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Model-independent Approach of the JUNO 8B solar Neutrino Program

the Astrophysical Journal 2024年第2期965卷 122-122页

作者： Jie Zhao Baobiao Yue Haoqi Lu Yufeng Li Jiajie Ling Zeyuan Yu Angel Abusleme thomas Adam shakeel Ahmad Rizwan Ahmed sebastiano Aiello Muhammad Akram Abid Aleem tsagkarakis Alexandros Fengpeng An Qi An Giuseppe Andronico Nikolay Anfimov Vito Antonelli tatiana Antoshkina Burin Asavapibhop João Pedro Athayde Marcondes de André Didier Auguste Weidong Bai Nikita Balashov Wander Baldini Andrea Barresi Davide Basilico Eric Baussan Marco Bellato Antonio Bergnoli thilo Birkenfeld sylvie Blin David Blum simon Blyth Anastasia Bolshakova Mathieu Bongrand Clément Bordereau Dominique Breton Augusto Brigatti Riccardo Brugnera Riccardo Bruno Antonio Budano Jose Busto ilya Butorov Anatael Cabrera Barbara Caccianiga Hao Cai Xiao Cai Yanke Cai Zhiyan Cai Riccardo Callegari Antonio Cammi Agustin Campeny Chuanya Cao Guofu Cao Jun Cao Rossella Caruso Cédric Cerna Chi Chan Jinfan Chang Yun Chang Guoming Chen Pingping Chen Po-An Chen shaomin Chen Xurong Chen Yixue Chen Yu Chen Zhiyuan Chen Zikang Chen Jie Cheng Yaping Cheng Alexander Chepurnov Alexey Chetverikov Davide Chiesa Pietro Chimenti Artem Chukanov Gérard Claverie Catia Clementi Barbara Clerbaux Marta Colomer Molla selma Conforti Di Lorenzo Daniele Corti Flavio Dal Corso Olivia Dalager Christophe De La taille Zhi Deng Ziyan Deng Wilfried Depnering Marco Diaz Xuefeng Ding Yayun Ding Bayu Dirgantara sergey Dmitrievsky tadeas Dohnal Dmitry Dolzhikov Georgy Donchenko Jianmeng Dong Evgeny Doroshkevich Marcos Dracos Frédéric Druillole Ran Du shuxian Du stefano Dusini Martin Dvorak timo Enqvist Heike Enzmann Andrea Fabbri Donghua Fan Lei Fan Jian Fang Wenxing Fang Marco Fargetta Dmitry Fedoseev Zhengyong Fei Li-Cheng Feng Qichun Feng Richard Ford Amélie Fournier Haonan Gan Feng Gao Alberto Garfagnini Arsenii Gavrikov Marco Giammarchi Nunzio Giudice Maxim Gonchar Guanghua Gong Hui Gong Yuri Gornushkin Alexandre Göttel Marco Grassi Maxim Gromov Vasily Gromov Minghao Gu Xiaofei Gu Yu Gu Mengyun Guan Yuduo Guan Nunzio Guardone Cong Guo Jingyuan Guo Wanlei Guo Xinheng Guo Yuhang Guo Paul Ha Institute of High Energy Physics Beijing People's Republic of China liyufeng@*** Sun Yat-Sen University Guangzhou People's Republic of China lingjj5@*** Pontificia Universidad Católica de Chile Santiago Chile Millennium Institute for SubAtomic Physics at the High-energy Frontier (SAPHIR) ANID Chile IPHC Université de Strasbourg CNRS/IN2P3 F-67037 Strasbourg France Pakistan Institute of Nuclear Science and Technology Islamabad Pakistan INFN Catania and Dipartimento di Fisica e Astronomia dell Università di Catania Catania Italy III. Physikalisches Institut B RWTH Aachen University Aachen Germany East China University of Science and Technology Shanghai People's Republic of China University of Science and Technology of China Hefei People's Republic of China Joint Institute for Nuclear Research Dubna Russia INFN Sezione di Milano and Dipartimento di Fisica dell Università di Milano Milano Italy Department of Physics Faculty of Science Chulalongkorn University Bangkok Thailand IJCLab Université Paris-Saclay CNRS/IN2P3 91405 Orsay France Department of Physics and Earth Science University of Ferrara and INFN Sezione di Ferrara Ferrara Italy INFN Milano Bicocca and University of Milano Bicocca Milano Italy INFN Sezione di Padova Padova Italy Eberhard Karls Universität Tübingen Physikalisches Institut Tübingen Germany SUBATECH Nantes Université IMT Atlantique CNRS-IN2P3 Nantes France Université Bordeaux CNRS LP2i Bordeaux UMR 5797 F-33170 Gradignan France Department of Physics National Taiwan University Taipei Dipartimento di Fisica e Astronomia dell’Università di Padova and INFN Sezione di Padova Padova Italy University of Roma Tre and INFN Sezione Roma Tre Roma Italy Centre de Physique des Particules de Marseille Marseille France Wuhan University Wuhan People's Republic of China INFN Milano Bicocca and Politecnico of Milano Milano Italy Institute of Physics National Yang Ming Chiao Tung University Hsinchu National United University Miao-Li Guangxi Uni

the physics potential of detecting 8B solar neutrinos will be exploited at the Jiangmen Underground Neutrino Observatory (JUNO), in a model-independent manner by using three distinct channels of the charged current (C...

the physics potential of detecting 8sup>B solar neutrinos will be exploited at the Jiangmen Underground Neutrino Observatory (JUNO), in a model-independent manner by using three distinct channels of the charged current (CC), neutral current (NC), and elastic scattering (Es) interactions. Due to the largest-ever mass of 13sup>C nuclei in the liquid scintillator detectors and the expected low background level, 8sup>B solar neutrinos are observable in the CC and NC interactions on 13sup>C for the first time. By virtue of optimized event selections and muon veto strategies, backgrounds from the accidental coincidence, muon-induced isotopes, and external backgrounds can be greatly suppressed. Excellent signal-to-background ratios can be achieved in the CC, NC, and Es channels to guarantee the observation of the 8sup>B solar neutrinos. From the sensitivity studies performed in this work, we show that JUNO, with 10 yr of data, can reach the 1σi> precision levels of 5%, 8%, and 20% for the 8sup>B neutrino flux, ${\sin }^{2}{\theta }_{12}$ tainer class="MathJax CtxtMenu_Attached_0" jax="CHtML" tabindex="0" ctxtmenu_counter="0" style="font-size: 107.5%; position: relative;">th class="MJX-tEX" aria-hidden="true">sup>texatom texclass="ORD">i class="mjx-n">ss="mjx-c73">ss="mjx-c69">ss="mjx-c6E">i>texatom>scri.t.style="vertical-align: 0.396em;">texatom size="s" texclass="ORD">ss="mjx-n">ss="mjx-c32">

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Measurement of the cosmogenic neutron yield in super-Kamiokande with gadolinium loaded water

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Physical Review D 2023年第9期107卷 092009-092009页

作者： M. shinoki K. Abe Y. Hayato K. Hiraide K. Hosokawa K. ieki M. ikeda J. Kameda Y. Kanemura R. Kaneshima Y. Kashiwagi Y. Kataoka s. Miki s. Mine M. Miura s. Moriyama Y. Nakano M. Nakahata s. Nakayama Y. Noguchi K. Okamoto K. sato H. sekiya H. shiba K. shimizu M. shiozawa Y. sonoda Y. suzuki A. takeda Y. takemoto A. takenaka H. tanaka s. Watanabe t. Yano s. Han t. Kajita K. Okumura t. tashiro t. tomiya X. Wang s. Yoshida G. D. Megias P. Fernandez L. Labarga N. Ospina B. Zaldivar B. W. Pointon E. Kearns J. L. Raaf L. Wan t. Wester J. Bian N. J. Griskevich W. R. Kropp s. Locke M. B. smy H. W. sobel V. takhistov A. Yankelevich J. Hill s. H. Lee D. H. Moon R. G. Park B. Bodur K. scholberg C. W. Walter A. Beauchêne L. Bernard A. Coffani O. Drapier s. El Hedri A. Giampaolo th. A. Mueller A. D. santos P. Paganini B. Quilain t. ishizuka t. Nakamura J. s. Jang J. G. Learned K. Choi s. Cao L. H. V. Anthony D. Martin M. scott A. A. sztuc Y. Uchida V. Berardi M. G. Catanesi E. Radicioni N. F. Calabria A. Langella L. N. Machado G. De Rosa G. Collazuol F. iacob M. Lamoureux M. Mattiazzi L. Ludovici M. Gonin G. Pronost C. Fujisawa Y. Maekawa Y. Nishimura R. Akutsu M. Friend t. Hasegawa t. ishida t. Kobayashi M. Jakkapu t. Matsubara t. Nakadaira K. Nakamura Y. Oyama K. sakashita t. sekiguchi t. tsukamoto N. Bhuiyan t. Boschi G. t. Burton F. Di Lodovico J. Gao A. Goldsack t. Katori J. Migenda M. taani Z. Xie s. Zsoldos Y. Kotsar H. Ozaki A. t. suzuki Y. takeuchi C. Bronner J. Feng t. Kikawa M. Mori t. Nakaya R. A. Wendell K. Yasutome s. J. Jenkins N. McCauley P. Mehta A. tarrant K. M. tsui Y. Fukuda Y. itow H. Menjo K. Ninomiya J. Lagoda s. M. Lakshmi M. Mandal P. Mijakowski Y. s. Prabhu J. Zalipska M. Jia J. Jiang C. K. Jung M. J. Wilking C. Yanagisawa M. Harada H. ishino s. ito H. Kitagawa Y. Koshio F. Nakanishi s. sakai G. Barr D. Barrow L. Cook s. samani D. Wark A. Holin F. Nova J. Y. Yang B. s. Yang J. Yoo J. E. P. Fannon L. Kneale M. Malek J. M. McElwee O. stone M. D. thiesse L. F. thompson H. Okazawa s. B. Kim E. Kwon J. W. s Department of Physics Faculty of Science and Technology Tokyo University of Science Noda Chiba 278-8510 Japan Kamioka Observatory Institute for Cosmic Ray Research University of Tokyo Kamioka Gifu 506-1205 Japan Kavli Institute for the Physics and Mathematics of the Universe (WPI) The University of Tokyo Institutes for Advanced Study University of Tokyo Kashiwa Chiba 277-8583 Japan Department of Physics and Astronomy University of California Irvine Irvine California 92697-4575 USA Research Center for Cosmic Neutrinos Institute for Cosmic Ray Research University of Tokyo Kashiwa Chiba 277-8582 Japan ILANCE CNRS—University of Tokyo International Research Laboratory Kashiwa Chiba 277-8582 Japan Institute for Cosmic Ray Research University of Tokyo Kashiwa Chiba 277-8582 Japan Department of Theoretical Physics University Autonoma Madrid 28049 Madrid Spain Department of Physics British Columbia Institute of Technology Burnaby British Columbia V5G 3H2 Canada TRIUMF 4004 Wesbrook Mall Vancouver British Columbia V6T2A3 Canada Department of Physics Boston University Boston Massachusetts 02215 USA High Energy Accelerator Research Organization (KEK) Tsukuba Ibaraki 305-0801 Japan Department of Physics California State University Dominguez Hills Carson California 90747 USA Institute for Universe and Elementary Particles Chonnam National University Gwangju 61186 Korea Department of Physics Duke University Durham North Carolina 27708 USA Ecole Polytechnique IN2P3-CNRS Laboratoire Leprince-Ringuet F-91120 Palaiseau France Junior College Fukuoka Institute of Technology Fukuoka Fukuoka 811-0295 Japan Department of Physics Gifu University Gifu Gifu 501-1193 Japan GIST College Gwangju Institute of Science and Technology Gwangju 500-712 Korea Department of Physics and Astronomy University of Hawaii Honolulu Hawaii 96822 USA Institute for Basic Science (IBS) Daejeon 34126 Korea Institute For Interdisciplinary Research in Science and Education ICISE

Cosmic-ray muons that enter the super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. these are a major background source for studies of MeV-scale neutrinos and searches for rare events. in 2020, gadolinium was introduced into the ultra-pure water in the super-Kamiokande detector to improve the detection efficiency of neutrons. in this study, the cosmogenic neutron yield was measured using data acquired during the period after the gadolinium loading. the yield was found to be (2.76±0.02(stat)±0.19(syst))×10−4 μ−1 g−1 cm2 at an average muon energy 259 GeV at the super-Kamiokande detector.

关键词： Particle interactions Cherenkov detectors

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Comparative Analysis of Photonic Bandgap and transmittance in iD Photonic Crystals 5

Comparative Analysis of Photonic Bandgap and Transmittance i...

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5th iEEE Uttar Pradesh section international Conference on Electrical, Electronics and computer engineering, UPCON 2018

作者： Mishra, Upendra Kumar Chandel, Vishal singh Vibhu, isht singh, Prabal Pratap Department of Physics Integral University Lucknow226026 India Department of Applied Science and Humanities Rajkiya Engineering College Ambedkar Nagar224122 India Department of Physics YD.P. G. College Lakhimpur Kheri262701 India Department of Physics U.I.E.T. C.S.J.M. Kanpur University Kanpur208024 India

ISBN: (纸本)9781538650028

in this article, the variation of photonic bandgap and transmittance for one-dimensional dielectric periodic layered structure with angles of incidence have been studied. it gives the working of s-polarized electromagnetic wave, as tunable s-polarized filter, which stops the p-polarized wave. two material structures Air/AgNO3and Air/Pb2O, have been studied. the transmittance in (Air/Pb2O) has been found to be better. transmission of the wave best appears at increase in incidence angle. © 2018 iEEE.

关键词： Energy gap

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Erratum to: search for heavy Higgs bosons decaying to a top quark pair in proton-proton collisions at s = 13 teV

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Journal of High Energy Physics 2022年第3期2022卷 1-21页

作者： sirunyan, A. M. tumasyan, A. Adam, W. Ambrogi, F. Bergauer, t. Brandstetter, J. Dragicevic, M. Erö, J. Escalante Del Valle, A. Flechl, M. Frühwirth, R. Jeitler, M. Krammer, N. Krätschmer, i. Liko, D. Madlener, t. Mikulec, i. Rad, N. schieck, J. schöfbeck, R. spanring, M. spitzbart, D. Waltenberger, W. Wulz, C.-E. Zarucki, M. Drugakov, V. Mossolov, V. suarez Gonzalez, J. Darwish, M. R. De Wolf, E. A. Di Croce, D. Janssen, X. Lauwers, J. Lelek, A. Pieters, M. Rejeb sfar, H. Van Haevermaet, H. Van Mechelen, P. Van Putte, s. Van Remortel, N. Blekman, F. Bols, E. s. Chhibra, s. s. D’Hondt, J. De Clercq, J. Lontkovskyi, D. Lowette, s. Marchesini, i. Moortgat, s. Moreels, L. Python, Q. skovpen, K. tavernier, s. Van Doninck, W. Van Mulders, P. Van Parijs, i. Beghin, D. Bilin, B. Brun, H. Clerbaux, B. De Lentdecker, G. Delannoy, H. Dorney, B. Favart, L. Grebenyuk, A. Kalsi, A. K. Luetic, J. Popov, A. Postiau, N. starling, E. thomas, L. Vander Velde, C. Vanlaer, P. Vannerom, D. Cornelis, t. Dobur, D. Khvastunov, i. Niedziela, M. Roskas, C. trocino, D. tytgat, M. Verbeke, W. Vermassen, B. Vit, M. Zaganidis, N. Bondu, O. Bruno, G. Caputo, C. David, P. Delaere, C. Delcourt, M. Giammanco, A. Lemaitre, V. Magitteri, A. Prisciandaro, J. saggio, A. Vidal Marono, M. Vischia, P. Zobec, J. Alves, F. L. Alves, G. A. Correia silva, G. Hensel, C. Moraes, A. Rebello teles, P. Belchior Batista Das Chagas, E. Carvalho, W. Chinellato, J. Coelho, E. Da Costa, E. M. Da silveira, G. G. De Jesus Damiao, D. De Oliveira Martins, C. Fonseca De souza, s. Huertas Guativa, L. M. Malbouisson, H. Martins, J. Matos Figueiredo, D. Medina Jaime, M. Melo De Almeida, M. Mora Herrera, C. Mundim, L. Nogima, H. Prado Da silva, W. L. sanchez Rosas, L. J. santoro, A. sznajder, A. thiel, M. tonelli Manganote, E. J. torres Da silva De Araujo, F. Vilela Pereira, A. Ahuja, s. Bernardes, C. A. Calligaris, L. Fernandez Perez tomei, t. R. Gregores, E. M. Lemos, D. s. Mercadante, P. G. Novaes, s. F. Padula, sandra s. Aleksandrov, A. Antchev, G. Hadjiiska, R. iaydjiev, Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Wien Austria Vienna University of Technology Vienna Austria Institute for Nuclear Problems Minsk Belarus Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Ghent University Ghent Belgium IRFU CEA Université Paris-Saclay Gif-sur-Yvette France Université Catholique de Louvain Louvain-la-Neuve Belgium Centro Brasileiro de Pesquisas Fisicas Rio de Janeiro Brazil Universidade do Estado do Rio de Janeiro Rio de Janeiro Brazil Universidade Estadual de Campinas Campinas Brazil Federal University of Rio Grande do Sul Porto Alegre Brazil UFMS Nova Andradina Brazil Universidade Federal de Pelotas Pelotas Brazil Universidade Estadual Paulista São Paulo Brazil Universidade Federal do ABC São Paulo Brazil Institute for Nuclear Research and Nuclear Energy Bulgarian Academy of Sciences Sofia Bulgaria University of Sofia Sofia Bulgaria Beihang University Beijing China Department of Physics Tsinghua University Beijing China Institute of High Energy Physics Beijing China University of Chinese Academy of Sciences Beijing China State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China Universidad de Los Andes Bogota Colombia Universidad de Antioquia Medellin Colombia University of Split Faculty of Electrical Engineering Mechanical Engineering and Naval Architecture Split Croatia University of Split Faculty of Science Split Croatia Institute Rudjer Boskovic Zagreb Croatia Institute for Theoretical and Experimental Physics named by A.I. Alikhanov of NRC ‘Kurchatov Institute’ Moscow Russia University of Cyprus Nicosia Cyprus Charles University Prague Czech Republic Joint Institute for Nuclear Research Dubna Russia Escuela Politecnica Nacional Quito Ecuador Universidad San Francisco de Quito Quito Ecuador Cairo University Cairo Egypt Academy of Scientific Research and Technolog

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History and Habitability of the LP 890-9 Planetary system

arXiv

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arXiv 2024年

作者： Barnes, Rory do Amaral, Laura N.R. Birky, Jessica Carone, Ludmila Driscoll, Peter Livesey, Joseph R. Graham, David Becker, Juliette Cui, Kaiming schlecker, Martin Garcia, Rodolfo Gialluca, Megan Adams, Arthur Ahmed, M.D. Redyan Bonney, Paul Broussard, Wynter Chawla, Chetan Damasso, Mario Danchi, William C. Deitrick, Russell Ducrot, Elsa Fromont, Emeline F. Gaches, Brandt A.L. Gupta, sakshi Hill, Michelle L. Jackman, James A.G. Janin, Estelle M. Karawacki, Mikolaj Koren, Matheus Daniel Greca, Roberto La Leung, Michaela Miranda-Rosete, Arturo Olohoy, Michael Kent A. Ngo, Cecelia Paul, Daria sahu, Chandan Kumar sarkar, Debajyoti Basu shadab, Mohammad Afzal schwieterman, Edward W. sedler, Melissa texeira, Katie Vazan, Allona Delgado Vega, Karen N. Vijayakumar, Rohit Wojack, Jonathan t. Astronomy Department University of Washington Box 315180 SeattleWA98195 United States Instituto de Ciencias Nucleares Universidad Nacional Autónoma de México CDMX Cto. Exterior S/N C.U. Coyoacán Ciudad de México04510 Mexico Space Research Institute Austrian Academy of Sciences Schmiedlstrasse 6 GrazA-8042 Austria Centre for Exoplanet Science School of Physics & Astronomy University of St Andrews North Haugh St AndrewsKY169SS United Kingdom Earth and Planets Laboratory Carnegie Institution for Science 5241 Broad Branch Rd WashingtonDC20015 United States Department of Astronomy University of Wisconsin–Madison 475 N. Charter Street MadisonWI53706 United States Universität Heidelberg Albert-Ueberle-Str. Heidelberg2 69120 Germany Division of Geological and Planetary Sciences California Institute of Technology PasadenaCA91125 United States Tsung-Dao Lee Institute Shanghai Jiao Tong University 800 Dongchuan Road Shanghai200240 China Steward Observatory Department of Astronomy The University of Arizona TucsonAZ85721 United States Department of Earth and Planetary Sciences University of California RiversideCA92521 United States Department of Physical Sciences Indian Institute of Science Education and Research West Bengal Kolkata741246 India Department of Physics University of Arkansas 825 W. Dickson St. FayettevilleAR72701 United States Independent Researcher New Delhi110027 India INAF Osservatorio Astrofisico di Torino Via Osservatorio 20 TO Pino TorineseI-10025 Italy NASA Goddard Space Flight Center Exoplanets and Stellar Astrophysics Laboratory GreenbeltMD20771 United States School of Earth and Ocean Sciences University of Victoria VictoriaBC Canada AIM CEA CNRS Université Paris-Saclay Université de Paris Gif-sur-YvetteF-91191 France Paris Region Fellow Marie Sklodowska-Curie Action France Department of Astronomy University of Maryland College ParkMD20742 United States Department of Space Earth & Environment Cha

We present numerous aspects of the evolution of the LP 890-9 (sPECULOOs-2/tOi-4306) planetary system, focusing on the likelihood that planet c can support life. We find that the host star reaches the main sequence in 1 Gyr and that planet c lies close to the inner boundary of the habitable zone. We find the magma ocean stage can last up to 50 Myr, remove 8 Earth-oceans of water, and leave up to 2000 bars of oxygen in the atmosphere. However, if the planet forms with a hydrogen envelope as small as 0.1 Earth-masses, no water will be lost during the star’s pre-main sequence phase from thermal escape processes. We find that the planets are unlikely to be in a 3:1 mean motion resonance and that both planets tidally circularize within 0.5 Gyr when tidal dissipation is held constant. However, if tidal dissipation is a function of mantle temperature and rheology, then we find that planet c’s orbit may require more than 7 Gyr to circularize, during which time tidal heating may reach hundreds of terawatts. We thus conclude that the habitability of planet c depends most strongly on the initial volatile content and internal properties, but no data yet preclude the viability of an active biosphere on the planet. © 2024, CC BY.

关键词： stars

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Measurements of inclusive and differential cross sections for the Higgs boson production and decay to four-leptons in proton-proton collisions at s = 13 teV

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Journal of High Energy Physics 2023年第8期2023卷 1-80页

作者： Hayrapetyan, A. tumasyan, A. Adam, W. Andrejkovic, J.W. Bergauer, t. Chatterjee, s. Damanakis, K. Dragicevic, M. Escalante Del Valle, A. Hussain, P.s. Jeitler, M. Krammer, N. Lechner, L. Liko, D. Mikulec, i. schieck, J. schöfbeck, R. schwarz, D. sonawane, M. templ, s. Waltenberger, W. Wulz, C.-E. Darwish, M.R. Janssen, t. Kello, t. Van Mechelen, P. Bols, E.s. D’Hondt, J. De Moor, A. Delcourt, M. El Faham, H. Lowette, s. Makarenko, i. Morton, A. Müller, D. sahasransu, A.R. tavernier, s. Van Putte, s. Vannerom, D. Clerbaux, B. Dansana, s. De Lentdecker, G. Favart, L. Hohov, D. Jaramillo, J. Lee, K. Mahdavikhorrami, M. Malara, A. Paredes, s. Pétré, L. Postiau, N. thomas, L. Vanden Bemden, M. Vander Velde, C. Vanlaer, P. De Coen, M. Dobur, D. Knolle, J. Lambrecht, L. Mestdach, G. Rendón, C. samalan, A. skovpen, K. tytgat, M. Van Den Bossche, N. Vermassen, B. Wezenbeek, L. Benecke, A. Bruno, G. Bury, F. Caputo, C. Delaere, C. Donertas, i.s. Giammanco, A. Jaffel, K. Jain, sa. Lemaitre, V. Lidrych, J. Mastrapasqua, P. Mondal, K. tran, t.t. Wertz, s. Alves, G.A. Coelho, E. Hensel, C. Moraes, A. Rebello teles, P. Aldá Júnior, W.L. Alves Gallo Pereira, M. Barroso Ferreira Filho, M. Brandao Malbouisson, H. Carvalho, W. Chinellato, J. Da Costa, E.M. Da silveira, G.G. De Jesus Damiao, D. Dos santos sousa, V. Fonseca De souza, s. Martins, J. Mora Herrera, C. Mota Amarilo, K. Mundim, L. Nogima, H. santoro, A. silva Do Amaral, s.M. sznajder, A. thiel, M. Vilela Pereira, A. Bernardes, C.A. Calligaris, L. Fernandez Perez tomei, t.R. Gregores, E.M. Mercadante, P.G. Novaes, s.F. Orzari, B. Padula, sandra s. Aleksandrov, A. Antchev, G. Hadjiiska, R. iaydjiev, P. Misheva, M. shopova, M. sultanov, G. Dimitrov, A. ivanov, t. Litov, L. Pavlov, B. Petkov, P. Petrov, A. shumka, E. Keshri, s. thakur, s. Cheng, t. Guo, Q. Javaid, t. Mittal, M. Yuan, L. Bauer, G. Hu, Z. Yi, K. Chen, G.M. Chen, H.s. Chen, M. iemmi, F. Jiang, C.H. Kapoor, A. Liao, H. Liu, Z.-A. Monti, F. sharma, R. song, J.N. tao, J. Wang, J. Zhang, C. Zhang, H. Agapitos, A. Ba Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Vienna Austria Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Ghent University Ghent Belgium Université Catholique de Louvain Louvain-la-Neuve Belgium Centro Brasileiro de Pesquisas Fisicas Rio de Janeiro Brazil Universidade do Estado do Rio de Janeiro Rio de Janeiro Brazil Universidade Estadual Paulista Universidade Federal do ABC São Paulo Brazil Institute for Nuclear Research and Nuclear Energy Bulgarian Academy of Sciences Sofia Bulgaria University of Sofia Sofia Bulgaria Instituto De Alta Investigación Universidad de Tarapacá Casilla 7 D Arica Chile Beihang University Beijing China Department of Physics Tsinghua University Beijing China Institute of High Energy Physics Beijing China State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China Sun Yat-Sen University Guangzhou China University of Science and Technology of China Hefei China Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE) — Fudan University Shanghai China Zhejiang University Zhejiang Hangzhou China Universidad de Los Andes Bogota Colombia Universidad de Antioquia Medellin Colombia University of Split Faculty of Electrical Engineering Mechanical Engineering and Naval Architecture Split Croatia University of Split Faculty of Science Split Croatia Institute Rudjer Boskovic Zagreb Croatia University of Cyprus Nicosia Cyprus Charles University Prague Czech Republic Escuela Politecnica Nacional Quito Ecuador Universidad San Francisco de Quito Quito Ecuador Academy of Scientific Research and Technology of the Arab Republic of Egypt Egyptian Network of High Energy Physics Cairo Egypt Center for High Energy Physics (CHEP-FU) Fayoum University El-Fayoum Egypt National Institute of Chemical Physics and Biophysics Tallinn Estonia Department of Physics

Measurements of the inclusive and differential fiducial cross sections for the Higgs boson production in the H → ZZ → 4ℓ (ℓ = e, μ) decay channel are presented. the results are obtained from the analysis of proton-proton collision data recorded by the CMs experiment at the CERN LHC at a center-of-mass energy of 13 teV, corresponding to an integrated luminosity of 138 fb−1sup>. the measured inclusive fiducial cross section is 2.73 ± 0.26 fb, in agreement with the standard model expectation of 2.86 ± 0.1 fb. Differential cross sections are measured as a function of several kinematic observables sensitive to the Higgs boson production and decay to four leptons. A set of double-differential measurements is also performed, yielding a comprehensive characterization of the four leptons final state. Constraints on the Higgs boson trilinear coupling and on the bottom and charm quark coupling modifiers are derived from its transverse momentum distribution. All results are consistent with theoretical predictions from the standard model. © the Author(s) 2023.

关键词： Hadron-Hadron scattering Higgs Physics

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search for high-mass resonances in final states with a τ-lepton and missing transverse momentum with the AtLAs detector

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Physical Review D 2024年第11期109卷 112008-112008页

作者： G. Aad B. Abbott D. C. Abbott A. Abed Abud K. Abeling D. K. Abhayasinghe s. H. Abidi H. Abramowicz H. Abreu Y. Abulaiti A. C. Abusleme Hoffman B. s. Acharya B. Achkar L. Adam C. Adam Bourdarios L. Adamczyk L. Adamek s. V. Addepalli J. Adelman A. Adiguzel s. Adorni t. Adye A. A. Affolder Y. Afik C. Agapopoulou M. N. Agaras J. Agarwala A. Aggarwal C. Agheorghiesei J. A. Aguilar-saavedra A. Ahmad F. Ahmadov W. s. Ahmed X. Ai G. Aielli i. Aizenberg s. Akatsuka M. Akbiyik t. P. A. Åkesson A. V. Akimov K. Al Khoury G. L. Alberghi J. Albert P. Albicocco M. J. Alconada Verzini s. Alderweireldt M. Aleksa i. N. Aleksandrov C. Alexa t. Alexopoulos A. Alfonsi F. Alfonsi M. Alhroob B. Ali s. Ali M. Aliev G. Alimonti C. Allaire B. M. M. Allbrooke P. P. Allport A. Aloisio F. Alonso C. Alpigiani E. Alunno Camelia M. Alvarez Estevez M. G. Alviggi Y. Amaral Coutinho A. Ambler L. Ambroz C. Amelung D. Amidei s. P. Amor Dos santos s. Amoroso C. s. Amrouche C. Anastopoulos N. Andari t. Andeen J. K. Anders s. Y. Andrean A. Andreazza s. Angelidakis A. Angerami A. V. Anisenkov A. Annovi C. Antel M. t. Anthony E. Antipov M. Antonelli D. J. A. Antrim F. Anulli M. Aoki J. A. Aparisi Pozo M. A. Aparo L. Aperio Bella N. Aranzabal V. Araujo Ferraz C. Arcangeletti A. t. H. Arce E. Arena J-F. Arguin s. Argyropoulos J.-H. Arling A. J. Armbruster A. Armstrong O. Arnaez H. Arnold Z. P. Arrubarrena tame G. Artoni H. Asada K. Asai s. Asai N. A. Asbah E. M. Asimakopoulou L. Asquith K. Assamagan R. Astalos R. J. Atkin M. Atkinson N. B. Atlay H. Atmani P. A. Atmasiddha K. Augsten s. Auricchio V. A. Austrup G. Avner G. Avolio M. K. Ayoub G. Azuelos D. Babal H. Bachacou K. Bachas A. Bachiu F. Backman A. Badea P. Bagnaia H. Bahrasemani A. J. Bailey V. R. Bailey J. t. Baines C. Bakalis O. K. Baker P. J. Bakker E. Bakos D. Bakshi Gupta s. Balaji R. Balasubramanian E. M. Baldin P. Balek E. Ballabene F. Balli W. K. Balunas J. Balz E. Banas M. Bandieramonte A. Bandyopadhyay s. Bansal L. Barak E. L. Barberio D. Barberis M. Barbero G. Barbour K. N. Barends t. Bar CPPM Aix-Marseille Université CNRS/IN2P3 Marseille France Homer L. Dodge Department of Physics and Astronomy University of Oklahoma Norman OK United States of America Department of Physics University of Massachusetts Amherst MA United States of America CERN Geneva Switzerland II. Physikalisches Institut Georg-August-Universität Göttingen Göttingen Germany Department of Physics Royal Holloway University of London Egham United Kingdom Physics Department Brookhaven National Laboratory Upton NY United States of America Raymond and Beverly Sackler School of Physics and Astronomy Tel Aviv University Tel Aviv Israel Department of Physics Technion Israel Institute of Technology Haifa Israel High Energy Physics Division Argonne National Laboratory Argonne IL United States of America Departamento de Física Pontificia Universidad Católica de Chile Santiago Chile INFN Gruppo Collegato di Udine Sezione di Trieste Udine Italy ICTP Trieste Italy Institut für Physik Universität Mainz Mainz Germany LAPP Université Savoie Mont Blanc CNRS/IN2P3 Annecy France AGH University of Krakow Faculty of Physics and Applied Computer Science Krakow Poland Department of Physics University of Toronto Toronto ON Canada Department of Physics Brandeis University Waltham MA United States of America Department of Physics Northern Illinois University DeKalb IL United States of America Department of Physics Bogazici University Istanbul Türkiye Département de Physique Nucléaire et Corpusculaire Université de Genève Genève Switzerland Particle Physics Department Rutherford Appleton Laboratory Didcot United Kingdom Santa Cruz Institute for Particle Physics University of California Santa Cruz Santa Cruz CA United States of America IJCLab Université Paris-Saclay CNRS/IN2P3 91405 Orsay France Institut de Física d’Altes Energies (IFAE) Barcelona Institute of Science and Technology Barcelona Spain INFN Sezione di Pavia Italy Dipartimento di Fisica Università di Pavia Pavia Italy

A search for high-mass resonances decaying into a τ-lepton and a neutrino using proton-proton collisions at a center-of-mass energy of s=13 teV is presented. the full run 2 data sample corresponding to an integrated luminosity of 139 fb−1 recorded by the AtLAs experiment in the years 2015–2018 is analyzed. the τ-lepton is reconstructed in its hadronic decay modes and the total transverse momentum carried out by neutrinos is inferred from the reconstructed missing transverse momentum. the search for new physics is performed on the transverse mass between the τ-lepton and the missing transverse momentum. No excess of events above the standard Model expectation is observed and upper exclusion limits are set on the W′→τν production cross section. Heavy W′ vector bosons with masses up to 5.0 teV are excluded at 95% confidence level, assuming that they have the same couplings as the standard Model W boson. For nonuniversal couplings, W′ bosons are excluded for masses less than 3.5–5.0 teV, depending on the model parameters. in addition, model-independent limits on the visible cross section times branching ratio are determined as a function of the lower threshold on the transverse mass of the τ-lepton and missing transverse momentum.

关键词： Extensions of gauge sector Particle production Gauge bosons Hypothetical particles Neutrinos tau leptons Hadron colliders

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Gaia Data Release 3: the Galaxy in your preferred colours: synthetic photometry from Gaia low-resolution spectra

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Astronomy and Astrophysics 2023年 674卷

作者： Montegriffo, P. Bellazzini, M. De Angeli, F. Andrae, R. Barstow, M.A. Bossini, D. Bragaglia, A. Burgess, P.W. Cacciari, C. Carrasco, J.M. Chornay, N. Delchambre, L. Evans, D.W. Fouesneau, M. Frémat, Y. Garabato, D. Jordi, C. Manteiga, M. Massari, D. Palaversa, L. Pancino, E. Riello, M. Ruz Mieres, D. sanna, N. santoveña, R. sordo, R. Vallenari, A. Walton, N.A. Brown, A.G.A. Prusti, t. De Bruijne, J.H.J. Arenou, F. Babusiaux, C. Biermann, M. Creevey, O.L. Ducourant, C. Eyer, L. Guerra, R. Hutton, A. Klioner, s.A. Lammers, U.L. Lindegren, L. Luri, X. Mignard, F. Panem, C. Pourbaix, D. Randich, s. sartoretti, P. soubiran, C. tanga, P. Bailer-Jones, C.A.L. Bastian, U. Drimmel, R. Jansen, F. Katz, D. Lattanzi, M.G. Van Leeuwen, F. Bakker, J. Castañeda, J. Fabricius, C. Galluccio, L. Guerrier, A. Heiter, U. Masana, E. Messineo, R. Mowlavi, N. Nicolas, C. Nienartowicz, K. Pailler, F. Panuzzo, P. Riclet, F. Roux, W. seabroke, G.M. thévenin, F. Gracia-Abril, G. Portell, J. teyssier, D. Altmann, M. Audard, M. Bellas-Velidis, i. Benson, K. Berthier, J. Blomme, R. Busonero, D. Busso, G. Cánovas, H. Carry, B. Cellino, A. Cheek, N. Clementini, G. Damerdji, Y. Davidson, M. De teodoro, P. Nuñez Campos, M. Dell Oro, A. Esquej, P. Fernández-Hernández, J. Fraile, E. García-Lario, P. Gosset, E. Haigron, R. Halbwachs, J.-L. Hambly, N.C. Harrison, D.L. Hernández, J. Hestroffer, D. Hodgkin, s.t. Holl, B. JanãEn, K. Jevardat De Fombelle, G. Jordan, s. Krone-Martins, A. Lanzafame, A.C. Löffler, W. Marchal, O. INAF Osservatorio di Astrofisica e Scienza Dello Spazio di Bologna Via Piero Gobetti 93/3 Bologna40129 Italy Institute of Astronomy University of Cambridge Madingley Road CambridgeCB3 0HA United Kingdom Max Planck Institute for Astronomy Königstuhl 17 Heidelberg69117 Germany School of Physics and Astronomy/Space Park Leicester University of Leicester University Road LeicesterLE1 7RH United Kingdom Instituto de Astrofísica e Ciências Do Espaço Universidade Do Porto CAUP Rua das Estrelas Porto4150-762 Portugal Martí i Franquès 1 Barcelona08028 Spain Institut D Astrophysique et de Géophysique Université de Liège 19c Allée du 6 Août Liège4000 Belgium Royal Observatory of Belgium Ringlaan 3 Brussels1180 Belgium CIGUS CITIC Department of Computer Science and Information Technologies University of A Coruña Campus de Elviña s/n A Coruña15071 Spain CIGUS CITIC Department of Nautical Sciences and Marine Engineering University of A Coruña Paseo de Ronda 51 A Coruña15071 Spain Ruer Boškovic Institute Bijenička cesta 54 Zagreb10000 Croatia INAF Osservatorio Astrofisico di Arcetri Largo Enrico Fermi 5 Firenze50125 Italy Space Science Data Center ASI Via del Politecnico SNC Roma00133 Italy INAF Osservatorio Astronomico di Padova Vicolo Osservatorio 5 Padova35122 Italy Leiden Observatory Leiden University Niels Bohrweg 2 Leiden2333 CA Netherlands Keplerlaan 1 Noordwijk2201 AZ Netherlands GEPI Observatoire de Paris Université PSL CNRS 5 Place Jules Janssen Meudon92190 France Univ. Grenoble Alpes CNRS IPAG Grenoble38000 France Astronomisches Rechen-Institut Zentrum für Astronomie der Universität Heidelberg Mönchhofstr. 12-14 Heidelberg69120 Germany Université Côte D Azur Observatoire de la Côte D Azur CNRS Laboratoire Lagrange Bd de l Observatoire CS 34229 NiceCedex 4 06304 France Laboratoire D Astrophysique de Bordeaux Univ. Bordeaux CNRS B18N Allée Geoffroy Saint-Hilaire Pessac33615 France Department of Astronomy Univers

Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for '220 million sources in the wavelength range 330 nm ≤ λ ≤ 1050 nm (XP spectra). synthetic photometry directly tied to a flux in physical units can be obtained from these spectra for any passband fully enclosed in this wavelength range. We describe how synthetic photometry can be obtained from XP spectra, illustrating the performance that can be achieved under a range of different conditions - for example passband width and wavelength range - as well as the limits and the problems affecting it. Existing top-quality photometry can be reproduced within a few per cent over a wide range of magnitudes and colour, for wide and medium bands, and with up to millimag accuracy when synthetic photometry is standardised with respect to these external sources. some examples of potential scientific application are presented, including the detection of multiple populations in globular clusters, the estimation of metallicity extended to the very metal-poor regime, and the classification of white dwarfs. A catalogue providing standardised photometry for 2.2×108sources in several wide bands of widely used photometric systems is provided (Gaia synthetic Photometry Catalogue;GsPC) as well as a catalogue of '105 white dwarfs with DA/non-DA classification obtained with a Random Forest algorithm (Gaia synthetic Photometry Catalogue for White Dwarfs;GsPC-WD). © 2023 EDP sciences. All rights reserved.

关键词： White dwarfs

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A fast radio burst localized at detection to an edge-on galaxy using very-long-baseline interferometry

arXiv

引用

arXiv 2023年

作者： Cassanelli, tomas Leung, Calvin sanghavi, Pranav Mena-Parra, Juan Cary, savannah McKinven, Ryan Bhardwaj, Mohit Masui, Kiyoshi W. Michilli, Daniele Bandura, Kevin Chatterjee, shami Peterson, Jeffrey B. Kaczmarek, Jane Rahman, Mubdi shin, Kaitlyn Vanderlinde, Keith Berger, sabrina Brar, Charanjot Boyle, P.J. Breitman, Daniela Chawla, Pragya Curtin, Alice P. Dobbs, Matt Dong, Fengqiu Adam Fonseca, Emmanuel Gaensler, B.M. ibik, Adaeze Kaspi, Victoria M. Kholoud, Khairy Lanman, Adam E. Lazda, Mattias Lin, Hsiu-Hsien Luo, Jing Meyers, Bradley W. Milutinovic, Nikola Ng, Cherry Noble, Gavin Pearlman, Aaron B. Pen, Ue-Li Petroff, Emily Pleunis, Ziggy Quine, Brendan Rafiei-Ravandi, Masoud Renard, Andre sand, Ketan R. schoen, Eve scholz, Paul smith, Kendrick M. stairs, ingrid tendulkar, shriharsh P. David A. Dunlap Department of Astronomy & Astrophysics University of Toronto 50 St. George Street TorontoONM5S 3H4 Canada Dunlap Institute for Astronomy & Astrophysics University of Toronto 50 St. George Street TorontoONM5S 3H4 Canada Department of Electrical Engineering Universidad de Chile Av. Tupper 2007 Santiago8370451 Chile MIT Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology 77 Massachusetts Ave CambridgeMA02139 United States Department of Physics Massachusetts Institute of Technology 77 Massachusetts Ave CambridgeMA02139 United States Lane Department of Computer Science and Electrical Engineering West Virginia University 1220 Evansdale Drive PO Box 6109 MorgantownWV26506 United States Center for Gravitational Waves and Cosmology West Virginia University Chestnut Ridge Research Building MorgantownWV26505 United States Department of Physics Yale University New HavenCT06520 United States Department of Astronomy Wellesley College 106 Central Street WellesleyMA02481 United States Department of Physics McGill University 3600 rue University MontréalQCH3A 2T8 Canada Trottier Space Institute McGill University 3550 rue University MontréalQCH3A 2A7 Canada Cornell Center for Astrophysics and Planetary Science IthacaNY14853 United States McWilliams Center for Cosmology Department of Physics Carnegie Mellon University 5000 Forbes Ave PittsburghPA15213 United States Dominion Radio Astrophysical Observatory Herzberg Research Centre for Astronomy and Astrophysics National Research Council Canada PO Box 248 PentictonBCV2A 6J9 Canada Department of Computer Science Math Physics & Statistics University of British Columbia KelownaBCV1V 1V7 Canada CSIRO Space & Astronomy Parkes Observatory P.O. Box 276 ParkesNSW2870 Australia Sidrat Research 124 Merton Street Suite 507 TorontoONM4S 2Z2 Canada Scuola Normale Superiore PI Pisa56126 Italy Anton Pannekoek Institute for Astronomy Univers

Fast radio bursts (FRBs) are millisecond-duration radio transients whose origins remain unknown. since the vast majority of bursts are one-off events, it is necessary to pinpoint FRBs precisely within their host galaxies at the time of detection. Here, we use two purpose-built outrigger telescopes to localize FRB 20210603A at the time of its detection by the Canadian Hydrogen intensity Mapping Experiment (CHiME). Our VLBi stations localize the burst to a 0.2′′ × 2′′ final ellipse in the disk of its host galaxy sDss J004105.82+211331.9. spatially-resolved spectroscopic followup reveals recent star formation (Hα emission) on kiloparsec scales near the burst position. the excess DM is consistent with expectations from the nearly edge-on disk of the host galaxy, demonstrating the utility of FRBs as probes of the interstellar medium in distant galaxies. the excess DM, rotation measure, and scattering are consistent with expectations for a pulse traveling from deep within its host galactic plane, strengthening the link between the local environment of FRB 20210603A and the disk of its host galaxy. Finally, this technique demonstrates a way to overcome the trade-off between angular resolution and field of view in FRB instrumentation, paving the way towards plentiful and precise FRB localizations. © 2023, CC BY.

关键词： interferometry

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From FAiR to CURE: Guidelines for Computational Models of Biological systems

arXiv

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arXiv 2025年

作者： sauro, Herbert M. Agmon, Eran Blinov, Michael L. Gennari, John H. Hellerstein, Joe Heydarabadipour, Adel Hunter, Peter Jardine, Bartholomew E. May, Elebeoba Nickerson, David P. smith, Lucian P. Bader, Gary D. Bergmann, Frank Boyle, Patrick M. Dräger, Andreas Faeder, James R. Feng, song Freire, Juliana Fröhlich, Fabian Glazier, James A. Gorochowski, thomas E. Helikar, tomas Hoops, stefan imoukhuede, Princess Keating, sarah M. Konig, Matthias Laubenbacher, Reinhard Loew, Leslie M. Lopez, Carlos F. Lytton, William W. McCulloch, Andrew Mendes, Pedro Myers, Chris J. Myers, Jerry G. Mulugeta, Lealem Niarakis, Anna van Niekerk, David D. Olivier, Brett G. Patrie, Alexander A. Quardokus, Ellen M. Radde, Nicole Rohwer, Johann M. sahle, sven schaff, James C. sego, t.J. shin, Janis snoep, Jacky L. Vadigepalli, Rajanikanth Wiley, H. steve Waltemath, Dagmar Moraru, ion Department of Bioengineering University of Washington SeattleWA98195-5061 United States Intelligent Systems Engineering and Biocomplexity Institute Indiana University Street BloomingtonIN47408 United States Center for Cardiovascular Biology University of Washington SeattleWA98195-5061 United States eScience Institute University of Washington SeattleWA98195-5061 United States Institute for Stem Cell and Regenerative Medicine University of Washington SeattleWA98195-5061 United States School of Biological Sciences University of Bristol 24 Tyndall Avenue BristolBS8 1TQ United Kingdom Departments of Physiology & Pharmacology Neurology Downstate Health Science University BrooklynNY11203 United States Department of Neurology Kings County Hospital BrooklynNY11203 United States NASA-John H. Glenn Research Center MS 110-3 21000 Brookpark Road ClevelandOH44135 United States Center for Cell Analysis and Modeling UConn Health 263 Farmington Avenue FarmingtonCT06030-6406 United States Amsterdam Institute for Life and Environment Vrije Universiteit Amsterdam De Boelelaan 1108 Amsterdam1081 HZ Netherlands Department of Pathology and Genomic Medicine Thomas Jefferson University 1020 Locust St PhiladelphiaPA19107 United States Biological Sciences Division Pacific Northwest National Laboratory 902 Battelle Blvd RichlandWA99354 United States Auckland Bioengineering Institute University of Auckland Auckland1010 New Zealand Center of Integrative Biology University of Toulouse III-Paul Sabatier 165 Rue Marianne Grunberg-Manago Toulouse31400 France Lifeware Group Inria Building Alan Turing 1 Rue Honoré d’Estienne d’Orves Palaiseau91120 France Multiscale Modeling Group Altos Labs Redwood CityCA94065 United States partner site Tübingen Tübingen Germany Ottfried-Müller-Str. 37 Tübingen72076 Germany 06120 Germany Department of Computer Science Center for Data Science New York University New YorkNY11201 United States Department of Bi

Guidelines for managing scientific data have been established under the FAiR principles requiring that data be Findable, Accessible, interoperable, and Reusable. in many scientific disciplines, especially computational biology, both data and models are key to progress. For this reason, and recognizing that such models are a very special type of "data", we argue that computational models, especially mechanistic models prevalent in medicine, physiology and systems biology, deserve a complementary set of guidelines. We propose the CURE principles, emphasizing that models should be Credible, Understandable, Reproducible, and Extensible. We delve into each principle, discussing verification, validation, and uncertainty quantification for model credibility;the clarity of model descriptions and annotations for understandability;adherence to standards and open science practices for reproducibility;and the use of open standards and modular code for extensibility and reuse. We outline recommended and baseline requirements for each aspect of CURE, aiming to enhance the impact and trustworthiness of computational models, particularly in biomedical applications where credibility is paramount. Our perspective underscores the need for a more disciplined approach to modeling, aligning with emerging trends such as Digital twins and emphasizing the importance of data and modeling standards for interoperability and reuse. Finally, we emphasize that given the non-trivial effort required to implement the guidelines, the community moves to automate as many of the guidelines as possible. © 2025, CC BY.

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