학술논문

Sensitivity of the SHiP experiment to dark photons decaying to a pair of charged particles
Document Type
article
Author
SHiP CollaborationC. AhdidaA. AkmeteR. AlbaneseA. AlexandrovA. AnokhinaS. AokiG. ArduiniE. AtkinN. AzorskiyJ. J. BackA. BagulyaF. Baaltasar Dos SantosA. BaranovF. BardouG. J. BarkerM. BattistinJ. BaucheA. BayV. BaylissG. BencivenniA. Y. BerdnikovY. A. BerdnikovM. BertaniC. BetancourtI. BezshyikoO. BezshyykoD. BickS. BieschkeA. BlancoJ. BoehmM. BogomilovI. BoiarskaK. BondarenkoW. M. BoniventoJ. BorburghA. BoyarskyR. BrennerD. BretonV. BüscherA. BuonauraS. BuontempoS. CadedduA. CalcaterraM. CalvianiM. CampanelliM. CasolinoN. CharitonidisP. ChauJ. ChauveauA. ChepurnovM. ChernyavskiyK.-Y. ChoiA. ChumakovP. CiambroneV. CiceroL. CongedoK. CornelisM. CristinzianiA. CrupanoG. M. DallavalleA. DatwylerN. D’AmbrosioG. D’AppollonioR. de AsmundisJ. De Carvalho SaraivaG. De LellisM. de MagistrisA. De RoeckM. De SerioD. De SimoneL. DedenkoP. DergachevA. Di CrescenzoL. Di GiulioN. Di MarcoC. DibH. DijkstraV. DmitrenkoL. A. DoughertyA. DolmatovD. DomeniciS. DonskovV. DrohanA. DubreuilO. DurhanM. EhlertE. ElikkayaT. EnikA. EtenkoF. FabbriO. FedinF. FedotovsG. FeliciM. FerrilloM. Ferro-LuzziK. FilippovR. A. FiniP. FonteC. FrancoM. FraserR. FresaR. FroeschlT. FukudaG. GalatiJ. GallL. GatignonG. GavrilovV. GentileB. GoddardL. Golinka-BezshyykoA. GolovatiukV. GolovtsovD. GolubkovA. GolutvinP. GorbounovD. GorbunovS. GorbunovV. GorkavenkoM. GorshenkovV. GrachevA. L. GrandchampE. GraveriniJ.-L. GrenardD. GrenierV. GrichineN. GruzinskiiA. M. GulerYu. GuzG. J. HaefeliC. HagnerH. HakobyanI. W. HarrisE. van HerwijnenC. HesslerA. HollnagelB. HosseiniM. HushchynG. IaselliA. IulianoR. JacobssonD. JokovićM. JonkerI. KadenkoV. KainB. KaiserC. KamisciogluD. KarpenkovK. KershawM. KhabibullinE. KhalikovG. KhaustovG. KhoriauliA. KhotyantsevY. G. KimV. KimN. KitagawaJ.-W. KoK. KodamaA. KolesnikovD. I. KolevV. KolosovM. KomatsuA. KonoN. KonovalovaS. KormannshausI. KorolI. Korol’koA. KorzenevV. KostyukhinE. Koukovini PlatiaS. KovalenkoI. KrasilnikovaY. KudenkoE. KurbatovP. KurbatovV. KurochkaE. KuznetsovaH. M. LackerM. LamontG. LanfranchiO. LantwinA. LauriaK. S. LeeK. Y. LeeN. LeonardoJ.-M. LévyV. P. LoschiavoL. LopesE. Lopez SolaV. LyubovitskijJ. MaalmiA.-M. MagnanV. MaleevA. MalininY. ManabeA. K. ManagadzeM. ManfrediS. MarshA. M. MarshallA. MefodevP. MermodA. MianoS. MikadoYu. MikhaylovD. A. MilsteadO. MineevA. MontanariM. C. MontesiK. MorishimaS. MovchanY. MuttoniN. NaganawaM. NakamuraT. NakanoS. NasybulinP. NininA. NishioB. ObinyakovS. OgawaN. OkatevaB. OpitzJ. OsborneM. OvchynnikovN. OwtscharenkoP. H. OwenP. PacholekA. PaoloniB. D. ParkA. PastoreM. PatelD. PereymaA. Perillo-MarconeG. L. PetkovK. PetridisA. PetrovD. PodgrudkovV. PoliakovN. PolukhinaJ. Prieto PrietoM. ProkudinA. ProtaA. QuerciaA. RademakersA. RakaiF. RatnikovT. RawlingsF. RediS. RicciardiM. RinaldesiVolodymyr RodinViktor RodinP. RobbeA. B. Rodrigues CavalcanteT. RoganovaH. RokujoG. RosaT. RovelliO. RuchayskiyT. RufV. SamoylenkoV. SamsonovF. Sanchez GalanP. Santos DiazA. Sanz UllA. SaputiO. SatoE. S. SavchenkoJ. S. SchliwinskiW. Schmidt-ParzefallN. SerraS. SgobbaO. ShaduraA. ShakinM. ShaposhnikovP. ShatalovT. ShchedrinaL. ShchutskaV. ShevchenkoH. ShibuyaS. ShirobokovA. ShustovS. B. SilversteinS. SimoneR. SimonielloM. SkorokhvatovS. SmirnovG. SoaresJ. Y. SohnA. SokolenkoE. SolodkoN. StarkovL. StoelM. E. StramagliaD. SukhonosY. SuzukiS. TakahashiJ. L. TastetP. TeterinS. Than NaingI. TimiryasovV. TioukovD. TommasiniM. ToriiN. TosiD. TreilleR. TsenovS. UlinE. UrsovA. UstyuzhaninZ. UteshevL. UvarovG. Vankova-KirilovaF. VannucciV. VenturiI. VidulinS. VilchinskiHeinz VinckeHelmut VinckeC. VisoneK. VlasikA. VolkovR. VoronkovS. van WaasenR. WankeP. WertelaersO. WilliamsJ.-K. WooM. WurmS. XellaD. YilmazA. U. YilmazerC. S. YoonYu. ZaytsevA. ZelenovJ. Zimmerman
Source
European Physical Journal C: Particles and Fields, Vol 81, Iss 5, Pp 1-17 (2021)
Subject
Astrophysics
QB460-466
Nuclear and particle physics. Atomic energy. Radioactivity
QC770-798
Language
English
ISSN
1434-6044
1434-6052
Abstract
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 $$_{\gamma ^{\mathrm {D}}}$$ γ D and its mixing parameter with the photon, $$\varepsilon $$ ε . The sensitivity of the SHiP detector is reviewed for dark photons in the mass range between 0.002 and 10 GeV. Different production mechanisms 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 $$_{\gamma ^{\mathrm {D}}}$$ γ D ranging between 0.8 and 3.3 $$^{+0.2}_{-0.5}$$ - 0.5 + 0.2 GeV, and $$\varepsilon ^2$$ ε 2 ranging between $$10^{-11}$$ 10 - 11 and $$10^{-17}$$ 10 - 17 .