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author Andreev, Yu.M.
Banerjee, D.
Bernhard, J.
Bondi, 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.
Lyubovitskij, V.E.
Lysan, V.
Marsicano, L.
Matveev, V.A.
Mikhailov, Yu.V.
Bueno, L. Molina
Peshekhonov, D.V.
Polyakov, V.A.
Radics, B.
Rojas, R.
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.
author_facet Andreev, Yu.M.
Banerjee, D.
Bernhard, J.
Bondi, 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.
Lyubovitskij, V.E.
Lysan, V.
Marsicano, L.
Matveev, V.A.
Mikhailov, Yu.V.
Bueno, L. Molina
Peshekhonov, D.V.
Polyakov, V.A.
Radics, B.
Rojas, R.
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.
author_sort Andreev, Yu.M.
collection CERN
description The current most stringent constraints for the existence of sub-GeV dark matter coupling to Standard Model via a massive vector boson <math display="inline"><msup><mi>A</mi><mo>′</mo></msup></math> were set by the NA64 experiment for the mass region <math display="inline"><msub><mi>m</mi><msup><mi>A</mi><mo>′</mo></msup></msub><mo>≲</mo><mn>250</mn><mtext> </mtext><mtext> </mtext><mi>MeV</mi></math>, by analyzing data from the interaction of <math display="inline"><mn>2.84</mn><mo>×</mo><msup><mn>10</mn><mn>11</mn></msup></math> 100-GeV electrons with an active thick target and searching for missing-energy events. In this work, by including <math display="inline"><msup><mi>A</mi><mo>′</mo></msup></math> 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 <math display="inline"><msup><mi>e</mi><mo>+</mo></msup></math> beam efforts.
id cern-2778372
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2021
record_format invenio
spelling cern-27783722023-10-26T07:11:58Zdoi:10.1103/PhysRevD.104.L091701http://cds.cern.ch/record/2778372engAndreev, Yu.M.Banerjee, D.Bernhard, J.Bondi, 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.Lyubovitskij, V.E.Lysan, V.Marsicano, L.Matveev, V.A.Mikhailov, Yu.V.Bueno, L. MolinaPeshekhonov, D.V.Polyakov, V.A.Radics, B.Rojas, R.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.Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64hep-phParticle Physics - Phenomenologyhep-exParticle Physics - ExperimentThe current most stringent constraints for the existence of sub-GeV dark matter coupling to Standard Model via a massive vector boson <math display="inline"><msup><mi>A</mi><mo>′</mo></msup></math> were set by the NA64 experiment for the mass region <math display="inline"><msub><mi>m</mi><msup><mi>A</mi><mo>′</mo></msup></msub><mo>≲</mo><mn>250</mn><mtext> </mtext><mtext> </mtext><mi>MeV</mi></math>, by analyzing data from the interaction of <math display="inline"><mn>2.84</mn><mo>×</mo><msup><mn>10</mn><mn>11</mn></msup></math> 100-GeV electrons with an active thick target and searching for missing-energy events. In this work, by including <math display="inline"><msup><mi>A</mi><mo>′</mo></msup></math> 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 <math display="inline"><msup><mi>e</mi><mo>+</mo></msup></math> beam efforts.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.arXiv:2108.04195CERN-EP-2021-164oai:cds.cern.ch:27783722021-08-09
spellingShingle hep-ph
Particle Physics - Phenomenology
hep-ex
Particle Physics - Experiment
Andreev, Yu.M.
Banerjee, D.
Bernhard, J.
Bondi, 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.
Lyubovitskij, V.E.
Lysan, V.
Marsicano, L.
Matveev, V.A.
Mikhailov, Yu.V.
Bueno, L. Molina
Peshekhonov, D.V.
Polyakov, V.A.
Radics, B.
Rojas, R.
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.
Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title_full Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title_fullStr Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title_full_unstemmed Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title_short Improved exclusion limit for light dark matter from $e^+e^-$ annihilation in NA64
title_sort improved exclusion limit for light dark matter from $e^+e^-$ annihilation in na64
topic hep-ph
Particle Physics - Phenomenology
hep-ex
Particle Physics - Experiment
url https://dx.doi.org/10.1103/PhysRevD.104.L091701
http://cds.cern.ch/record/2778372
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