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Measurement of the Positive Muon Anomalous Magnetic Moment to 0.20 ppm

D. P. Aguillard33, T. Albahri30, D. Allspach7, A. Anisenkov4,a, K. Badgley7, S. Baeßler35,b, I. Bailey17,c, L. Bailey27, V. A. Baranov15,d et al. (The Muon g−2 Collaboration)

V. A. Baranov15,d, E. Barlas-Yucel28, T. Barrett6, E. Barzi7, F. Bedeschi10, M. Berz18, M. Bhattacharya7, H. P. Binney36, P. Bloom19, J. Bono7, E. Bottalico30, T. Bowcock30, S. Braun36, M. Bressler32, G. Cantatore12,e, R. M. Carey2, B. C. K. Casey7, D. Cauz26,f, R. Chakraborty29, A. Chapelain6, S. Chappa7, S. Charity30, C. Chen23,22, M. Cheng28, R. Chislett27, Z. Chu22,g, T. E. Chupp33, C. Claessens36, M. E. Convery7, S. Corrodi1, L. Cotrozzi10,h, J. D. Crnkovic7, S. Dabagov8,i, P. T. Debevec28, S. Di Falco10, G. Di Sciascio11, B. Drendel7, A. Driutti10,h, V. N. Duginov15,d, M. Eads20, A. Edmonds2, J. Esquivel7, M. Farooq33, R. Fatemi29, C. Ferrari10,j, M. Fertl14, A. T. Fienberg36, A. Fioretti10,j, D. Flay32, S. B. Foster2, H. Friedsam7, N. S. Froemming20, C. Gabbanini10,j, I. Gaines7, M. D. Galati10,h, S. Ganguly7, A. Garcia36, J. George32,k, L. K. Gibbons6, A. Gioiosa25,l, K. L. Giovanetti13, P. Girotti10, W. Gohn29, L. Goodenough7, T. Gorringe29, J. Grange33, S. Grant1,27, F. Gray21, S. Haciomeroglu5,m, T. Halewood-Leagas30, D. Hampai8, F. Han29, J. Hempstead36, D. W. Hertzog36, G. Hesketh27, E. Hess10, A. Hibbert30, Z. Hodge36, K. W. Hong35, R. Hong29,1, T. Hu23,22, Y. Hu22,g, M. Iacovacci9,n, M. Incagli10, P. Kammel36, M. Kargiantoulakis7, M. Karuza12,o, J. Kaspar36, D. Kawall32, L. Kelton29, A. Keshavarzi31, D. S. Kessler32, K. S. Khaw23,22, Z. Khechadoorian6, N. V. Khomutov15, B. Kiburg7, M. Kiburg7,19, O. Kim34, N. Kinnaird2, E. Kraegeloh33, V. A. Krylov15, N. A. Kuchinskiy15, K. R. Labe6, J. LaBounty36, M. Lancaster31, S. Lee5, B. Li22,1,p, D. Li22,q, L. Li22,g, I. Logashenko4,a, A. Lorente Campos29, Z. Lu22,g, A. Lucà7, G. Lukicov27, A. Lusiani10,r, A. L. Lyon7, B. MacCoy36, R. Madrak7, K. Makino18, S. Mastroianni9, J. P. Miller2, S. Miozzi11, B. Mitra34, J. P. Morgan7, W. M. Morse3, J. Mott7,2, A. Nath9,n, J. K. Ng23,22, H. Nguyen7, Y. Oksuzian1, Z. Omarov16,5, R. Osofsky36, S. Park5, G. Pauletta26,s, G. M. Piacentino25,t, R. N. Pilato30, K. T. Pitts28,u, B. Plaster29, D. Počanić35, N. Pohlman20, C. C. Polly7, J. Price30, B. Quinn34, M. U. H. Qureshi14, S. Ramachandran1,k, E. Ramberg7, R. Reimann14, B. L. Roberts2, D. L. Rubin6, L. Santi26,f, C. Schlesier28,v, A. Schreckenberger7, Y. K. Semertzidis5,16, D. Shemyakin4,a, M. Sorbara11,w, D. Stöckinger24, J. Stapleton7, D. Still7, C. Stoughton7, D. Stratakis7, H. E. Swanson36, G. Sweetmore31, D. A. Sweigart6, M. J. Syphers20, D. A. Tarazona6,30,18, T. Teubner30, A. E. Tewsley-Booth29,33, V. Tishchenko3, N. H. Tran2,x, W. Turner30, E. Valetov18, D. Vasilkova27,30, G. Venanzoni30,l, V. P. Volnykh15, T. Walton7, A. Weisskopf18, L. Welty-Rieger7, P. Winter1, Y. Wu1, B. Yu34, M. Yucel7, Y. Zeng23,22, and C. Zhang30 (The Muon g−2 Collaboration)

  • 1Argonne National Laboratory, Lemont, Illinois, USA
  • 2Boston University, Boston, Massachusetts, USA
  • 3Brookhaven National Laboratory, Upton, New York, USA
  • 4Budker Institute of Nuclear Physics, Novosibirsk, Russia
  • 5Center for Axion and Precision Physics (CAPP)/Institute for Basic Science (IBS), Daejeon, Republic of Korea
  • 6Cornell University, Ithaca, New York, USA
  • 7Fermi National Accelerator Laboratory, Batavia, Illinois, USA
  • 8INFN, Laboratori Nazionali di Frascati, Frascati, Italy
  • 9INFN, Sezione di Napoli, Naples, Italy
  • 10INFN, Sezione di Pisa, Pisa, Italy
  • 11INFN, Sezione di Roma Tor Vergata, Rome, Italy
  • 12INFN, Sezione di Trieste, Trieste, Italy
  • 13Department of Physics and Astronomy, James Madison University, Harrisonburg, Virginia, USA
  • 14Institute of Physics and Cluster of Excellence PRISMA+, Johannes Gutenberg University Mainz, Mainz, Germany
  • 15Joint Institute for Nuclear Research, Dubna, Russia
  • 16Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon, Republic of Korea
  • 17Lancaster University, Lancaster, United Kingdom
  • 18Michigan State University, East Lansing, Michigan, USA
  • 19North Central College, Naperville, Illinois, USA
  • 20Northern Illinois University, DeKalb, Illinois, USA
  • 21Regis University, Denver, Colorado, USA
  • 22School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, China
  • 23Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai, China
  • 24Institut für Kern- und Teilchenphysik, Technische Universität Dresden, Dresden, Germany
  • 25Università del Molise, Campobasso, Italy
  • 26Università di Udine, Udine, Italy
  • 27Department of Physics and Astronomy, University College London, London, United Kingdom
  • 28University of Illinois at Urbana-Champaign, Urbana, Illinois, USA
  • 29University of Kentucky, Lexington, Kentucky, USA
  • 30University of Liverpool, Liverpool, United Kingdom
  • 31Department of Physics and Astronomy, University of Manchester, Manchester, United Kingdom
  • 32Department of Physics, University of Massachusetts, Amherst, Massachusetts, USA
  • 33University of Michigan, Ann Arbor, Michigan, USA
  • 34University of Mississippi, University, Mississippi, USA
  • 35University of Virginia, Charlottesville, Virginia, USA
  • 36University of Washington, Seattle, Washington, USA

  • aAlso at Novosibirsk State University.
  • bAlso at Oak Ridge National Laboratory.
  • cAlso at The Cockcroft Institute of Accelerator Science and Technology, Daresbury, United Kingdom.
  • dDeceased.
  • eAlso at Università di Trieste, Trieste, Italy.
  • fAlso at INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy.
  • gAlso at Shanghai Key Laboratory for Particle Physics and Cosmology; also at Key Lab for Particle Physics, Astrophysics and Cosmology (MOE).
  • hAlso at Università di Pisa, Pisa, Italy.
  • iAlso at Lebedev Physical Institute and NRNU MEPhI.
  • jAlso at Istituto Nazionale di Ottica—Consiglio Nazionale delle Ricerche, Pisa, Italy.
  • kNow at Alliance University, Bangalore, India.
  • lAlso at INFN, Sezione di Pisa, Pisa, Italy.
  • mAlso at Istinye University, Istanbul, Türkiye.
  • nAlso at Università di Napoli, Naples, Italy.
  • oAlso at University of Rijeka, Rijeka, Croatia.
  • pAlso at Research Center for Graph Computing, Zhejiang Lab, Hangzhou, Zhejiang, China.
  • qAlso at Shenzhen Technology University, Shenzhen, Guangdong, China.
  • rAlso at Scuola Normale Superiore, Pisa, Italy.
  • sAlso at INFN Gruppo Collegato di Udine, Sezione di Trieste, Udine, Italy; Deceased.
  • tAlso at INFN, Sezione di Roma Tor Vergata, Rome, Italy.
  • uNow at Virginia Tech, Blacksburg, Virginia, USA.
  • vNow at Wellesley College, Wellesley, Massachusetts, USA.
  • wAlso at Università di Roma Tor Vergata, Rome, Italy.
  • xNow at Institute for Interdisciplinary Research in Science and Education (ICISE), Quy Nhon, Binh Dinh, Vietnam.

Phys. Rev. Lett. 131, 161802 – Published 17 October, 2023

DOI: https://doi.org/10.1103/PhysRevLett.131.161802

Abstract

We present a new measurement of the positive muon magnetic anomaly, aμ≡(gμ−2)/2, from the Fermilab Muon g−2 Experiment using data collected in 2019 and 2020. We have analyzed more than 4 times the number of positrons from muon decay than in our previous result from 2018 data. The systematic error is reduced by more than a factor of 2 due to better running conditions, a more stable beam, and improved knowledge of the magnetic field weighted by the muon distribution, ω˜p′, and of the anomalous precession frequency corrected for beam dynamics effects, ωa. From the ratio ωa/ω˜p′, together with precisely determined external parameters, we determine aμ=116 592 057(25)×10−11 (0.21 ppm). Combining this result with our previous result from the 2018 data, we obtain aμ(FNAL)=116 592 055(24)×10−11 (0.20 ppm). The new experimental world average is aμ(exp)=116 592 059(22)×10−11 (0.19 ppm), which represents a factor of 2 improvement in precision.

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See Also

Detailed report on the measurement of the positive muon anomalous magnetic moment to 0.20 ppm

D. P. Aguillard et al. (Muon g−2 Collaboration)
Phys. Rev. D 110, 032009 (2024)

Article Text

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