European Physical Journal C: Particles and Fields (Oct 2021)
Probing the explanation of the muon (g-2) anomaly and thermal light dark matter with the semi-visible dark photon channel
- C. Cazzaniga,
- P. Odagiu,
- E. Depero,
- L. Molina Bueno,
- Yu. M. Andreev,
- D. Banerjee,
- J. Bernhard,
- V. E. Burtsev,
- N. Charitonidis,
- A. G. Chumakov,
- D. Cooke,
- P. Crivelli,
- A. V. Dermenev,
- S. V. Donskov,
- R. R. Dusaev,
- T. Enik,
- A. Feshchenko,
- V. N. Frolov,
- A. Gardikiotis,
- S. G. Gerassimov,
- S. Girod,
- S. N. Gninenko,
- M. Hösgen,
- V. A. Kachanov,
- A. E. Karneyeu,
- G. Kekelidze,
- B. Ketzer,
- D. V. Kirpichnikov,
- M. M. Kirsanov,
- V. N. Kolosov,
- I. V. Konorov,
- S. G. Kovalenko,
- V. A. Kramarenko,
- L. V. Kravchuk,
- N. V. Krasnikov,
- S. V. Kuleshov,
- V. E. Lyubovitskij,
- V. Lysan,
- V. A. Matveev,
- Yu. V. Mikhailov,
- D. V. Peshekhonov,
- V. A. Polyakov,
- B. Radics,
- R. Rojas,
- A. Rubbia,
- V. D. Samoylenko,
- D. Shchukin,
- H. Sieber,
- V. O. Tikhomirov,
- I. V. Tlisova,
- D. A. Tlisov,
- A. N. Toropin,
- A. Yu. Trifonov,
- B. I. Vasilishin,
- G. Vasquez Arenas,
- P. V. Volkov,
- V. Yu. Volkov,
- P. Ulloa,
- NA64 Collaboration
Affiliations
- C. Cazzaniga
- ETH Zürich Institute for Particle Physics and Astrophysics
- P. Odagiu
- ETH Zürich Institute for Particle Physics and Astrophysics
- E. Depero
- ETH Zürich Institute for Particle Physics and Astrophysics
- L. Molina Bueno
- ETH Zürich Institute for Particle Physics and Astrophysics
- Yu. M. Andreev
- Institute for Nuclear Research
- D. Banerjee
- CERN, EN-EA
- J. Bernhard
- CERN, EN-EA
- V. E. Burtsev
- Joint Institute for Nuclear Research
- N. Charitonidis
- CERN, EN-EA
- A. G. Chumakov
- Tomsk State Pedagogical University
- D. Cooke
- UCL Departement of Physics and Astronomy, University College London
- P. Crivelli
- ETH Zürich Institute for Particle Physics and Astrophysics
- A. V. Dermenev
- Institute for Nuclear Research
- S. V. Donskov
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- R. R. Dusaev
- Tomsk Polytechnic University
- T. Enik
- Joint Institute for Nuclear Research
- A. Feshchenko
- Joint Institute for Nuclear Research
- V. N. Frolov
- Joint Institute for Nuclear Research
- A. Gardikiotis
- Physics Department, University of Patras
- S. G. Gerassimov
- Physik Department, Technische Universität München
- S. Girod
- CERN, EN-EA
- S. N. Gninenko
- Institute for Nuclear Research
- M. Hösgen
- Helmholtz-Institut für Strahlen-und Kernphysik, Universität Bonn
- V. A. Kachanov
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- A. E. Karneyeu
- Institute for Nuclear Research
- G. Kekelidze
- Joint Institute for Nuclear Research
- B. Ketzer
- Helmholtz-Institut für Strahlen-und Kernphysik, Universität Bonn
- D. V. Kirpichnikov
- Institute for Nuclear Research
- M. M. Kirsanov
- Institute for Nuclear Research
- V. N. Kolosov
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- I. V. Konorov
- Physik Department, Technische Universität München
- S. G. Kovalenko
- Departamento de Ciencias Físicas, Universidad Andres Bello
- V. A. Kramarenko
- Joint Institute for Nuclear Research
- L. V. Kravchuk
- Institute for Nuclear Research
- N. V. Krasnikov
- Institute for Nuclear Research
- S. V. Kuleshov
- Departamento de Ciencias Físicas, Universidad Andres Bello
- V. E. Lyubovitskij
- Tomsk State Pedagogical University
- V. Lysan
- Joint Institute for Nuclear Research
- V. A. Matveev
- Joint Institute for Nuclear Research
- Yu. V. Mikhailov
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- D. V. Peshekhonov
- Joint Institute for Nuclear Research
- V. A. Polyakov
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- B. Radics
- ETH Zürich Institute for Particle Physics and Astrophysics
- R. Rojas
- Universidad Técnica Federico Santa María
- A. Rubbia
- ETH Zürich Institute for Particle Physics and Astrophysics
- V. D. Samoylenko
- State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center ‘Kurchatov Institute’ (IHEP)
- D. Shchukin
- P.N. Lebedev Physical Institute
- H. Sieber
- ETH Zürich Institute for Particle Physics and Astrophysics
- V. O. Tikhomirov
- P.N. Lebedev Physical Institute
- I. V. Tlisova
- Institute for Nuclear Research
- D. A. Tlisov
- Institute for Nuclear Research
- A. N. Toropin
- Institute for Nuclear Research
- A. Yu. Trifonov
- Tomsk State Pedagogical University
- B. I. Vasilishin
- Tomsk Polytechnic University
- G. Vasquez Arenas
- Universidad Técnica Federico Santa María
- P. V. Volkov
- Joint Institute for Nuclear Research
- V. Yu. Volkov
- Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University
- P. Ulloa
- Departamento de Ciencias Físicas, Universidad Andres Bello
- NA64 Collaboration
- DOI
- https://doi.org/10.1140/epjc/s10052-021-09705-5
- Journal volume & issue
-
Vol. 81,
no. 10
pp. 1 – 6
Abstract
Abstract We report the results of a search for a new vector boson ( $$ A'$$ A ′ ) decaying into two dark matter particles $$\chi _1 \chi _2$$ χ 1 χ 2 of different mass. The heavier $$\chi _2$$ χ 2 particle subsequently decays to $$\chi _1$$ χ 1 and an off-shell Dark Photon $$ A'^* \rightarrow e^+e^-$$ A ′ ∗ → e + e - . For a sufficiently large mass splitting, this model can explain in terms of new physics the recently confirmed discrepancy observed in the muon anomalous magnetic moment at Fermilab. Remarkably, it also predicts the observed yield of thermal dark matter relic abundance. A detailed Monte-Carlo simulation was used to determine the signal yield and detection efficiency for this channel in the NA64 setup. The results were obtained re-analyzing the previous NA64 searches for an invisible decay $$A'\rightarrow \chi \overline{\chi }$$ A ′ → χ χ ¯ and axion-like or pseudo-scalar particles $$a \rightarrow \gamma \gamma $$ a → γ γ . With this method, we exclude a significant portion of the parameter space justifying the muon g-2 anomaly and being compatible with the observed dark matter relic density for $$A'$$ A ′ masses from 2 $$m_e$$ m e up to 390 MeV and mixing parameter $$\varepsilon $$ ε between $$3\times 10^{-5}$$ 3 × 10 - 5 and $$2\times 10^{-2}$$ 2 × 10 - 2 .