Search for a light Z′ in the Lμ-Lτ scenario with the NA64-e experiment at CERN
dc.contributor.author | Andreev, Yu. M. | |
dc.contributor.author | Banerjee, D. | |
dc.contributor.author | Banto Oberhauser, B. | |
dc.contributor.author | Bernhard, J. | |
dc.contributor.author | Bisio, P. | |
dc.contributor.author | Bondí, M. | |
dc.contributor.author | Burtsev, V.E. | |
dc.contributor.author | Celentano, A. | |
dc.contributor.author | Charitonidis, N. | |
dc.contributor.author | Chumakov, A.G. | |
dc.contributor.author | Cooke, D. | |
dc.contributor.author | Crivelli, P. | |
dc.contributor.author | Depero, E. | |
dc.contributor.author | Dermenev, A.V. | |
dc.contributor.author | Donskov, S.V. | |
dc.contributor.author | Dusaev, R.R. | |
dc.contributor.author | Enik, T. | |
dc.contributor.author | Frolov, V.N. | |
dc.contributor.author | Gardikiotis, A. | |
dc.contributor.author | Gerassimov, S.G. | |
dc.contributor.author | Gninenko, S.N. | |
dc.contributor.author | Hösgen, M. | |
dc.contributor.author | Jeckel, M. | |
dc.contributor.author | Kachanov, V.A. | |
dc.contributor.author | Karneyeu, A.E. | |
dc.contributor.author | Kekelidze, G. | |
dc.contributor.author | Ketzer, B. | |
dc.contributor.author | Kirpichnikov, D.V. | |
dc.contributor.author | Kirsanov, M.M. | |
dc.contributor.author | Kolosov, V.N. | |
dc.contributor.author | Konorov, I.V. | |
dc.contributor.author | Kovalenko, S.G. | |
dc.contributor.author | Kramarenko, V.A. | |
dc.contributor.author | Kravchuk, L.V. | |
dc.contributor.author | Krasnikov, N.V. | |
dc.contributor.author | Kuleshov, S.V. | |
dc.contributor.author | Lyubovitskij, V.E. | |
dc.contributor.author | Lysan, V. | |
dc.contributor.author | Marsicano, L. | |
dc.contributor.author | Matveev, V.A. | |
dc.contributor.author | Mikhailov, Yu. V. | |
dc.contributor.author | Molina Bueno, L. | |
dc.contributor.author | Peshekhonov, D.V. | |
dc.contributor.author | Polyakov, V.A. | |
dc.contributor.author | Radics, B. | |
dc.contributor.author | Rojas, R. | |
dc.contributor.author | Rubbia, A. | |
dc.contributor.author | Salamatin, K.M. | |
dc.contributor.author | Samoylenko, V.D. | |
dc.contributor.author | Sieber, H. | |
dc.contributor.author | Shchukin, D. | |
dc.contributor.author | Tikhomirov, V.O. | |
dc.contributor.author | Tlisova, I. | |
dc.contributor.author | Toropin, A.N. | |
dc.contributor.author | Trifonov, A. Yu. | |
dc.contributor.author | Ulloa, P. | |
dc.contributor.author | Vasilishin, B.I. | |
dc.contributor.author | Vasquez Arenas, G. | |
dc.contributor.author | Volkov, P.V. | |
dc.contributor.author | Volkov, V. Yu. | |
dc.contributor.author | Voronchikhin, I. | |
dc.date.accessioned | 2023-10-30T19:11:37Z | |
dc.date.available | 2023-10-30T19:11:37Z | |
dc.date.issued | 2022-08 | |
dc.description | Indexación: Scopus. | es |
dc.description.abstract | The extension of Standard Model made by inclusion of additional U(1) gauge Lμ-Lτ symmetry can explain the difference between the measured and the predicted value of the muon magnetic moment and solve the tension in B meson decays. This model predicts the existence of a new, light Z′ vector boson, predominantly coupled to second and third generation leptons, whose interaction with electrons is due to a loop mechanism involving muons and taus. In this work, we present a rigorous evaluation of the upper limits in the Z′ parameter space, obtained from the analysis of the data collected by the NA64-e experiment at CERN SPS, that performed a search for light dark matter with 2.84×1011 electrons impinging with 100 GeV on an active thick target. The resulting limits touch the muon g-2 preferred band for values of the Z′ mass of order of 1 MeV, while the sensitivity projections for the future high-statistics NA64-e runs demonstrate the power of the electrons/positron beam approach in this theoretical scenario. © 2022 authors. Published by the American Physical Society. Published by the American Physical Society under the terms of the "https://creativecommons.org/licenses/by/4.0/"Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. Funded by SCOAP3. | es |
dc.description.uri | https://journals-aps-org.recursosbiblioteca.unab.cl/prd/abstract/10.1103/PhysRevD.106.032015 | |
dc.identifier.citation | Physical Review D, Volume 106, Issue 31, August 2022, Article number 032015 | es |
dc.identifier.doi | 10.1103/PhysRevD.106.032015 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.uri | https://repositorio.unab.cl/xmlui/handle/ria/53724 | |
dc.language.iso | en | es |
dc.publisher | American Physical Society | es |
dc.rights.license | CC BY 4.0 DEED Attribution 4.0 International | |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/deed.en | |
dc.subject | Dark Matter | es |
dc.subject | Missing Mass (Astrophysics) | es |
dc.subject | Darkness | es |
dc.title | Search for a light Z′ in the Lμ-Lτ scenario with the NA64-e experiment at CERN | es |
dc.type | Artículo | es |
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