Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Featured in Physics
  • Open Access

First Results in the Search for Dark Sectors at NA64 with the CERN SPS High Energy Muon Beam

Yu. M. Andreev1, D. Banerjee2, B. Banto Oberhauser3, J. Bernhard2, P. Bisio4,5, N. Charitonidis2, P. Crivelli3,*, E. Depero3, A. V. Dermenev1 et al.

S. V. Donskov1, R. R. Dusaev1, T. Enik6, V. N. Frolov6, A. Gardikiotis7, S. V. Gertsenberger6, S. Girod2, S. N. Gninenko1,8, M. Hösgen9, R. Joosten10, V. A. Kachanov1, Y. Kambar6, A. E. Karneyeu1, E. A. Kasianova6, G. Kekelidze6, B. Ketzer9, D. V. Kirpichnikov1, M. M. Kirsanov1, V. N. Kolosov1, V. A. Kramarenko1,6, L. V. Kravchuk1, N. V. Krasnikov1,6, S. V. Kuleshov8,11, V. E. Lyubovitskij1,12,11, V. Lysan6, V. A. Matveev6, R. Mena Fredes11,12, R. G. Mena Yanssen11,12, L. Molina Bueno13,†, M. Mongillo3, D. V. Peshekhonov6, V. A. Polyakov1, B. Radics14, K. M. Salamatin6, V. D. Samoylenko1, D. A. Shchukin1, O. Soto15,11, H. Sieber3,‡, V. O. Tikhomirov1, I. V. Tlisova1, A. N. Toropin1, M. Tuzi13, M. B. Veit16, P. V. Volkov1,6, V. Yu. Volkov1,§, I. V. Voronchikhin1, J. Zamora-Saá8,11, and A. S. Zhevlakov6

  • 1Authors affiliated with an institute covered by a cooperation agreement with CERN
  • 2CERN, European Organization for Nuclear Research, CH-1211 Geneva, Switzerland
  • 3ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland
  • 4INFN, Sezione di Genova, 16147 Genova, Italia
  • 5Università degli Studi di Genova, 16126 Genova, Italia
  • 6Authors affiliated with an international laboratory covered by a cooperation agreement with CERN
  • 7Physics Department, University of Patras, 265 04 Patras, Greece
  • 8Center for Theoretical and Experimental Particle Physics, Facultad de Ciencias Exactas, Universidad Andres Bello, Fernandez Concha 700, Santiago, Chile
  • 9Universität Bonn, Helmholtz-Institut für Strahlen-und Kernphysik, 53115 Bonn, Germany
  • 10Rheinische Friedrich-Wilhelms-Universität, Bonn, Germany
  • 11Millennium Institute for Subatomic Physics at High-Energy Frontier (SAPHIR), Fernandez Concha 700, Santiago, Chile
  • 12Universidad Técnica Federico Santa María and CCTVal, 2390123 Valparaíso, Chile
  • 13Instituto de Fisica Corpuscular (CSIC/UV), Carrer del Catedratic Jose Beltran Martinez, 2, 46980 Paterna, Valencia, Spain
  • 14York University, Toronto, Canada
  • 15Departamento de Fisica, Facultad de Ciencias, Universidad de La Serena, Avenida Cisternas 1200, La Serena, Chile
  • 16Johannes Gutenberg Universitaet Mainz, Germany

  • *paolo.crivelli@cern.ch
  • †laura.molina.bueno@cern.ch
  • ‡henri.hugo.sieber@cern.ch
  • §Deceased.

Phys. Rev. Lett. 132, 211803 – Published 21 May, 2024

DOI: https://doi.org/10.1103/PhysRevLett.132.211803

Abstract

We report the first search for dark sectors performed at the NA64 experiment employing a high energy muon beam and a missing energy-momentum technique. Muons from the M2 beamline at the CERN Super Proton Synchrotron with a momentum of 160  GeV/c are directed to an active target. The signal signature consists of a single scattered muon with momentum <80  GeV/c in the final state, accompanied by missing energy, i.e., no detectable activity in the downstream calorimeters. For a total dataset of (1.98±0.02)×1010 muons on target, no event is observed in the expected signal region. This allows us to set new limits on the remaining (mZ′,gZ′) parameter space of a new Z′ (Lμ−Lτ) vector boson which could explain the muon (g−2)μ anomaly. Additionally, our study excludes part of the parameter space suggested by the thermal dark matter relic abundance. Our results pave the way to explore dark sectors and light dark matter with muon beams in a unique and complementary way to other experiments.

View figure in article

Physics Subject Headings (PhySH)

synopsis

Careful Accounting Could Reveal the Dark Sector

Published 21 May, 2024

An experiment at CERN seeks signs of dark matter by looking for missing energy and momentum in the debris of particle collisions.

See more in Physics

See Also

Shedding light on dark sectors with high-energy muons at the NA64 experiment at the CERN SPS

Yu. M. Andreev et al. (NA64 Collaboration)
Phys. Rev. D 110, 112015 (2024)

Article Text

References (69)

  1. S. Gninenko (NA64 Collaboration), Addendum to the Proposal P348: Search for dark sector particles weakly coupled to muon with NA64μ, Technical Reports No. CERN-SPSC-2018-024, No. SPSC-P-348-ADD-3, CERN, Geneva, 2018.
  2. J. L. Feng, Annu. Rev. Astron. Astrophys. 48, 495 (2010).
  3. N. Arkani-Hamed, D. P. Finkbeiner, T. R. Slatyer, and N. Weiner, Phys. Rev. D 79, 015014 (2009).
  4. M. Pospelov and A. Ritz, Phys. Lett. B 671, 391 (2009).
  5. D. Hooper, N. Weiner, and W. Xue, Phys. Rev. D 86, 056009 (2012).
  6. M. Pospelov, A. Ritz, and M. B. Voloshin, Phys. Lett. B 662, 53 (2008).
  7. M. Pospelov, Phys. Rev. D 80, 095002 (2009).
  8. R. Essig et al., in Community Summer Study 2013: Snowmass on the Mississippi (SLAC National Accelerator Laboratory, 2013), arXiv:1311.0029.
  9. J. L. Feng, H. Tu, and H.-B. Yu, J. Cosmol. Astropart. Phys. 10 (2008) 043.
  10. J. L. Feng and J. Kumar, Phys. Rev. Lett. 101, 231301 (2008).
  11. G. Arcadi, M. Dutra, P. Ghosh, M. Lindner, Y. Mambrini, M. Pierre, S. Profumo, and F. S. Queiroz, Eur. Phys. J. C 78, 203 (2018).
  12. N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020); 652, C4(E) (2021).
  13. J. Jaeckel, M. Lamont, and C. Vallée, Nat. Phys. 16, 393 (2020).
  14. G. Lanfranchi, M. Pospelov, and P. Schuster, Annu. Rev. Nucl. Part. Sci. 71, 279 (2021).
  15. G. Krnjaic et al., arXiv:2207.00597.
  16. C. Antel et al., Eur. Phys. J. C 83, 1122 (2023).
  17. I. Holst, D. Hooper, and G. Krnjaic, Phys. Rev. Lett. 128, 141802 (2022).
  18. J. P. Lees et al. (BABAR Collaboration, Phys. Rev. D 94, 011102 (2016).
  19. A. M. Sirunyan et al. (CMS Collaboration), Phys. Lett. B 792, 345 (2019).
  20. G. Aad et al. (ATLAS Collaboration), J. High Energy Phys. 07 (2023) 090.
  21. A. Kamada and H.-B. Yu, Phys. Rev. D 92, 113004 (2015).
  22. S. R. Mishra et al. (CCFR Collaboration), Phys. Rev. Lett. 66, 3117 (1991).
  23. D. Geiregat et al. (CHARM-II Collaboration), Phys. Lett. B 245, 271 (1990).
  24. Y. M. Andreev et al. (NA64 Collaboration), Phys. Rev. D 106, 032015 (2022).
  25. I. Adachi et al. (Belle-II Collaboration), Phys. Rev. Lett. 130, 231801 (2023).
  26. B. Ahlgren, T. Ohlsson, and S. Zhou, Phys. Rev. Lett. 111, 199001 (2013).
  27. M. Escudero, D. Hooper, G. Krnjaic, and M. Pierre, J. High Energy Phys. 03 (2019) 071.
  28. N. Sabti, J. Alvey, M. Escudero, M. Fairbairn, and D. Blas, J. Cosmol. Astropart. Phys. 01 (2020) 004.
  29. S. N. Gninenko, D. V. Kirpichnikov, M. M. Kirsanov, and N. V. Krasnikov, Phys. Lett. B 782, 406 (2018).
  30. D. V. Kirpichnikov, H. Sieber, L. M. Bueno, P. Crivelli, and M. M. Kirsanov, Phys. Rev. D 104, 076012 (2021).
  31. H. Sieber, D. V. Kirpichnikov, I. V. Voronchikhin, P. Crivelli, S. N. Gninenko, M. M. Kirsanov, N. V. Krasnikov, L. Molina-Bueno, and S. K. Sekatskii, Phys. Rev. D 108, 056018 (2023).
  32. Y. Kahn, G. Krnjaic, N. Tran, and A. Whitbeck, J. High Energy Phys. 09 (2018) 153.
  33. N. Doble, L. Gatignon, G. von Holtey, and F. Novoskoltsev, Nucl. Instrum. Methods Phys. Res., Sect. A 343, 351 (1994).
  34. H. Sieber, D. Banerjee, P. Crivelli, E. Depero, S. N. Gninenko, D. V. Kirpichnikov, M. M. Kirsanov, V. Poliakov, and L. Molina Bueno, Phys. Rev. D 105, 052006 (2022).
  35. D. Banerjee et al. (NA64 Collaboration), Phys. Rev. D 97, 072002 (2018).
  36. D. Banerjee et al., Nucl. Instrum. Methods Phys. Res., Sect. A 881, 72 (2018).
  37. S. Agostinelli et al. (GEANT4 Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 506, 250 (2003).
  38. J. Allison et al., Nucl. Instrum. Methods Phys. Res., Sect. A 835, 186 (2016).
  39. K. L. Brown, F. Rothacker, D. C. Carey, and F. C. Iselin, 10.5170/CERN-1980-004 (1983).
  40. C. Iselin, 10.5170/CERN-1974-017 (1974).
  41. K. L. Brown and F. C. Iselin, 10.5170/CERN-1974-002 (1974).
  42. L. J. Nevay et al., Comput. Phys. Commun. 252, 107200 (2020).
  43. L. J. Nevay, A. Abramov, S. T. Boogert et al., CERN Yellow Rep. Conf. Proc. 2, 45 (2020).
  44. L. J. Nevay, A. Abramov, J. Albrecht et al., in Proceedings of the 10th International Particle Accelerator Conference (2019), p. WEPTS058, 10.18429/JACoW-IPAC2019-WEPTS058.
  45. M. Bondi, A. Celentano, R. R. Dusaev, D. V. Kirpichnikov, M. M. Kirsanov, N. V. Krasnikov, L. Marsicano, and D. Shchukin, Comput. Phys. Commun. 269, 108129 (2021).
  46. B. B. Oberhauser et al., Comput. Phys. Commun. 300, 109199 (2024).
  47. J. Rauch and T. Schlüter, J. Phys. Conf. Ser. 608, 012042 (2015).
  48. T. Bilka et al., arXiv:1902.04405.
  49. W. Verkerke and D. P. Kirkby, eConf C0303241, MOLT007 (2003).
  50. Z. Wolffs, P. Bos, C. Burgard, E. Michalainas, L. Moneta, J. Rembser, and W. Verkerke, Proc. Sci. ICHEP2022 (2022) 249.
  51. L. Moneta, K. Belasco, K. S. Cranmer, S. Kreiss, A. Lazzaro, D. Piparo, G. Schott, W. Verkerke, and M. Wolf, Proc. Sci. ACAT2010 (2010) 057 [arXiv:1009.1003].
  52. G. Cowan, K. Cranmer, E. Gross, and O. Vitells, Eur. Phys. J. C 71, 1554 (2011); 73, 2501(E) (2013).
  53. D. P. Aguillard et al. (Muon g-2 Collaboration), Phys. Rev. Lett. 131, 161802 (2023).
  54. T. Aoyama et al., Phys. Rep. 887, 1 (2020).
  55. F. V. Ignatov et al. (CMD-3 Collaboration), arXiv:2302.08834.
  56. F. V. Ignatov et al. (CMD-3 Collaboration), arXiv:2309.12910.
  57. S. Borsanyi et al., Nature (London) 593, 51 (2021).
  58. R. Godang (BABAR Collaboration), EPJ Web Conf. 141, 02005 (2017).
  59. R. Capdevilla, D. Curtin, Y. Kahn, and G. Krnjaic, J. High Energy Phys. 04 (2022) 129.
  60. Y. Kaneta and T. Shimomura, Prog. Theor. Exp. Phys. 2017, 053B04 (2017).
  61. S. Gninenko and D. Gorbunov, Phys. Lett. B 823, 136739 (2021).
  62. W. Altmannshofer, S. Gori, M. Pospelov, and I. Yavin, Phys. Rev. Lett. 113, 091801 (2014).
  63. A. Berlin, N. Blinov, G. Krnjaic, P. Schuster, and N. Toro, Phys. Rev. D 99, 075001 (2019).
  64. S. N. Gninenko, D. V. Kirpichnikov, M. M. Kirsanov, and N. V. Krasnikov, Phys. Lett. B 796, 117 (2019).
  65. S. N. Gninenko, D. V. Kirpichnikov, and N. V. Krasnikov, Phys. Rev. D 100, 035003 (2019).
  66. S. Gninenko, S. Kovalenko, S. Kuleshov, V. E. Lyubovitskij, and A. S. Zhevlakov, Phys. Rev. D 98, 015007 (2018).
  67. S. N. Gninenko and N. V. Krasnikov (NA64 Collaboration), Phys. Rev. D 106, 015003 (2022).
  68. B. Radics, L. Molina-Bueno, L. Fields, H. Sieber, and P. Crivelli, Eur. Phys. J. C 83, 775 (2023).
  69. A. Ariga, R. Balkin, I. Galon, E. Kajomovitz, and Y. Soreq, Phys. Rev. D 109, 035003 (2024).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation