A novel mechanism to produce and detect light dark matter in experiments making use of GeV electrons (and positrons) impinging on a thick target (beam dump) is proposed. The positron-rich environment produced by the electromagnetic shower allows us to produce an A′ via nonresonant (e++e-→γ+A′) and resonant (e++e-→A′) annihilation on atomic electrons. The latter mechanism, for some selected kinematics, results in a larger sensitivity with respect to limits derived by the commonly used A′-strahlung. This idea, applied to beam-dump experiments and active beam-dump experiments, pushes down the current limits by an order of magnitude.

Novel Way to Search for Light Dark Matter in Lepton Beam-Dump Experiments / Marsicano, L.; Battaglieri, M.; Bondí, M.; Carvajal, C. D. R.; Celentano, A.; De Napoli, M.; De Vita, R.; Nardi, E.; Raggi, M.; Valente, P.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 121:4(2018). [10.1103/PhysRevLett.121.041802]

Novel Way to Search for Light Dark Matter in Lepton Beam-Dump Experiments

Raggi, M.;
2018

Abstract

A novel mechanism to produce and detect light dark matter in experiments making use of GeV electrons (and positrons) impinging on a thick target (beam dump) is proposed. The positron-rich environment produced by the electromagnetic shower allows us to produce an A′ via nonresonant (e++e-→γ+A′) and resonant (e++e-→A′) annihilation on atomic electrons. The latter mechanism, for some selected kinematics, results in a larger sensitivity with respect to limits derived by the commonly used A′-strahlung. This idea, applied to beam-dump experiments and active beam-dump experiments, pushes down the current limits by an order of magnitude.
2018
Physics and Astronomy (all)
01 Pubblicazione su rivista::01a Articolo in rivista
Novel Way to Search for Light Dark Matter in Lepton Beam-Dump Experiments / Marsicano, L.; Battaglieri, M.; Bondí, M.; Carvajal, C. D. R.; Celentano, A.; De Napoli, M.; De Vita, R.; Nardi, E.; Raggi, M.; Valente, P.. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 121:4(2018). [10.1103/PhysRevLett.121.041802]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1134542
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