Abstract
Dark photons are hypothetical massive vector particles that could mix with ordinary photons. The simplest theoretical model is fully characterised by only two parameters: the mass of the dark photon m(gamma)D and its mixing parameter with the photon, epsilon. The sensitivity of the SHiP detector is reviewed for dark photons in the mass range between 0.002 and 10 GeV. Different productionmechanisms are simulated, with the dark photons decaying to pairs of visible fermions, including both leptons and quarks. Exclusion contours are presented and compared with those of past experiments. The SHiP detector is expected to have a unique sensitivity for m. D ranging between 0.8 and 3.3(-0.5)(+0.2) GeV, and epsilon(2) ranging between 10(-11) and 10(-17).
| Originalsprog | Engelsk |
|---|---|
| Artikelnummer | 451 |
| Tidsskrift | European Physical Journal C |
| Vol/bind | 81 |
| Udgave nummer | 5 |
| Antal sider | 17 |
| ISSN | 1434-6044 |
| DOI | |
| Status | Udgivet - maj 2021 |
Finansiering
The SHiP Collaboration wishes to thank the Castaldo company (Naples, Italy) for their contribution to the development studies of the decay vessel. The SHiP Collaboration acknowledges support from the following funding agencies: the TAEK of Turkey with Grant number 2018TAEK(CERN)-A5.H6.F2-17; the National Research Foundation of Korea with grant numbers 2018R1A2B2007757, 2018R1D1A3B07050649, 2018R1D1A1B07050701, 2017R1D1A1B 03036042, 2017R1A6A3A01075752, 2016R1A2B4012302, and 2016R1A6A3A11930680; the Fundacao para a Ciencia e a Tecnologia of Portugal with grant number CERN/FIS-PAR/0030/2017; the Russian Foundation for Basic Research (RFBR), with Grant number 17-02-00607.
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