wu, Fengcheng Gao, Wei-Bo Division of Physics and Applied Physics School of Physical and Mathematical Sciences Nanyang Technological University Singapore Singapore School of Physics and Technology Wuhan University Wuhan China Department of Physics School of Science and Research Center for Industries of the Future Westlake University Hangzhou China Institute of Natural Sciences Westlake Institute for Advanced Study Hangzhou China Centre for Quantum Technologies Nanyang Technological University Singapore Singapore School of microelectronics University of Science and Technology of China Hefei China Research Center for Electronic and Optical Materials National Institute for Materials Science Tsukuba Japan Research Center for Materials Nanoarchitectonics National Institute for Materials Science Tsukuba Japan School of Electrical and Electronic Engineering Nanyang Technological University Singapore Singapore National Centre for Advanced Integrated Photonics (NCAIP) Singapore Nanyang Technological University Singapore Singapore Quantum Science and Engineering Centre (QSec) Nanyang Technological University Singapore Singapore

Flat bands and electron correlation in moiré lattices give rise to many exotic phases, including Mott insulators, superconductivity, and topological states. Within the first moiré band, integer and fractional quantum anomalous Hall effects have been observed in twisted bilayer MoTe2 (tMoTe2) at one hole doping and fractional doping per moiré unit cell, respectively. When the second moiré band is fully hole doped, quantum spin Hall insulator has also been reported in tMoTe2 at a certain twist angle. Exotic topological states together with ferromagnetic (FM) states in the high moiré band can potentially exist as well. In this study, we report the observation of a FM phase in the second moiré band in tMoTe2. The FM phase can be tuned by both the doping level and displacement field. At filling around 2.58 holes per moiré unit cell, the FM phase reaches a Curie temperature of 3.5 K. A large displacement field can suppress the FM phase, like the FM phase at the filling of −1. Our results demonstrate the realization of time-reversal symmetry-breaking states in the higher moiré bands in tMoTe2.

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