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Improved exclusion limit for light dark matter from e+e- annihilation in NA64
Journal
Physical Review D
Date Issued
2021-11-01
Author(s)
Andreev, Yu M.
Banerjee, D.
Bernhard, J.
Bondì, M.
Burtsev, V. E.
Celentano, A.
Charitonidis, N.
Chumakov, A. G.
Cooke, D.
Crivelli, P.
Depero, E.
Dermenev, A. V.
Donskov, S. V.
Dusaev, R. R.
Enik, T.
Feshchenko, A.
Frolov, V. N.
Gardikiotis, A.
Gerassimov, S. G.
Gninenko, S. N.
Hösgen, M.
Jeckel, M.
Kachanov, V. A.
Karneyeu, A. E.
Kekelidze, G.
Ketzer, B.
Kirpichnikov, D. V.
Kirsanov, M. M.
Kolosov, V. N.
Konorov, I. V.
Kovalenko, S. G.
Kramarenko, V. A.
Kravchuk, L. V.
Krasnikov, N. V.
Kuleshov, S. V.
Lysan, V.
Marsicano, L.
Matveev, V. A.
Mikhailov, Yu V.
Molina Bueno, L.
Peshekhonov, D. V.
Polyakov, V. A.
Radics, B.
Rubbia, A.
Samoylenko, V. D.
Sieber, H.
Shchukin, D.
Tikhomirov, V. O.
Tlisova, I.
Toropin, A. N.
Trifonov, A. Yu
Ulloa, P.
Vasilishin, B. I.
Vasquez Arenas, G.
Volkov, P. V.
Volkov, V. Yu
Abstract
The current most stringent constraints for the existence of sub-GeV dark matter coupling to Standard
Model via a massive vector boson A0 were set by the NA64 experiment for the mass region
mA0 ≲ 250 MeV, by analyzing data from the interaction of 2.84 × 1011 100-GeV electrons with an active
thick target and searching for missing-energy events. In this work, by including A0 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 p
Model via a massive vector boson A0 were set by the NA64 experiment for the mass region
mA0 ≲ 250 MeV, by analyzing data from the interaction of 2.84 × 1011 100-GeV electrons with an active
thick target and searching for missing-energy events. In this work, by including A0 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 p
Subjects
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