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Constraints on dark photons and axionlike particles from the SuperCDMS Soudan experiment

Physical Review D 2020年第5期101卷 052008-052008页

作者： T. Aralis T. Aramaki I. J. Arnquist E. Azadbakht W. Baker S. Banik D. Barker C. Bathurst D. A. Bauer L. V. S. Bezerra R. Bhattacharyya T. Binder M. A. Bowles P. L. Brink R. Bunker B. Cabrera R. Calkins R. A. Cameron C. Cartaro D. G. Cerdeño Y.-Y. Chang J. Cooley H. Coombes J. Corbett B. Cornell P. Cushman F. De Brienne M. L. di Vacri M. D. Diamond E. Fascione E. Figueroa-Feliciano C. W. Fink K. Fouts M. Fritts G. Gerbier R. Germond M. Ghaith S. R. Golwala H. R. Harris N. Herbert B. A. Hines M. I. Hollister Z. Hong E. W. Hoppe L. Hsu M. E. Huber V. Iyer D. Jardin A. Jastram M. H. Kelsey A. Kennedy A. Kubik N. A. Kurinsky R. E. Lawrence A. Li B. Loer E. Lopez Asamar P. Lukens D. MacDonell D. B. MacFarlane R. Mahapatra V. Mandic N. Mast É. M. Michaud E. Michielin N. Mirabolfathi B. Mohanty J. D. Morales Mendoza S. Nagorny J. Nelson H. Neog J. L. Orrell S. M. Oser W. A. Page P. Pakarha R. Partridge R. Podviianiuk F. Ponce S. Poudel M. Pyle W. Rau R. Ren T. Reynolds A. Roberts A. E. Robinson H. E. Rogers T. Saab B. Sadoulet J. Sander R. W. Schnee S. Scorza K. Senapati B. Serfass D. J. Sincavage C. Stanford M. Stein J. Street D. Toback R. Underwood S. Verma A. N. Villano B. von Krosigk S. L. Watkins L. Wills J. S. Wilson M. J. Wilson J. Winchell D. H. Wright S. Yellin B. A. Young T. C. Yu E. Zhang X. Zhao L. Zheng Division of Physics Mathematics & Astronomy California Institute of Technology Pasadena California 91125 USA SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology Menlo Park California 94025 USA Pacific Northwest National Laboratory Richland Washington 99352 USA Department of Physics and Astronomy and the Mitchell Institute for Fundamental Physics and Astronomy Texas A&M University College Station Texas 77843 USA School of Physical Sciences National Institute of Science Education and Research HBNI Jatni—752050 India School of Physics & Astronomy University of Minnesota Minneapolis Minnesota 55455 USA Department of Physics University of Florida Gainesville Florida 32611 USA Fermi National Accelerator Laboratory Batavia Illinois 60510 USA Department of Physics & Astronomy University of British Columbia Vancouver British Columbia V6T 1Z1 Canada TRIUMF Vancouver British Columbia V6T 2A3 Canada Department of Physics University of South Dakota Vermillion South Dakota 57069 USA Department of Physics South Dakota School of Mines and Technology Rapid City South Dakota 57701 USA Department of Physics Stanford University Stanford California 94305 USA Department of Physics Southern Methodist University Dallas Texas 75275 USA Department of Physics Durham University Durham DH1 3LE United Kingdom Instituto de Física Teórica UAM/CSIC Universidad Autónoma de Madrid 28049 Madrid Spain Department of Physics Queen’s University Kingston Ontario K7L 3N6 Canada Département de Physique Université de Montréal Montréal Québec H3C 3J7 Canada Department of Physics University of Toronto Toronto Ontario M5S 1A7 Canada Department of Physics & Astronomy Northwestern University Evanston Illinois 60208-3112 USA Department of Physics University of California Berkeley California 94720 USA Department of Electrical and Computer Engineering Texas A&M University College Station Texas 77843 USA Department of Physics University of

We present an analysis of electron recoils in cryogenic germanium detectors operated during the SuperCDMS Soudan experiment. The data are used to set new constraints on the axioelectric coupling of axionlike particles and the kinetic mixing parameter of dark photons, assuming the respective species constitutes all of the galactic dark matter. This study covers the mass range from 40 eV/c2 to 500 keV/c2 for both candidates, excluding previously untested parameter space for masses below ∼1 keV/c2. For the kinetic mixing of dark photons, values below 10−15 are reached for particle masses around 100 eV/c2; for the axioelectric coupling of axionlike particles, values below 10−12 are reached for particles with masses in the range of a few-hundred eV/c2.

关键词： Axions Particle dark matter Dark matter detectors Solid-state detectors

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Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

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Physical Review D 2020年第9期102卷 091101(R)-091101(R)页

作者： D. W. Amaral T. Aralis T. Aramaki I. J. Arnquist E. Azadbakht S. Banik D. Barker C. Bathurst D. A. Bauer L. V. S. Bezerra R. Bhattacharyya T. Binder M. A. Bowles P. L. Brink R. Bunker B. Cabrera R. Calkins R. A. Cameron C. Cartaro D. G. Cerdeño Y.-Y. Chang R. Chen N. Chott J. Cooley H. Coombes J. Corbett P. Cushman F. De Brienne M. L. di Vacri M. D. Diamond E. Fascione E. Figueroa-Feliciano C. W. Fink K. Fouts M. Fritts G. Gerbier R. Germond M. Ghaith S. R. Golwala H. R. Harris N. Herbert B. A. Hines M. I. Hollister Z. Hong E. W. Hoppe L. Hsu M. E. Huber V. Iyer D. Jardin A. Jastram M. H. Kelsey A. Kubik N. A. Kurinsky R. E. Lawrence A. Li B. Loer E. Lopez Asamar P. Lukens D. MacDonell D. B. MacFarlane R. Mahapatra V. Mandic N. Mast A. J. Mayer É. M. Michaud E. Michielin N. Mirabolfathi B. Mohanty J. D. Morales Mendoza S. Nagorny J. Nelson H. Neog V. Novati J. L. Orrell S. M. Oser W. A. Page P. Pakarha R. Partridge R. Podviianiuk F. Ponce S. Poudel M. Pyle W. Rau E. Reid R. Ren T. Reynolds A. Roberts A. E. Robinson H. E. Rogers T. Saab B. Sadoulet J. Sander A. Sattari R. W. Schnee S. Scorza B. Serfass D. J. Sincavage C. Stanford M. Stein J. Street D. Toback R. Underwood S. Verma A. N. Villano B. von Krosigk S. L. Watkins L. Wills J. S. Wilson M. J. Wilson J. Winchell D. H. Wright S. Yellin B. A. Young T. C. Yu E. Zhang H. G. Zhang X. Zhao L. Zheng Department of Physics Durham University Durham DH1 3LE United Kingdom Division of Physics Mathematics and Astronomy California Institute of Technology Pasadena California 91125 USA SLAC National Accelerator Laboratory/Kavli Institute for Particle Astrophysics and Cosmology Menlo Park California 94025 USA Pacific Northwest National Laboratory Richland Washington 99352 USA Department of Physics and Astronomy and the Mitchell Institute for Fundamental Physics and Astronomy Texas A&M University College Station Texas 77843 USA School of Physical Sciences National Institute of Science Education and Research HBNI Jatni—752050 India School of Physics and Astronomy University of Minnesota Minneapolis Minnesota 55455 USA Department of Physics University of Florida Gainesville Florida 32611 USA Fermi National Accelerator Laboratory Batavia Illinois 60510 USA Department of Physics and Astronomy University of British Columbia Vancouver British Columbia V6T 1Z1 Canada TRIUMF Vancouver British Columbia V6T 2A3 Canada Department of Physics University of South Dakota Vermillion South Dakota 57069 USA Department of Physics South Dakota School of Mines and Technology Rapid City South Dakota 57701 USA Department of Physics Stanford University Stanford California 94305 USA Department of Physics Southern Methodist University Dallas Texas 75275 USA Instituto de Física Teórica UAM/CSIC Universidad Autónoma de Madrid 28049 Madrid Spain Department of Physics and Astronomy Northwestern University Evanston Illinois 60208-3112 USA Department of Physics Queen’s University Kingston Ontario K7L 3N6 Canada Département de Physique Université de Montréal Montréal Quebec H3C 3J7 Canada Department of Physics University of Toronto Toronto Ontario M5S 1A7 Canada Department of Physics University of California Berkeley California 94720 USA Department of Electrical and Computer Engineering Texas A&M University College Station Texas 77843 USA Department of Physics Univer

This article presents an analysis and the resulting limits on light dark matter inelastically scattering off of electrons, and on dark photon and axionlike particle absorption, using a second-generation SuperCDMS high-voltage eV-resolution detector. The 0.93 g Si detector achieved a 3 eV phonon energy resolution; for a detector bias of 100 V, this corresponds to a charge resolution of 3% of a single electron-hole pair. The energy spectrum is reported from a blind analysis with 1.2 g-days of exposure acquired in an above-ground laboratory. With charge carrier trapping and impact ionization effects incorporated into the dark matter signal models, the dark matter-electron cross section σ¯e is constrained for dark matter masses from 0.5 to 104 MeV/c2; in the mass range from 1.2 to 50 eV/c2 the dark photon kinetic mixing parameter ϵ and the axioelectric coupling constant gae are constrained. The minimum 90% confidence-level upper limits within the above-mentioned mass ranges are σ¯e=8.7×10−34 cm2, ϵ=3.3×10−14, and gae=1.0×10−9.

关键词： Dark matter Particle dark matter Semiconductors Dark matter detectors Solid-state detectors

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Search for top squarks in final states with two top quarks and several light-flavor jets in proton-proton collisions at s=13 TeV

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Physical Review D 2021年第3期104卷 032006-032006页

作者： A. M. Sirunyan A. Tumasyan W. Adam J. W. Andrejkovic T. Bergauer S. Chatterjee M. Dragicevic A. Escalante Del Valle R. Frühwirth M. Jeitler N. Krammer L. Lechner D. Liko I. Mikulec F. M. Pitters J. Schieck R. Schöfbeck M. Spanring S. Templ W. Waltenberger C.-E. Wulz V. Chekhovsky A. Litomin V. Makarenko M. R. Darwish E. A. De Wolf X. Janssen T. Kello A. Lelek H. Rejeb Sfar P. Van Mechelen S. Van Putte N. Van Remortel F. Blekman E. S. Bols J. D’Hondt J. De Clercq M. Delcourt S. Lowette S. Moortgat A. Morton D. Müller A. R. Sahasransu S. Tavernier W. Van Doninck P. Van Mulders D. Beghin B. Bilin B. Clerbaux G. De Lentdecker L. Favart A. Grebenyuk A. K. Kalsi K. Lee M. Mahdavikhorrami I. Makarenko L. Moureaux L. Pétré A. Popov N. Postiau E. Starling L. Thomas M. Vanden Bemden C. Vander Velde P. Vanlaer D. Vannerom L. Wezenbeek T. Cornelis D. Dobur M. Gruchala G. Mestdach M. Niedziela C. Roskas K. Skovpen M. Tytgat W. Verbeke B. Vermassen M. Vit A. Bethani G. Bruno F. Bury C. Caputo P. David C. Delaere I. S. Donertas A. Giammanco V. Lemaitre K. Mondal J. Prisciandaro A. Taliercio M. Teklishyn P. Vischia S. Wertz S. Wuyckens G. A. Alves C. Hensel A. Moraes W. L. Aldá Júnior M. Barroso Ferreira Filho H. Brandao Malbouisson W. Carvalho J. Chinellato E. M. Da Costa G. G. Da Silveira D. De Jesus Damiao S. Fonseca De Souza D. Matos Figueiredo C. Mora Herrera K. Mota Amarilo L. Mundim H. Nogima P. Rebello Teles L. J. Sanchez Rosas A. Santoro S. M. Silva Do Amaral A. Sznajder M. Thiel F. Torres Da Silva De Araujo A. Vilela Pereira C. A. Bernardes L. Calligaris T. R. Fernandez Perez Tomei E. M. Gregores D. S. Lemos P. G. Mercadante S. F. Novaes Sandra S. Padula A. Aleksandrov G. Antchev I. Atanasov R. Hadjiiska P. Iaydjiev M. Misheva M. Rodozov M. Shopova G. Sultanov A. Dimitrov T. Ivanov L. Litov B. Pavlov P. Petkov A. Petrov T. Cheng W. Fang Q. Guo T. Javaid M. Mittal H. Wang L. Yuan M. Ahmad G. Bauer C. Dozen Z. Hu J. Martins Y. Wang K. Yi E. Chapon G. M. Chen H. S. Chen M. Chen A. Kapoor D. Leggat H. Liao Z.-A. LIU R. Sha Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Wien Austria Institute for Nuclear Problems Minsk Belarus Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Korea University Seoul Korea 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 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 Rutgers The State University of New Jersey Piscataway New Jersey USA Department of Physics Tsinghua University Beijing China Institute of High Energy Physics Beijing China Massachusetts Institute of Technology Cambridge Massachusetts USA State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China The University of Kansas Lawrence Kansas USA Sun Yat-Sen University Guangzhou China Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE)—Fudan University Shanghai China Zhejiang University 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) Fa

Many new physics models, including versions of supersymmetry characterized by R-parity violation (RPV), compressed mass spectra, long decay chains, or additional hidden sectors, predict the production of events with top quarks, low missing transverse momentum, and many additional quarks or gluons. The results of a search for new physics in events with two top quarks and additional jets are reported. The search is performed using events with at least seven jets and exactly one electron or muon. No requirement on missing transverse momentum is imposed. The study is based on a sample of proton-proton collisions at s=13TeV corresponding to 137 fb−1 of integrated luminosity collected with the CMS detector at the LHC in 2016–2018. The data are used to determine best fit values and upper limits on the cross section for pair production of top squarks in scenarios of RPV and stealth supersymmetry. Top squark masses up to 670 (870) GeV are excluded at 95% confidence level for the RPV (stealth) scenario, and the maximum observed local signal significance is 2.8 standard deviations for the RPV scenario with top squark mass of 400 GeV.

关键词： Supersymmetry Hadron colliders

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High-dimensional dependency structure learning for physical processes

arXiv

引用

arXiv 2017年

作者： Golmohammadi, Jamal Ebert-Uphoff, Imme He, Sijie Deng, Yi Banerjee, Arindam Department of Computer Science & Engineering University of Minnesota Twin-cities United States Department of Electrical and Computer Engineering Colorado State University School of Earth and Atmospheric Sciences Georgia Institute of Technology

In this paper, we consider the use of structure learning methods for probabilistic graphical models to identify statistical dependencies in high-dimensional physical processes. Such processes are often synthetically characterized using PDEs (partial differential equations) and are observed in a variety of natural phenomena, including geoscience data capturing atmospheric and hydrological phenomena. Classical structure learning approaches such as the PC algorithm and variants are challenging to apply due to their high computational and sample requirements. Modern approaches, often based on sparse regression and variants, do come with finite sample guarantees, but are usually highly sensitive to the choice of hyper-parameters, e.g., parameter λ for sparsity inducing constraint or regularization. In this paper, we present ACLIME-ADMM, an efficient two-step algorithm for adaptive structure learning, which estimates an edge specific parameter λij in the first step, and uses these parameters to learn the structure in the second step. Both steps of our algorithm use (inexact) ADMM to solve suitable linear programs, and all iterations can be done in closed form in an efficient block parallel manner. We compare ACLIME-ADMM with baselines on both synthetic data simulated by partial differential equations (PDEs) that model advection-diffusion processes, and real data (50 years) of daily global geopotential heights to study information flow in the atmosphere. ACLIME-ADMM is shown to be efficient, stable, and competitive, usually better than the baselines especially on difficult problems. On real data, ACLIME-ADMM recovers the underlying structure of global atmospheric circulation, including switches in wind directions at the equator and tropics entirely from the data. Copyright © 2017, The Authors. All rights reserved.

关键词： Linear programming

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A Deep Neural Network for Simultaneous Estimation of b Jet Energy and Resolution

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Computing and Software for Big Science 2020年第1期4卷 1-20页

作者： Sirunyan, A.M. Tumasyan, A. Adam, W. Ambrogi, F. Bergauer, T. Dragicevic, M. Erö, J. Valle, A. Escalante Del 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. Gonzalez, J. Suarez Darwish, M.R. De Wolf, E.A. Croce, D. Di Janssen, X. Lelek, A. Pieters, M. Sfar, H. Rejeb Haevermaet, H. Van Mechelen, P. Van Putte, S. Van Remortel, N. Van Blekman, F. Bols, E.S. Chhibra, S.S. D’Hondt, J. De Clercq, J. Lontkovskyi, D. Lowette, S. Marchesini, I. Moortgat, S. Python, Q. Skovpen, K. Tavernier, S. Doninck, W. Van Mulders, P. Van Beghin, D. Bilin, B. Clerbaux, B. De Lentdecker, G. Delannoy, H. Dorney, B. Favart, L. Grebenyuk, A. Kalsi, A.K. Popov, A. Postiau, N. Starling, E. Thomas, L. Velde, C. Vander Vanlaer, P. Vannerom, D. Cornelis, T. Dobur, D. Khvastunov, I. Niedziela, M. Roskas, C. Tytgat, M. Verbeke, W. Vermassen, B. Vit, M. Bondu, O. Bruno, G. Caputo, C. David, P. Delaere, C. Delcourt, M. Giammanco, A. Lemaitre, V. Prisciandaro, J. Saggio, A. Marono, M. Vidal Vischia, P. Zobec, J. Alves, F.L. Alves, G.A. Silva, G. Correia Hensel, C. Moraes, A. Teles, P. Rebello Chagas, E. Belchior Batista Das Carvalho, W. Chinellato, J. Coelho, E. Da Costa, E.M. Da Silveira, G.G. De Jesus Damiao, D. De Oliveira Martins, C. De Souza, S. Fonseca Guativa, L. M. Huertas Malbouisson, H. Martins, J. Figueiredo, D. Matos Jaime, M. Medina De Almeida, M. Melo Herrera, C. Mora Mundim, L. Nogima, H. Da Silva, W. L. Prado Rosas, L. J. Sanchez Santoro, A. Sznajder, A. Thiel, M. Manganote, E. J. Tonelli Da Silva De Araujo, F. Torres Pereira, A. Vilela Bernardes, C.A. Calligaris, L. Tomei, T. R. Fernandez Perez Gregores, E.M. Lemos, D.S. Mercadante, P.G. Novaes, S.F. Padula, SandraS. Aleksandrov, A. Antchev, G. Hadjiiska, R. Iaydjiev, P. Misheva, M. Rodozov, M. Shopova, M. Sultanov, G. Bonchev, M. Dimitrov, A. Ivanov, T. Litov, L. Pavlov, B. Petkov, P. Fang, W. Gao, X. Yuan, Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Wien 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 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 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 Zhejiang University 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 National Institute of Chemical Physics and Biophysics Tallinn Estonia Department of Physics University of Helsinki Helsinki Finland Helsinki Institute of Physics Helsinki Finland Lappeenranta University of Technology Lappeenranta Finland IRFU CEA Université Paris-Saclay Gif-sur-Yvette France Laboratoire Leprince-Ringuet CNRS/IN2P3 Ecole Polytechnique Institut Polytechnique de Paris Palaiseau France Université de Strasbourg CNRS IPH

We describe a method to obtain point and dispersion estimates for the energies of jets arising from b quarks produced in proton–proton collisions at an energy of s=13TeV at the CERN LHC. The algorithm is trained on a large sample of simulated b jets and validated on data recorded by the CMS detector in 2017 corresponding to an integrated luminosity of 41 fb-1. A multivariate regression algorithm based on a deep feed-forward neural network employs jet composition and shape information, and the properties of reconstructed secondary vertices associated with the jet. The results of the algorithm are used to improve the sensitivity of analyses that make use of b jets in the final state, such as the observation of Higgs boson decay to b b ¯. © 2020, The Author(s).

关键词： b jets CMS Deep learning Higgs boson Jet energy Jet resolution

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The meerKAT galaxy cluster legacy survey I. survey overview and highlights

arXiv

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arXiv 2021年

作者： Knowles, Kenda Cotton, W.D. Rudnick, L. Camilo, F. Goedhart, S. Deane, R. Ramatsoku, M. Bietenholz, M.F. Brüggen, M. Button, C. Chen, H. Chibueze, J.O. Clarke, T.E. de Gasperin, F. Ianjamasimanana, R. Józsa, G.I.G. Hilton, M. Kesebonye, K.C. Kolokythas, K. Kraan-Korteweg, R.C. Lawrie, G. Lochner, M. Loubser, S.I. Marchegiani, P. Mhlahlo, N. Moodley, K. Murphy, E. Namumba, B. Oozeer, N. Parekh, V. Pillay, D.S. Passmoor, S.S. Ramaila, A.J.T. Ranchod, S. Retana-Montenegro, E. Sebokolodi, L. Sikhosana, S.P. Smirnov, O. Thorat, K. Venturi, T. Abbott, T.D. Adam, R.M. Adams, G. Aldera, M.A. Bauermeister, E.F. Bennett, T.G.H. Bode, W.A. Botha, D.H. Botha, A.G. Brederode, L.R.S. Buchner, S. Burger, J.P. Cheetham, T. de Villiers, D.I.L. Dikgale-Mahlakoana, M.A. du Toit, L.J. Esterhuyse, S.W.P. Fadana, G. Fanaroff, B.L. Fataar, S. Foley, A.R. Fourie, D.J. Frank, B.S. Gamatham, R.R.G. Gatsi, T.G. Geyer, M. Gouws, M. Gumede, S.C. Heywood, I. Hlakola, M.J. Hokwana, A. Hoosen, S.W. Horn, D.M. Horrell, J.M.G. Hugo, B.V. Isaacson, A.R. Jonas, J.L. Jordaan, J.D.B. Joubert, A.F. Julie, R.P.M. Kapp, F.B. Kasper, V.A. Kenyon, J.S. Kotzé, P.P.A. Kotze, A.G. Kriek, N. Kriel, H. Krishnan, V.K. Kusel, T.W. Legodi, L.S. Lehmensiek, R. Liebenberg, D. Lord, R.T. Lunsky, B.M. Madisa, K. Magnus, L.G. Main, J.P.L. Makhaba, A. Makhathini, S. Malan, J.A. Manley, J.R. Marais, S.J. Maree, M.D.J. Martens, A. Mauch, T. McAlpine, K. Merry, B.C. Millenaar, R.P. Mokone, O.J. Monama, T.E. Mphego, M.C. New, W.S. Ngcebetsha, B. Ngoasheng, K.J. Ockards, M.T. Otto, A.J. Patel, A.A. Peens-Hough, A. Perkins, S.J. Ramanujam, N.M. Ramudzuli, Z.R. Ratcliffe, S.M. Renil, R. Robyntjies, A. Rust, A.N. Salie, S. Sambu, N. Schollar, C.T.G. Schwardt, L.C. Schwartz, R.L. Serylak, M. Siebrits, R. Sirothia, S.K. Slabber, M. Sofeya, L. Taljaard, B. Tasse, C. Tiplady, A.J. Toruvanda, O. Twum, S.N. van Balla, T.J. van der Byl, A. van der Merwe, C. van Dyk, C.L. van Tonder, V. van Wyk, R. Venter, A.J. Venter, M. Welz, M.G. Williams, L.P. Xaia, B. Astrophysics Research Centre University of KwaZulu-Natal Durban4041 South Africa Centre for Radio Astronomy Techniques and Technologies Department of Physics and Electronics Rhodes University P.O. Box 94 Makhanda6140 South Africa South African Radio Astronomy Observatory 2 Fir Street Observatory7925 South Africa National Radio Astronomy Observatory CharlottesvilleVA22903 United States Minnesota Institute for Astrophysics University of Minnesota 116 Church St SE MinneapolisMN55455 United States Wits Centre for Astrophysics School of Physics University of the Witwatersrand 1 Jan Smuts Avenue Johannesburg2050 South Africa Department of Physics University of Pretoria Hatfield0028 South Africa I-09047 Italy Hartebeesthoek Radio Astronomy Observatory SARAO Krugersdorp1740 South Africa York University TorontoON Canada Hamburger Sternwarte Universität Hamburg Gojenbergsweg 112 Hamburg21029 Germany Department of Astronomy University of Cape Town Rondebosch7700 South Africa Centre for Space Research North-West University Potchefstroom2520 South Africa Department of Physics and Astronomy Faculty of Physical Sciences University of Nigeria Carver Building 1 University Road Nsukka Nigeria Naval Research Laboratory WashingtonDC20375 United States INAF – Istituto di Radioastronomia via Gobetti 101 BolognaI–40129 Italy Argelander-Institut für Astronomie Universität Bonn Auf dem Hügel 71 BonnD-53121 Germany School of Mathematics Statistics and Computer Science University of KwaZulu-Natal Westville 3696 South Africa Department of Physics and Astronomy University of the Western Cape Bellville7535 South Africa Dipartimento di Fisica Universitá Sapienza P.le Aldo Moro 2 Roma00185 Italy African Institute for Mathematical Sciences 6-8 Melrose Road Muizenberg7945 South Africa Inter-University Institute for Data Intensive Astronomy University of Cape Town Rondebosch7700 South Africa Ltd. 64-74 White Road Retreat 7945 South Africa EMSS Ant

MeerKAT’s large number (64) of 13.5 m-diameter antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of angular scales. The MeerKAT Galaxy Cluster Legacy Survey (MGCLS) is a programme of long-track MeerKAT L-band (900–1670 MHz) observations of 115 galaxy clusters, observed for ∼ 6–10 hours each in full polarisation. The first legacy product data release (DR1), made available with this paper, includes the MeerKAT visibilities, basic image cubes at ∼ 800 resolution, and enhanced spectral and polarisation image cubes at ∼ 800 and 1500 resolutions. Typical sensitivities for the full-resolution MGCLS image products range over ∼ 3–5 µJy beam−1. The basic cubes are full-field and span 2◦ × 2◦. The enhanced products consist of the inner 1.2◦ × 1.2◦ field of view, corrected for the primary beam. The survey is fully sensitive to structures up to ∼ 100 scales and the wide bandwidth allows spectral and Faraday rotation mapping. Relatively narrow frequency channels (209 kHz) are also used to provide H i mapping in windows of 0 200. We find no dependence of the star formation rate on distance from the cluster centre, and observe a small excess of the radio-to-100 µm flux ratio towards the centre of Abell 209 that may reflect a ram pressure enhancement in the denser environment. We detect diffuse cluster radio emission in 62 of the surveyed systems and present a catalogue of the 99 diffuse cluster emission structures, of which 56 are new. These include mini-halos, halos, relics, and other diffuse structures for which no suitable characterization currently exists. We highlight some of the radio galaxies which challenge current paradigms such as trident-shaped structures, jets that remain well-collimated far beyond their bending radius, and filamentary features linked to radio galaxies that likely illuminate magnetic flux tubes in the intracluster medium. We also present early results from

关键词： Surveys

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Measurement of the electroweak production of Zγ and two jets in proton-proton collisions at s=13 TeV and constraints on anomalous quartic gauge couplings

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Physical Review D 2021年第7期104卷 072001-072001页

作者： A. Tumasyan W. Adam J. W. Andrejkovic T. Bergauer S. Chatterjee M. Dragicevic A. Escalante Del Valle R. Frühwirth M. Jeitler N. Krammer L. Lechner D. Liko I. Mikulec P. Paulitsch F. M. Pitters J. Schieck R. Schöfbeck M. Spanring S. Templ W. Waltenberger C.-E. Wulz V. Chekhovsky A. Litomin V. Makarenko M. R. Darwish E. A. De Wolf T. Janssen T. Kello A. Lelek H. Rejeb Sfar P. Van Mechelen S. Van Putte N. Van Remortel F. Blekman E. S. Bols J. D’Hondt M. Delcourt H. El Faham S. Lowette S. Moortgat A. Morton D. Müller A. R. Sahasransu S. Tavernier W. Van Doninck P. Van Mulders D. Beghin B. Bilin B. Clerbaux G. De Lentdecker L. Favart A. Grebenyuk A. K. Kalsi K. Lee M. Mahdavikhorrami I. Makarenko L. Moureaux L. Pétré A. Popov N. Postiau E. Starling L. Thomas M. Vanden Bemden C. Vander Velde P. Vanlaer D. Vannerom L. Wezenbeek T. Cornelis D. Dobur J. Knolle L. Lambrecht G. Mestdach M. Niedziela C. Roskas A. Samalan K. Skovpen M. Tytgat W. Verbeke B. Vermassen M. Vit A. Bethani G. Bruno F. Bury C. Caputo P. David C. Delaere I. S. Donertas A. Giammanco K. Jaffel Sa. Jain V. Lemaitre K. Mondal J. Prisciandaro A. Taliercio M. Teklishyn T. T. Tran P. Vischia S. Wertz G. A. Alves C. Hensel A. Moraes W. L. Aldá Júnior M. Alves Gallo Pereira M. Barroso Ferreira Filho H. Brandao Malbouisson W. Carvalho J. Chinellato E. M. Da Costa G. G. Da Silveira D. De Jesus Damiao S. Fonseca De Souza D. Matos Figueiredo C. Mora Herrera K. Mota Amarilo L. Mundim H. Nogima P. Rebello Teles A. Santoro S. M. Silva Do Amaral A. Sznajder M. Thiel F. Torres Da Silva De Araujo A. Vilela Pereira C. A. Bernardes L. Calligaris T. R. Fernandez Perez Tomei E. M. Gregores D. S. Lemos P. G. Mercadante S. F. Novaes Sandra S. Padula A. Aleksandrov G. Antchev R. Hadjiiska P. Iaydjiev M. Misheva M. Rodozov M. Shopova G. Sultanov A. Dimitrov T. Ivanov L. Litov B. Pavlov P. Petkov A. Petrov T. Cheng Q. Guo T. Javaid M. Mittal H. Wang L. Yuan M. Ahmad G. Bauer C. Dozen Z. Hu J. Martins Y. Wang K. Yi E. Chapon G. M. Chen H. S. Chen M. Chen F. Iemmi A. Kapoor D. Le Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Wien Austria Institute for Nuclear Problems Minsk Belarus Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Korea University Seoul Korea 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 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 Rutgers The State University of New Jersey Piscataway New Jersey USA Department of Physics Tsinghua University Beijing China Institute of High Energy Physics Beijing China Massachusetts Institute of Technology Cambridge Massachusetts USA State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China The University of Kansas Lawrence Kansas USA Sun Yat-Sen University Guangzhou China Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE)—Fudan University Shanghai China Zhejiang University 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) Fa

The first observation of the electroweak (EW) production of a Z boson, a photon, and two forward jets (Zγjj) in proton-proton collisions at a center-of-mass energy of 13 TeV is presented. A data set corresponding to an integrated luminosity of 137 fb−1, collected by the CMS experiment at the LHC in 2016–2018 is used. The measured fiducial cross section for EW Zγjj is σEW=5.21±0.52(stat)±0.56(syst) fb=5.21±0.76 fb. Single-differential cross sections in photon, leading lepton, and leading jet transverse momenta, and double-differential cross sections in mjj and |Δηjj| are also measured. Exclusion limits on anomalous quartic gauge couplings are derived at 95% confidence level in terms of the effective field theory operators M0 to M5, M7, T0 to T2, and T5 to T9.

关键词： Photons W & Z bosons Hadron colliders

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Measurement of differential tt¯ production cross sections in the full kinematic range using lepton+jets events from proton-proton collisions at s=13 TeV

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Physical Review D 2021年第9期104卷 092013-092013页

作者： A. Tumasyan W. Adam J. W. Andrejkovic T. Bergauer S. Chatterjee M. Dragicevic A. Escalante Del Valle R. Frühwirth M. Jeitler N. Krammer L. Lechner D. Liko I. Mikulec P. Paulitsch F. M. Pitters J. Schieck R. Schöfbeck M. Spanring S. Templ W. Waltenberger C.-E. Wulz V. Chekhovsky A. Litomin V. Makarenko M. R. Darwish E. A. De Wolf T. Janssen T. Kello A. Lelek H. Rejeb Sfar P. Van Mechelen S. Van Putte N. Van Remortel F. Blekman E. S. Bols J. D’Hondt M. Delcourt H. El Faham S. Lowette S. Moortgat A. Morton D. Müller A. R. Sahasransu S. Tavernier W. Van Doninck P. Van Mulders D. Beghin B. Bilin B. Clerbaux G. De Lentdecker L. Favart A. Grebenyuk A. K. Kalsi K. Lee M. Mahdavikhorrami I. Makarenko L. Moureaux L. Pétré A. Popov N. Postiau E. Starling L. Thomas M. Vanden Bemden C. Vander Velde P. Vanlaer D. Vannerom L. Wezenbeek T. Cornelis D. Dobur J. Knolle L. Lambrecht G. Mestdach M. Niedziela C. Roskas A. Samalan K. Skovpen M. Tytgat B. Vermassen M. Vit A. Bethani G. Bruno F. Bury C. Caputo P. David C. Delaere I. S. Donertas A. Giammanco K. Jaffel Sa. Jain V. Lemaitre K. Mondal J. Prisciandaro A. Taliercio M. Teklishyn T. T. Tran P. Vischia S. Wertz G. A. Alves C. Hensel A. Moraes W. L. Aldá Júnior M. Alves Gallo Pereira M. Barroso Ferreira Filho H. Brandao Malbouisson W. Carvalho J. Chinellato E. M. Da Costa G. G. Da Silveira D. De Jesus Damiao S. Fonseca De Souza D. Matos Figueiredo C. Mora Herrera K. Mota Amarilo L. Mundim H. Nogima P. Rebello Teles A. Santoro S. M. Silva Do Amaral A. Sznajder M. Thiel F. Torres Da Silva De Araujo A. Vilela Pereira C. A. Bernardes L. Calligaris T. R. Fernandez Perez Tomei E. M. Gregores D. S. Lemos P. G. Mercadante S. F. Novaes Sandra S. Padula A. Aleksandrov G. Antchev R. Hadjiiska P. Iaydjiev M. Misheva M. Rodozov M. Shopova G. Sultanov A. Dimitrov T. Ivanov L. Litov B. Pavlov P. Petkov A. Petrov T. Cheng Q. Guo T. Javaid M. Mittal H. Wang L. Yuan M. Ahmad G. Bauer C. Dozen Z. Hu J. Martins Y. Wang K. Yi E. Chapon G. M. Chen H. S. Chen M. Chen F. Iemmi A. Kapoor D. Leggat H. Lia Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Vienna Austria Institute for Nuclear Problems Minsk Belarus Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Korea University Seoul Korea 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 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 Rutgers The State University of New Jersey Piscataway New Jersey USA Department of Physics Tsinghua University Institute of High Energy Physics Beijing China Massachusetts Institute of Technology Cambridge Massachusetts USA State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China The University of Kansas Lawrence Kansas USA Sun Yat-Sen University Guangzhou China Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE)—Fudan University Shanghai China Zhejiang University 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 Universit

Measurements of differential and double-differential cross sections of top-quark pair (tt¯) production are presented in the lepton+jets channels with a single electron or muon and jets in the final state. The analysis combines for the first time signatures of top quarks with low transverse momentum pT, where the top-quark decay products can be identified as separated jets and isolated leptons, and with high pT, where the decay products are collimated and overlap. The measurements are based on proton-proton collision data at s=13 TeV collected by the CMS experiment at the LHC, corresponding to an integrated luminosity of 137 fb−1. The cross sections are presented at the parton and particle levels, where the latter minimizes extrapolations based on theoretical assumptions. Most of the measured differential cross sections are well described by standard model predictions with the exception of some double-differential distributions. The inclusive tt¯ production cross section is measured to be σtt¯=791±25 pb, which constitutes the most precise measurement in the lepton+jets channel to date.

关键词： Particle production Top quark Hadron colliders

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Strong-Field Gravity Tests with the Double Pulsar

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Physical Review X 2021年第4期11卷 041050-041050页

作者： M. Kramer I. H. Stairs R. N. Manchester N. Wex A. T. Deller W. A. Coles M. Ali M. Burgay F. Camilo I. Cognard T. Damour G. Desvignes R. D. Ferdman P. C. C. Freire S. Grondin L. Guillemot G. B. Hobbs G. Janssen R. Karuppusamy D. R. Lorimer A. G. Lyne J. W. McKee M. McLaughlin L. E. Münch B. B. P. Perera N. Pol A. Possenti J. Sarkissian B. W. Stappers G. Theureau Max-Planck-Institut für Radioastronomie Auf dem Hügel 69 D-53121 Bonn Germany Jodrell Bank Centre for Astrophysics The University of Manchester Oxford M13 9PL United Kingdom Department of Physics and Astronomy University of British Columbia 6224 Agricultural Road Vancouver British Columbia V6T 1Z1 Canada Australia Telescope National Facility CSIRO Space and Astronomy P.O. Box 76 Epping New South Wales 1710 Australia Centre for Astrophysics and Supercomputing Swinburne University of Technology P.O. Box 218 Hawthorn Victoria 3122 Australia ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav) P.O. Box 218 Hawthorn Victoria 3122 Australia Electrical and Computer Engineering University of California at San Diego La Jolla California 92093 USA Perimeter Institute for Theoretical Physics 31 Caroline Street North Waterloo Ontario Canada N2L 2Y5 INAF-Osservatorio Astronomico di Cagliari Via della Scienza 5 09047 Selargius (CA) Italy South African Radio Astronomy Observatory 2 Fir Street Black River Park Observatory 7925 South Africa Laboratoire de Physique et Chimie de l’Environnement et de l’Espace LPC2E CNRS-Université d’Orléans F-45071 Orléans France Station de Radioastronomie de Nançay Observatoire de Paris CNRS/INSU F-18330 Nançay France Institut des Hautes Études Scientifiques 91440 Bures-sur-Yvette France LESIA Observatoire de Paris Universit PSL CNRS Sorbonne Université Universit de Paris 5 Place Jules Janssen 92195 Meudon France Faculty of Science University of East Anglia Norwich NR4 7TJ United Kingdom David A. Dunlap Department of Astronomy and Astrophysics University of Toronto 50 St. George Street Toronto Ontario M5S 3H4 Canada ASTRON Netherlands Institute for Radio Astronomy Oude Hoogeveensedijk 4 7991 PD Dwingeloo Netherlands Department of Astrophysics/IMAPP Radboud University P.O. Box 9010 6500 GL Nijmegen Netherlands Department of Physics and Astronomy West Virginia University P.O. Box 6315 Morgantown West Virginia

Continued timing observations of the double pulsar PSR J0737–3039A/B, which consists of two active radio pulsars (A and B) that orbit each other with a period of 2.45 h in a mildly eccentric (e=0.088) binary system, have led to large improvements in the measurement of relativistic effects in this system. With a 16-yr data span, the results enable precision tests of theories of gravity for strongly self-gravitating bodies and also reveal new relativistic effects that have been expected but are now observed for the first time. These include effects of light propagation in strong gravitational fields which are currently not testable by any other method. In particular, we observe the effects of retardation and aberrational light bending that allow determination of the spin direction of the pulsar. In total, we detect seven post-Keplerian parameters in this system, more than for any other known binary pulsar. For some of these effects, the measurement precision is now so high that for the first time we have to take higher-order contributions into account. These include the contribution of the A pulsar’s effective mass loss (due to spin-down) to the observed orbital period decay, a relativistic deformation of the orbit, and the effects of the equation of state of superdense matter on the observed post-Keplerian parameters via relativistic spin-orbit coupling. We discuss the implications of our findings, including those for the moment of inertia of neutron stars, and present the currently most precise test of general relativity’s quadrupolar description of gravitational waves, validating the prediction of general relativity at a level of 1.3×10−4 with 95% confidence. We demonstrate the utility of the double pulsar for tests of alternative theories of gravity by focusing on two specific examples and also discuss some implications of the observations for studies of the interstellar medium and models for the formation of the double pulsar system. Finally, we provide context t

关键词： Alternative gravity theories Electromagnetic radiation astronomy Experimental studies of gravity General relativity Gravitation Gravitational wave detection Gravitational wave sources Gravitational waves Radio, microwave, & sub-mm astronomy Binary stars Interstellar medium Neutron stars & pulsars

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Search for long-lived particles decaying to jets with displaced vertices in proton-proton collisions at s=13 TeV

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Physical Review D 2021年第5期104卷 052011-052011页

作者： A. M. Sirunyan A. Tumasyan W. Adam T. Bergauer M. Dragicevic A. Escalante Del Valle R. Frühwirth M. Jeitler N. Krammer L. Lechner D. Liko I. Mikulec F. M. Pitters J. Schieck R. Schöfbeck M. Spanring S. Templ W. Waltenberger C.-E. Wulz M. Zarucki V. Chekhovsky A. Litomin V. Makarenko M. R. Darwish E. A. De Wolf X. Janssen T. Kello A. Lelek H. Rejeb Sfar P. Van Mechelen S. Van Putte N. Van Remortel F. Blekman E. S. Bols J. D’Hondt J. De Clercq S. Lowette S. Moortgat A. Morton D. Müller A. R. Sahasransu S. Tavernier W. Van Doninck P. Van Mulders D. Beghin B. Bilin B. Clerbaux G. De Lentdecker B. Dorney L. Favart A. Grebenyuk A. K. Kalsi K. Lee I. Makarenko L. Moureaux L. Pétré A. Popov N. Postiau E. Starling L. Thomas C. Vander Velde P. Vanlaer D. Vannerom L. Wezenbeek T. Cornelis D. Dobur M. Gruchala I. Khvastunov G. Mestdach M. Niedziela C. Roskas K. Skovpen M. Tytgat W. Verbeke B. Vermassen M. Vit A. Bethani G. Bruno F. Bury C. Caputo P. David C. Delaere M. Delcourt I. S. Donertas A. Giammanco V. Lemaitre K. Mondal J. Prisciandaro A. Taliercio M. Teklishyn P. Vischia S. Wertz S. Wuyckens G. A. Alves C. Hensel A. Moraes W. L. Aldá Júnior E. Belchior Batista Das Chagas H. Brandao Malbouisson W. Carvalho J. Chinellato E. Coelho E. M. Da Costa G. G. Da Silveira D. De Jesus Damiao S. Fonseca De Souza J. Martins D. Matos Figueiredo C. Mora Herrera L. Mundim H. Nogima P. Rebello Teles L. J. Sanchez Rosas A. Santoro S. M. Silva Do Amaral A. Sznajder M. Thiel F. Torres Da Silva De Araujo A. Vilela Pereira C. A. Bernardes L. Calligaris T. R. Fernandez Perez Tomei E. M. Gregores D. S. Lemos P. G. Mercadante S. F. Novaes Sandra S. Padula A. Aleksandrov G. Antchev I. Atanasov R. Hadjiiska P. Iaydjiev M. Misheva M. Rodozov M. Shopova G. Sultanov A. Dimitrov T. Ivanov L. Litov B. Pavlov P. Petkov A. Petrov T. Cheng W. Fang Q. Guo M. Mittal H. Wang L. Yuan M. Ahmad G. Bauer Z. Hu Y. Wang K. Yi E. Chapon G. M. Chen H. S. Chen M. Chen T. Javaid A. Kapoor D. Leggat H. Liao Z.-A. Liu R. Sharma A. Spiezia J. Tao J. Thomas-Wilsker J. Yerevan Physics Institute Yerevan Armenia Institut für Hochenergiephysik Wien Austria Institute for Nuclear Problems Minsk Belarus Universiteit Antwerpen Antwerpen Belgium Vrije Universiteit Brussel Brussel Belgium Université Libre de Bruxelles Bruxelles Belgium Korea University Seoul Korea 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 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 Rutgers The State University of New Jersey Piscataway New Jersey USA Department of Physics Tsinghua University Beijing China Institute of High Energy Physics Beijing China Massachusetts Institute of Technology Cambridge Massachusetts USA State Key Laboratory of Nuclear Physics and Technology Peking University Beijing China The University of Kansas Lawrence Kansas USA Sun Yat-Sen University Guangzhou China Institute of Modern Physics and Key Laboratory of Nuclear Physics and Ion-beam Application (MOE)—Fudan University Shanghai China Zhejiang University 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) Fa

A search is presented for long-lived particles produced in pairs in proton-proton collisions at the LHC operating at a center-of-mass energy of 13 TeV. The data were collected with the CMS detector during the period from 2015 through 2018, and correspond to a total integrated luminosity of 140 fb−1. This search targets pairs of long-lived particles with mean proper decay lengths between 0.1 and 100 mm, each of which decays into at least two quarks that hadronize to jets, resulting in a final state with two displaced vertices. No significant excess of events with two displaced vertices is observed. In the context of R-parity violating supersymmetry models, the pair production of long-lived neutralinos, gluinos, and top squarks is excluded at 95% confidence level for cross sections larger than 0.08 fb, masses between 800 and 3000 GeV, and mean proper decay lengths between 1 and 25 mm.

关键词： Hypothetical particle physics models Supersymmetric models Hadron colliders

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