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Erratum: "A structural modeling approach to solid solutions based on the similar atomic environment" [J. Chem. Phys. 153, 034101 (2020)]

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The Journal of chemical physics 2020年第8期153卷 089901页

作者： Fuyang Tian De-Ye Lin Xingyu Gao Ya-Fan Zhao Hai-Feng Song Institute for Applied Physics Beijing Key Laboratory for Magneto-Photoelectrical Composite and Interface Science University of Science and Technology Beijing Beijing 100083 China. CAEP Software Center for High Performance Numerical Simulation Beijing 100088 China. Institute of Applied Physics and Computational Mathematics Beijing 100088 China.

Due to a misunderstanding at the proof stage, the authors’ contribution was not stated clearly in the original paper.1 Additionally, the information on the co-c

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Probe of the Solar Magnetic Field Using the “Cosmic-Ray Shadow” of the Sun

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Physical Review Letters 2013年第1期111卷 011101-011101页

作者： M. Amenomori X. J. Bi D. Chen T. L. Chen W. Y. Chen S. W. Cui Danzengluobu L. K. Ding C. F. Feng Zhaoyang Feng Z. Y. Feng Q. B. Gou Y. Q. Guo K. Hakamada H. H. He Z. T. He K. Hibino N. Hotta Haibing Hu H. B. Hu J. Huang H. Y. Jia L. Jiang F. Kajino K. Kasahara Y. Katayose C. Kato K. Kawata Labaciren G. M. Le A. F. Li H. J. Li W. J. Li C. Liu J. S. Liu M. Y. Liu H. Lu X. R. Meng K. Mizutani K. Munakata H. Nanjo M. Nishizawa M. Ohnishi I. Ohta H. Onuma S. Ozawa X. L. Qian X. B. Qu T. Saito T. Y. Saito M. Sakata T. K. Sako J. Shao M. Shibata A. Shiomi T. Shirai H. Sugimoto M. Takita Y. H. Tan N. Tateyama S. Torii H. Tsuchiya S. Udo H. Wang H. R. Wu L. Xue Y. Yamamoto Z. Yang S. Yasue A. F. Yuan T. Yuda L. M. Zhai H. M. Zhang J. L. Zhang X. Y. Zhang Y. Zhang Yi Zhang Ying Zhang Zhaxisangzhu X. X. Zhou Department of Physics Hirosaki University Hirosaki 036-8561 Japan Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Hebei Normal University Shijiazhuang 050016 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics SouthWest Jiaotong University Chengdu 610031 China Department of Natural Science and Mathematics Chubu University Kasugai 487-8501 Japan Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Department of Physics Konan University Kobe 658-8501 Japan Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan School of Information Science and Engineering Shandong Agriculture University Taian 271018 China Saitama University Saitama 338-8570 Japan National Institute of Informatics Tokyo 101-8430 Japan Sakushin Gakuin University Utsunomiya 321-3295 Japan Tokyo Metropolitan College of Industrial Technology Tokyo 116-8523 Japan Max-Planck-Institut für Physik München D-80805 Germany College of Industrial Technology Nihon University Narashino 275-8576 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Japan Atomic Energy Agency Tokai-mura 319-1195 Japan School of General Education Shinshu University Matsumoto 390-8621 Japan

We report on a clear solar-cycle variation of the Sun’s shadow in the 10 TeV cosmic-ray flux observed by the Tibet air shower array during a full solar cycle from 1996 to 2009. In order to clarify the physical implications of the observed solar cycle variation, we develop numerical simulations of the Sun’s shadow, using the potential field source surface model and the current sheet source surface (CSSS) model for the coronal magnetic field. We find that the intensity deficit in the simulated Sun’s shadow is very sensitive to the coronal magnetic field structure, and the observed variation of the Sun’s shadow is better reproduced by the CSSS model. This is the first successful attempt to evaluate the coronal magnetic field models by using the Sun’s shadow observed in the TeV cosmic-ray flux.

关键词： Cosmic rays

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Tensor-Networks-based Learning of Probabilistic Cellular Automata Dynamics

arXiv

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arXiv 2024年

作者： Casagrande, Heitor P. Xing, Bo Munro, William J. Guo, Chu Poletti, Dario Science Mathematics and Technology Cluster Singapore University of Technology and Design 8 Somapah Road Singapore487372 Singapore Okinawa Institute of Science Technology Graduate University Onna-son Okinawa904-0495 Japan Key Laboratory of Low-Dimensional Quantum Structures and Quantum Control of Ministry of Education Department of Physics and Synergetic Innovation Center for Quantum Effects and Applications Hunan Normal University Changsha410081 China EPD Pillar Singapore University of Technology and Design 8 Somapah Road Singapore487372 Singapore Centre for Quantum Technologies National University of Singapore Singapore117543 Singapore MajuLab CNRS-UNS-NUS-NTU International Joint Research Unit UMI 3654 Singapore Singapore

Algorithms developed to solve many-body quantum problems, like tensor networks, can turn into powerful quantum-inspired tools to tackle problems in the classical domain. In this work, we focus on matrix product operators, a prominent numerical technique to study many-body quantum systems, especially in one dimension. It has been previously shown that such a tool can be used for classification, learning of deterministic sequence-to-sequence processes and of generic quantum processes. We further develop a matrix product operator algorithm to learn probabilistic sequence-to-sequence processes and apply this algorithm to probabilistic cellular automata. This new approach can accurately learn probabilistic cellular automata processes in different conditions, even when the process is a probabilistic mixture of different chaotic rules. In addition, we find that the ability to learn these dynamics is a function of the bit-wise difference between the rules and whether one is much more likely than the other. Copyright © 2024, The Authors. All rights reserved.

关键词： Tensors

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Anthropogenic Influences on the Extremely Dry and Hot Summer of 2020 in Southern China and Projected Changes in the Likelihood of the Event

SSRN

引用

SSRN 2024年

作者： Wang, Kaixi Zheng, Zhiyuan Zhu, Xian Dong, Wenjie Tett, Simon F.B. Dong, Buwen Zhang, Wenxia Lott, Fraser C. Bu, Lulei Wang, Yumiao Li, Huixin Nanding, Nergui Freychet, Nicolas Wang, Dongqian Qiao, Shaobo Ministry of Education Sun Yat-sen University Zhuhai China Zhuhai Branch State Key Laboratory of Earth Surface Process and Resource Ecology Advanced Institute of Natural Sciences Beijing Normal University Zhuhai China School of Geosciences University of Edinburgh Edinburgh United Kingdom National Centre for Atmospheric Science Department of Meteorology University of Reading Reading United Kingdom State Key Laboratory of Numerical Modeling for Atmospheric Sciences and Geophysical Fluid Dynamics Institute of Atmospheric Physics Chinese Academy of Sciences Beijing China Met Office Hadley Centre ExeterEX1 3PB United Kingdom Department of Atmospheric and Oceanic Sciences Institute of Atmospheric Sciences IRDR International Center of Excellence on Risk Interconnectivity and Governance on Weather/Climate Extremes Impact and Public Health Fudan University Shanghai China School of Hydrology and Water Resources Nanjing University of Information Science and Technology Nanjing China Collaborative Innovation Center on Forecast and Evaluation of Meteorological Disasters Key Laboratory of Meteorological Disasters Ministry of Education Joint International Research Laboratory of Climate and Environment Change Nanjing University of Information Science and Technology Nanjing China School of Earth Sciences Yunnan University Kunming China National Climate Center China Meteorological Administration Beijing China State Key Laboratory of Earth Surface Processes and Resource Ecology Faculty of Geographical Science Beijing Normal University Beijing China Zhuhai China

During summer 2020, Southern China experienced an extremely dry and hot summer, which was identified as one of the top ten domestic weather and climate extreme events in 2020 by China Meteorological Administration. Summer mean precipitation, surface air temperature (TAS), and number of hot days (NHD) were about 25% dryer, 1.5℃ warmer, and 11 days larger than the 1981–2010 normal. These are the 4th largest precipitation deficit, the highest TAS, and the 2nd highest NHD in the 1961–2020 record. The large-scale circulation anomalies over the West Pacific increased the likelihood of these extremely event. Anthropogenic influences on this event were investigated using 525-member ensembles of the atmosphere-only HadGEM3-GA6 model and the multi-model ensembles from the Coupled Model Intercomparison Project Phase 6 (CMIP6). Anthropogenic forcings doubled (increased by 11%) the probability of precipitation deficits, and increased occurrence more than [[EQUATION]] times for both TAS anomaly (1.25[[EQUATION]] probability higher) and NHD anomaly (300% probability higher) in HadGEM-GA6 (CMIP6). That means that the 2020-like TAS and NHD anomalies would not occur without anthropogenic forcings, and there is weak evidence that human influences decrease rainfall over Southern China. However, the precipitation deficit increased the likelihood of exceeding the observed thresholds for both TAS and NHD by about 17 (4) and 9 (11) times in HadGEM3-GA6 (CMIP6), respectively. Under SSP2-4.5 and SSP5-8.5 scenarios in the future, 2020-like hot but wet extreme events increase in magnitude and frequency, while the frequency of dry events declines. © 2024, The Authors. All rights reserved.

关键词： Climate models

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Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun

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Physical Review Letters 2018年第3期120卷 031101-031101页

作者： M. Amenomori X. J. Bi D. Chen T. L. Chen W. Y. Chen S. W. Cui Danzengluobu L. K. Ding C. F. Feng Zhaoyang Feng Z. Y. Feng Q. B. Gou Y. Q. Guo H. H. He Z. T. He K. Hibino N. Hotta Haibing Hu H. B. Hu J. Huang H. Y. Jia L. Jiang F. Kajino K. Kasahara Y. Katayose C. Kato K. Kawata M. Kozai Labaciren G. M. Le A. F. Li H. J. Li W. J. Li C. Liu J. S. Liu M. Y. Liu H. Lu X. R. Meng T. Miyazaki K. Mizutani K. Munakata T. Nakajima Y. Nakamura H. Nanjo M. Nishizawa T. Niwa M. Ohnishi I. Ohta S. Ozawa X. L. Qian X. B. Qu T. Saito T. Y. Saito M. Sakata T. K. Sako J. Shao M. Shibata A. Shiomi T. Shirai H. Sugimoto M. Takita Y. H. Tan N. Tateyama S. Torii H. Tsuchiya S. Udo H. Wang H. R. Wu L. Xue Y. Yamamoto K. Yamauchi Z. Yang A. F. Yuan T. Yuda L. M. Zhai H. M. Zhang J. L. Zhang X. Y. Zhang Y. Zhang Yi Zhang Ying Zhang Zhaxisangzhu X. X. Zhou Department of Physics Hirosaki University Hirosaki 036-8561 Japan Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences Beijing 100049 China National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China Department of Mathematics and Physics Tibet University Lhasa 850000 China Department of Physics Hebei Normal University Shijiazhuang 050016 China Department of Physics Shandong University Jinan 250100 China Institute of Modern Physics SouthWest Jiaotong University Chengdu 610031 China Faculty of Engineering Kanagawa University Yokohama 221-8686 Japan Faculty of Education Utsunomiya University Utsunomiya 321-8505 Japan Department of Physics Konan University Kobe 658-8501 Japan Research Institute for Science and Engineering Waseda University Tokyo 169-8555 Japan Faculty of Engineering Yokohama National University Yokohama 240-8501 Japan Department of Physics Shinshu University Matsumoto 390-8621 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa 277-8582 Japan Institute of Space and Astronautical Science Japan Aerospace Exploration Agency (ISAS/JAXA) Sagamihara Kanagawa 252-5210 Japan National Center for Space Weather China Meteorological Administration Beijing 100081 China School of Information Science and Engineering Shandong Agriculture University Taian 271018 China Saitama University Saitama 338-8570 Japan National Institute of Informatics Tokyo 101-8430 Japan Sakushin Gakuin University Utsunomiya 321-3295 Japan College of Science China University of Petroleum Qingdao 266555 China Tokyo Metropolitan College of Industrial Technology Tokyo 116-8523 Japan Max-Planck-Institut für Physik München D-80805 Deutschland Escuela de Ciencias Físicas y Nanotechnología Yachay Tech Imbabura 100115 Ecuador College of Industrial Technology Nihon University Narashino 275-8576 Japan Shonan Institute of Technology Fujisawa 251-8511 Japan Japan Atomic Energy Agency Tokai-mu

We analyze the Sun’s shadow observed with the Tibet-III air shower array and find that the shadow’s center deviates northward (southward) from the optical solar disk center in the “away” (“toward”) interplanetary magnetic field (IMF) sector. By comparing with numerical simulations based on the solar magnetic field model, we find that the average IMF strength in the away (toward) sector is 1.54±0.21stat±0.20syst (1.62±0.15stat±0.22syst) times larger than the model prediction. These demonstrate that the observed Sun’s shadow is a useful tool for the quantitative evaluation of the average solar magnetic field.

关键词： Cosmic ray propagation Sun Interplanetary magnetic field Cosmic rays & astroparticles

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Scalar induced gravitational waves in modified teleparallel gravity theories

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Physical Review D 2023年第12期107卷 124019-124019页

作者： Charalampos Tzerefos Theodoros Papanikolaou Emmanuel N. Saridakis Spyros Basilakos National Observatory of Athens Lofos Nymfon 11852 Athens Greece Department of Physics National & Kapodistrian University of Athens Zografou Campus GR 157 73 Athens Greece CAS Key Laboratory for Researches in Galaxies and Cosmology Department of Astronomy University of Science and Technology of China Hefei Anhui 230026 People’s Republic of China Departamento de Matemáticas Universidad Católica del Norte Avenida Angamos 0610 Casilla 1280 Antofagasta Chile Academy of Athens Research Center for Astronomy and Applied Mathematics Soranou Efesiou 4 11527 Athens Greece School of Sciences European University Cyprus Diogenes Street Engomi 1516 Nicosia Cyprus

Primordial black holes (PBHs) forming out of the collapse of enhanced cosmological perturbations provide access to the early Universe through their associated observational signatures. In particular, enhanced cosmological perturbations collapsing to form PBHs are responsible for the generation of a stochastic gravitational-wave background (SGWB) induced by second-order gravitational interactions, usually called scalar induced gravitational waves (SIGWs). This SGWB is sensitive to the underlying gravitational theory; hence it can be used as a novel tool to test the standard paradigm of gravity and constrain possible deviations from general relativity. In this work, we study the aforementioned GW signal within modified teleparallel gravity theories, developing a formalism for the derivation of the GW spectral abundance within any form of gravitational action. At the end, working within viable f(T,ϕ) models without matter-gravity couplings, and accounting for the effect of monoparametric f(T) gravity at the level of the source and the propagation of the tensor perturbations, we show that the respective GW signal is indistinguishable from that within GR. Interestingly, we find that in order to break the degeneracy between different f(T) theories through the portal of SIGWs one should necessarily consider nonminimal matter-gravity couplings at the level of the gravitational action.

关键词： Alternative gravity theories Cosmology Gravitation Gravitational wave sources Gravitational waves Inflation

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A two-stage solution to quantum process tomography: error analysis and optimal design

arXiv

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arXiv 2024年

作者： Xiao, Shuixin Wang, Yuanlong Zhang, Jun Dong, Daoyi Mooney, Gary J. Petersen, Ian R. Yonezawa, Hidehiro School of Engineering and Technology University of New South Wales CanberraACT2600 Australia University of Michigan–Shanghai Jiao Tong University Joint Institute Shanghai Jiao Tong University Shanghai200240 China School of Engineering The Australian National University CanberraACT2601 Australia Key Laboratory of Systems and Control Academy of Mathematics and Systems Science Chinese Academy of Sciences Beijing100190 China CIICADA Lab School of Engineering Australian National University ACT2601 Australia School of Physics The University of Melbourne ParkvilleVIC3010 Australia School of Physics University of Melbourne ParkvilleVIC3010 Australia School of Engineering Australian National University ACT2601 Australia RIKEN Center for Quantum Computing Japan Centre for Quantum Computation and Communication Technology Australian Research Council CanberraACT2600 Australia

Quantum process tomography is a critical task for characterizing the dynamics of quantum systems and achieving precise quantum control. In this paper, we propose a two-stage solution for both trace-preserving and non-trace-preserving quantum process tomography. Utilizing a tensor structure, our algorithm exhibits a computational complexity of O(MLd2) where d is the dimension of the quantum system and M, L represent the numbers of different input states and measurement operators, respectively. We establish an analytical error upper bound and then design the optimal input states and the optimal measurement operators, which are both based on minimizing the error upper bound and maximizing the robustness characterized by the condition number. numerical examples and testing on IBM quantum devices are presented to demonstrate the performance and efficiency of our algorithm. Copyright © 2024, The Authors. All rights reserved.

关键词： Error analysis

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Responses of the Tropical Atmospheric Circulation to Climate Change and Connection to the Hydrological Cycle

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Earth and Planetary sciences 1000年第1期46卷 549-580页

作者： Jian Ma Robin Chadwick Kyong-Hwan Seo Changming Dong Gang Huang Gregory R. Foltz Jonathan H. Jiang 1College of Marine Sciences Shanghai Ocean University 201306 Shanghai China email: majian@*** 2Met Office Hadley Centre Exeter EX1 3PB United Kingdom email: robin.chadwick@metoffice.gov.uk 3Department of Atmospheric Sciences Pusan National University Busan 46279 South Korea email: khseo@pusan.ac.kr 5Department of Atmospheric and Oceanic Sciences University of California Los Angeles California 90095 USA email: cdong@atmos.ucla.edu 4School of Marine Sciences Nanjing University of Information Science and Technology 210044 Nanjing China 9University of Chinese Academy of Sciences 100049 Beijing China 6State Key Laboratory of Numerical Modeling for Atmospheric Sciences and Geophysical Fluid Dynamics Institute of Atmospheric Physics Chinese Academy of Sciences 100029 Beijing China email: hg@*** 7Qingdao National Laboratory for Marine Science and Technology 266237 Qingdao China 8Joint Center for Global Change Studies 100875 Beijing China 10Atlantic Oceanographic and Meteorological Laboratory National Oceanic and Atmospheric Administration Miami Florida 33149 USA email: gregory.foltz@noaa.gov 11Jet Propulsion Laboratory California Institute of Technology Pasadena California 91109 USA email: jonathan.h.jiang@jpl.nasa.gov

This review describes the climate change–induced responses of the tropical atmospheric circulation and their impacts on the hydrological cycle. We depict the theoretically predicted changes and diagnose physical mechanisms for observational and model-projected trends in large-scale and regional climate. The tropical circulation slows down with moisture and stratification changes, connecting to a poleward expansion of the Hadley cells and a shift of the intertropical convergence zone. Redistributions of regional precipitation consist of thermodynamic and dynamical components, including a strong offset between moisture increase and circulation weakening throughout the tropics. This allows other dynamical processes to dominate local circulation changes, such as a surface warming pattern effect over oceans and multiple mechanisms over land. To improve reliability in climate projections, more fundamental understandings of pattern formation, circulation change, and the balance of various processes redistributing land rainfall are suggested to be important.

关键词： climate change tropical atmospheric circulation ocean precipitation sea surface temperature land rainfall Hadley circulation

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First test of lepton flavor universality in the charmed baryon decays Ωc0→Ω−ℓ+νℓ using data of the Belle experiment

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Physical Review D 2022年第9期105卷 L091101-L091101页

作者： Y. B. Li C. P. Shen I. Adachi H. Aihara S. Al Said D. M. Asner H. Atmacan T. Aushev R. Ayad V. Babu S. Bahinipati P. Behera K. Belous J. Bennett F. Bernlochner M. Bessner B. Bhuyan T. Bilka A. Bobrov D. Bodrov J. Borah A. Bozek M. Bračko P. Branchini T. E. Browder A. Budano M. Campajola D. Červenkov M.-C. Chang P. Chang V. Chekelian A. Chen B. G. Cheon K. Chilikin H. E. Cho K. Cho S.-J. Cho S.-K. Choi Y. Choi S. Choudhury D. Cinabro S. Cunliffe N. Dash G. De Nardo G. De Pietro R. Dhamija F. Di Capua J. Dingfelder Z. Doležal T. V. Dong T. Ferber D. Ferlewicz B. G. Fulsom R. Garg V. Gaur N. Gabyshev A. Giri P. Goldenzweig B. Golob E. Graziani K. Gudkova C. Hadjivasiliou T. Hara K. Hayasaka H. Hayashii M. T. Hedges W.-S. Hou K. Inami G. Inguglia A. Ishikawa R. Itoh M. Iwasaki Y. Iwasaki W. W. Jacobs E.-J. Jang S. Jia Y. Jin K. K. Joo J. Kahn K. H. Kang T. Kawasaki H. Kichimi C. Kiesling C. H. Kim D. Y. Kim K.-H. Kim K. T. Kim Y.-K. Kim K. Kinoshita P. Kodyš T. Konno A. Korobov S. Korpar E. Kovalenko P. Križan R. Kroeger P. Krokovny M. Kumar R. Kumar K. Kumara A. Kuzmin Y.-J. Kwon K. Lalwani T. Lam M. Laurenza S. C. Lee J. Li L. K. Li Y. Li L. Li Gioi J. Libby K. Lieret D. Liventsev A. Martini M. Masuda D. Matvienko S. K. Maurya M. Merola K. Miyabayashi R. Mizuk G. B. Mohanty M. Nakao D. Narwal A. Natochii L. Nayak M. Nayak N. K. Nisar S. Nishida K. Ogawa S. Ogawa H. Ono P. Oskin P. Pakhlov G. Pakhlova T. Pang S. Pardi S.-H. Park S. Patra S. Paul T. K. Pedlar R. Pestotnik L. E. Piilonen T. Podobnik E. Prencipe M. T. Prim M. Röhrken A. Rostomyan N. Rout G. Russo D. Sahoo S. Sandilya A. Sangal L. Santelj V. Savinov G. Schnell J. Schueler C. Schwanda Y. Seino K. Senyo M. E. Sevior M. Shapkin C. Sharma V. Shebalin J.-G. Shiu B. Shwartz J. B. Singh A. Sokolov E. Solovieva M. Starič Z. S. Stottler M. Sumihama T. Sumiyoshi M. Takizawa U. Tamponi K. Tanida F. Tenchini M. Uchida T. Uglov Y. Unno K. Uno S. Uno P. Urquijo S. E. Vahsen R. Van Tonder G. Varner A. Vinokurova E. Waheed D. Wang E. Wang M.-Z. Wang S. Watanuki E. Won Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) and Institute of Modern Physics Fudan University Shanghai 200443 High Energy Accelerator Research Organization (KEK) Tsukuba 305-0801 SOKENDAI (The Graduate University for Advanced Studies) Hayama 240-0193 Department of Physics University of Tokyo Tokyo 113-0033 Department of Physics Faculty of Science University of Tabuk Tabuk 71451 Department of Physics Faculty of Science King Abdulaziz University Jeddah 21589 Brookhaven National Laboratory Upton New York 11973 University of Cincinnati Cincinnati Ohio 45221 National Research University Higher School of Economics Moscow 101000 Deutsches Elektronen–Synchrotron 22607 Hamburg Indian Institute of Technology Bhubaneswar Satya Nagar 751007 Indian Institute of Technology Madras Chennai 600036 Institute for High Energy Physics Protvino 142281 University of Mississippi University Mississippi 38677 University of Bonn 53115 Bonn University of Hawaii Honolulu Hawaii 96822 Indian Institute of Technology Guwahati Assam 781039 Faculty of Mathematics and Physics Charles University 121 16 Prague Budker Institute of Nuclear Physics SB RAS Novosibirsk 630090 Novosibirsk State University Novosibirsk 630090 P.N. Lebedev Physical Institute of the Russian Academy of Sciences Moscow 119991 H. Niewodniczanski Institute of Nuclear Physics Krakow 31-342 Faculty of Chemistry and Chemical Engineering University of Maribor 2000 Maribor J. Stefan Institute 1000 Ljubljana INFN—Sezione di Roma Tre I-00146 Roma INFN—Sezione di Napoli I-80126 Napoli Università di Napoli Federico II I-80126 Napoli Department of Physics Fu Jen Catholic University Taipei 24205 Department of Physics National Taiwan University Taipei 10617 Max-Planck-Institut für Physik 80805 München National Central University Chung-li 32054 Department of Physics and Institute of Natural Sciences Hanyang University Seoul 04763 Korea Institute of Science and Technology Information Daejeon 34141 Yonsei University Seoul 0372

We present the first observation of the Ωc0→Ω−μ+νμ decay and present measurements of the branching fraction ratios of the Ωc0→Ω−ℓ+νℓ decays compared to the reference mode Ωc0→Ω−π+, (ℓ=e or μ). This analysis is based on 89.5 fb−1, 711 fb−1, and 121.1 fb−1 data samples collected with the Belle detector at the KEKB asymmetric-energy e+e− collider at the center-of-mass energies of 10.52 GeV, 10.58 GeV, and 10.86 GeV, respectively. The Ωc0 signal yields are extracted by fitting MΩℓ and MΩπ spectra. The branching fraction ratios B(Ωc0→Ω−e+νe)/B(Ωc0→Ω−π+) and B(Ωc0→Ω−μ+νμ)/B(Ωc0→Ω−π+) are measured to be 1.98±0.13(stat)±0.08(syst) and 1.94±0.18(stat)±0.10(syst), respectively. The ratio of B(Ωc0→Ω−e+νe)/B(Ωc0→Ω−μ+νμ) is measured to be 1.02±0.10(stat)±0.02(syst), which is consistent with the expectation of lepton flavor universality.

关键词： Branching fraction Leptonic, semileptonic & radiative decays Charmed baryons Lepton colliders

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Scalar induced gravitational waves in modified teleparallel gravity theories

arXiv

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arXiv 2023年

作者： Tzerefos, Charalampos Papanikolaou, Theodoros Saridakis, Emmanuel N. Basilakos, Spyros National Observatory of Athens Lofos Nymfon Athens11852 Greece Department of Physics National & Kapodistrian University of Athens Zografou Campus GR 157 73 Athens Greece CAS Key Laboratory for Researches in Galaxies and Cosmology Department of Astronomy University of Science and Technology of China Anhui Hefei230026 China Departamento de Matemáticas Universidad Católica del Norte Avda. Angamos 0610 Casilla Antofagasta1280 Chile Academy of Athens Research Center for Astronomy and Applied Mathematics Soranou Efesiou 4 Athens11527 Greece School of Sciences European University Cyprus Diogenes Street Engomi Nicosia1516 Cyprus

Primordial black holes (PBHs) forming out of the collapse of enhanced cosmological perturbations provide access to the early Universe through their associated observational signatures. In particular, enhanced cosmological perturbations collapsing to form PBHs are responsible for the generation of a stochastic gravitational-wave background (SGWB) induced by second-order gravitational interactions, usually called scalar induced gravitational waves (SIGWs). This SGWB is sensitive to the underlying gravitational theory;hence it can be used as a novel tool to test the standard paradigm of gravity and constrain possible deviations from general relativity. In this work, we study the aforementioned GW signal within modified teleparallel gravity theories, developing a formalism for the derivation of the GW spectral abundance within any form of gravitational action. At the end, working within viable f(T, φ) models without matter-gravity couplings, and accounting for the effect of mono-parametric f(T) gravity at the level of the source and the propagation of the tensor perturbations, we show that the respective GW signal is indistinguishable from that within GR. Interestingly, we find that in order to break the degeneracy between different f(T) theories through the portal of SIGWs one should necessarily consider non-minimal matter-gravity couplings at the level of the gravitational action. Copyright © 2023, The Authors. All rights reserved.

关键词： Gravity waves

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