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Dark Matter Search in Missing Energy Events with NA64.
Banerjee, D; Burtsev, V E; Chumakov, A G; Cooke, D; Crivelli, P; Depero, E; Dermenev, A V; Donskov, S V; Dusaev, R R; Enik, T; Charitonidis, N; Feshchenko, A; Frolov, V N; Gardikiotis, A; Gerassimov, S G; Gninenko, S N; Hösgen, M; Jeckel, M; Karneyeu, A E; Kekelidze, G; Ketzer, B; Kirpichnikov, D V; Kirsanov, M M; Konorov, I V; Kovalenko, S G; Kramarenko, V A; Kravchuk, L V; Krasnikov, N V; Kuleshov, S V; Lyubovitskij, V E; Lysan, V; Matveev, V A; Mikhailov, Yu V; Molina Bueno, L; Peshekhonov, D V; Polyakov, V A; Radics, B; Rojas, R; Rubbia, A; Samoylenko, V D; Shchukin, D; Tikhomirov, V O; Tlisova, I; Tlisov, D A; Toropin, A N; Trifonov, A Yu; Vasilishin, B I; Vasquez Arenas, G; Volkov, P V; Volkov, V Yu.
  • Banerjee D; CERN, European Organization for Nuclear Research, CH-1211 Geneva, Switzerland.
  • Burtsev VE; University of Illinois at Urbana Champaign, Urbana, 61801-3080 Illinois, USA.
  • Chumakov AG; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Cooke D; Tomsk State Pedagogical University, 634061 Tomsk, Russia.
  • Crivelli P; Department of Physics and Astronomy, University College London, Gower St., London WC1E 6BT, United Kingdom.
  • Depero E; ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland.
  • Dermenev AV; ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland.
  • Donskov SV; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Dusaev RR; State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center 'Kurchatov Institute' (IHEP), 142281 Protvino, Russia.
  • Enik T; Tomsk State Pedagogical University, 634061 Tomsk, Russia.
  • Charitonidis N; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Feshchenko A; CERN, European Organization for Nuclear Research, CH-1211 Geneva, Switzerland.
  • Frolov VN; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Gardikiotis A; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Gerassimov SG; Physics Department, University of Patras, 265 04 Patras, Greece.
  • Gninenko SN; Technische Universität München, Physik Department, 85748 Garching, Germany.
  • Hösgen M; P.N. Lebedev Physical Institute, Moscow, Russia, 119 991 Moscow, Russia.
  • Jeckel M; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Karneyeu AE; Universität Bonn, Helmholtz-Institut für Strahlen-und Kernphysik, 53115 Bonn, Germany.
  • Kekelidze G; CERN, European Organization for Nuclear Research, CH-1211 Geneva, Switzerland.
  • Ketzer B; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Kirpichnikov DV; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Kirsanov MM; Universität Bonn, Helmholtz-Institut für Strahlen-und Kernphysik, 53115 Bonn, Germany.
  • Konorov IV; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Kovalenko SG; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Kramarenko VA; Technische Universität München, Physik Department, 85748 Garching, Germany.
  • Kravchuk LV; P.N. Lebedev Physical Institute, Moscow, Russia, 119 991 Moscow, Russia.
  • Krasnikov NV; Universidad Técnica Federico Santa María, 2390123 Valparaíso, Chile.
  • Kuleshov SV; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Lyubovitskij VE; Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, 119991 Moscow, Russia.
  • Lysan V; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Matveev VA; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Mikhailov YV; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Molina Bueno L; Departamento de Ciencias Fiisicas, Universidad Andres Bello, Sazié 2212, Piso 7, Santiago, Chile.
  • Peshekhonov DV; Tomsk State Pedagogical University, 634061 Tomsk, Russia.
  • Polyakov VA; Universidad Técnica Federico Santa María, 2390123 Valparaíso, Chile.
  • Radics B; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Rojas R; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Rubbia A; Institute for Nuclear Research, 117312 Moscow, Russia.
  • Samoylenko VD; State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center 'Kurchatov Institute' (IHEP), 142281 Protvino, Russia.
  • Shchukin D; ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland.
  • Tikhomirov VO; Joint Institute for Nuclear Research, 141980 Dubna, Russia.
  • Tlisova I; State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center 'Kurchatov Institute' (IHEP), 142281 Protvino, Russia.
  • Tlisov DA; ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland.
  • Toropin AN; Universidad Técnica Federico Santa María, 2390123 Valparaíso, Chile.
  • Trifonov AY; ETH Zürich, Institute for Particle Physics and Astrophysics, CH-8093 Zürich, Switzerland.
  • Vasilishin BI; State Scientific Center of the Russian Federation Institute for High Energy Physics of National Research Center 'Kurchatov Institute' (IHEP), 142281 Protvino, Russia.
  • Vasquez Arenas G; P.N. Lebedev Physical Institute, Moscow, Russia, 119 991 Moscow, Russia.
  • Volkov PV; P.N. Lebedev Physical Institute, Moscow, Russia, 119 991 Moscow, Russia.
  • Volkov VY; Institute for Nuclear Research, 117312 Moscow, Russia.
Phys Rev Lett ; 123(12): 121801, 2019 Sep 20.
Article en En | MEDLINE | ID: mdl-31633975
ABSTRACT
A search for sub-GeV dark matter production mediated by a new vector boson A^{'}, called a dark photon, is performed by the NA64 experiment in missing energy events from 100 GeV electron interactions in an active beam dump at the CERN SPS. From the analysis of the data collected in the years 2016, 2017, and 2018 with 2.84×10^{11} electrons on target no evidence of such a process has been found. The most stringent constraints on the A^{'} mixing strength with photons and the parameter space for the scalar and fermionic dark matter in the mass range ≲0.2 GeV are derived, thus demonstrating the power of the active beam dump approach for the dark matter search.

Texto completo: 1 Banco de datos: MEDLINE Idioma: En Año: 2019 Tipo del documento: Article

Texto completo: 1 Banco de datos: MEDLINE Idioma: En Año: 2019 Tipo del documento: Article