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Article
Report number arXiv:2108.04195 ; CERN-EP-2021-164
Title Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
Author(s) Andreev, Yu.M. (Moscow, INR) ; Banerjee, D. (CERN) ; Bernhard, J. (CERN) ; Bondi, M. (INFN, Genoa) ; Burtsev, V.E. (Dubna, JINR) ; Celentano, A. (INFN, Genoa) ; Charitonidis, N. (CERN) ; Chumakov, A.G. (Tomsk Polytechnic U. ; Tomsk Pedagogical Inst.) ; Cooke, D. (U. Coll. London) ; Crivelli, P. (Zurich, ETH) ; Depero, E. (Zurich, ETH) ; Dermenev, A.V. (Moscow, INR) ; Donskov, S.V. (Kurchatov Inst., Moscow) ; Dusaev, R.R. (Tomsk Polytechnic U.) ; Enik, T. (Dubna, JINR) ; Feshchenko, A. (Dubna, JINR) ; Frolov, V.N. (Dubna, JINR) ; Gardikiotis, A. (Patras U.) ; Gerassimov, S.G. (Munich, Tech. U. ; Lebedev Inst.) ; Gninenko, S.N. (Moscow, INR) ; Hösgen, M. (Bonn U., ITKP) ; Jeckel, M. (CERN) ; Kachanov, V.A. (Kurchatov Inst., Moscow) ; Karneyeu, A.E. (Moscow, INR) ; Kekelidze, G. (Dubna, JINR) ; Ketzer, B. (Bonn U., ITKP) ; Kirpichnikov, D.V. (Moscow, INR) ; Kirsanov, M.M. (Moscow, INR) ; Kolosov, V.N. (Kurchatov Inst., Moscow) ; Konorov, I.V. (Munich, Tech. U. ; Lebedev Inst.) ; Kovalenko, S.G. (Andres Bello Natl. U. ; Millenium Inst. Astro., Santiago) ; Kramarenko, V.A. (Dubna, JINR ; SINP, Moscow) ; Kravchuk, L.V. (Moscow, INR) ; Krasnikov, N.V. (Dubna, JINR ; Moscow, INR) ; Kuleshov, S.V. (Andres Bello Natl. U. ; Millenium Inst. Astro., Santiago) ; Lyubovitskij, V.E. (Tomsk Polytechnic U. ; Tomsk Pedagogical Inst. ; Santa Maria U., Valparaiso ; Millenium Inst. Astro., Santiago) ; Lysan, V. (Dubna, JINR) ; Marsicano, L. (INFN, Genoa) ; Matveev, V.A. (Dubna, JINR) ; Mikhailov, Yu.V. (Kurchatov Inst., Moscow) ; Bueno, L. Molina (Zurich, ETH ; Valencia U., IFIC) ; Peshekhonov, D.V. (Dubna, JINR) ; Polyakov, V.A. (Kurchatov Inst., Moscow) ; Radics, B. (Zurich, ETH) ; Rojas, R. (Santa Maria U., Valparaiso) ; Rubbia, A. (Zurich, ETH) ; Samoylenko, V.D. (Kurchatov Inst., Moscow) ; Sieber, H. (Zurich, ETH) ; Shchukin, D. (Lebedev Inst.) ; Tikhomirov, V.O. (Lebedev Inst.) ; Tlisova, I. (Moscow, INR) ; Toropin, A.N. (Moscow, INR) ; Trifonov, A.Yu. (Tomsk Polytechnic U. ; Tomsk Pedagogical Inst.) ; Ulloa, P. (Andres Bello Natl. U.) ; Vasilishin, B.I. (Tomsk Polytechnic U.) ; Vasquez Arenas, G.  (Santa Maria U., Valparaiso) ; Volkov, P.V. (Dubna, JINR ; SINP, Moscow) ; Volkov, V.Yu. (SINP, Moscow)
Publication 2021-11-01
Imprint 2021-08-09
Number of pages 7
Note Version accepted for publication as a Letter in Phys. Rev. D
In: Phys. Rev. D 104 (2021) L091701
DOI 10.1103/PhysRevD.104.L091701 (publication)
Subject category hep-ph ; Particle Physics - Phenomenology ; hep-ex ; Particle Physics - Experiment
Abstract The current most stringent constraints for the existence of sub-GeV dark matter coupling to Standard Model via a massive vector boson $A^\prime$ were set by the NA64 experiment for the mass region $m_{A^\prime}\lesssim 250$ MeV, by analyzing data from the interaction of $2.84\cdot10^{11}$ 100-GeV electrons with an active thick target and searching for missing-energy events. In this work, by including $A^\prime$ production via secondary positron annihilation with atomic electrons, we extend these limits in the $200$-$300$ MeV region by almost an order of magnitude, touching for the first time the dark matter relic density constrained parameter combinations. Our new results demonstrate the power of the resonant annihilation process in missing energy dark-matter searches, paving the road to future dedicated $e^+$ beam efforts.
Copyright/License preprint: (License: arXiv nonexclusive-distrib 1.0)
publication: Published by the American Physical Society



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