Sensitivity of the SHiP experiment to light dark matter

Ahdida, C.; Akmete, A.; Albanese, R.; Alexandrov, A.; Anokhina, A.; Aoki, S.; Arduini, G.; Atkin, E.; Azorskiy, N.; Back, J.J.; Bagulya, A.; Baaltasar Dos Santos, F.; Baranov, A.; Bardou, F.; Barker, G.J.; Battistin, M.; Bauche, J.; Bay, A.; Bayliss, V.; Bencivenni, G.; Berdnikov, A.Y.; Berdnikov, Y.A.; Bertani, M.; Betancourt, C.; Bezshyiko, I.; Bezshyyko, O.; Bick, D.; Bieschke, S.; Blanco, A.; Boehm, J.; Bogomilov, M.; Boiarska, I.; Bondarenko, K.; Bonivento, W.M.; Borburgh, J.; Boyarsky, A.; Brenner, R.; Breton, D.; Büscher, V.; Buonaura, A.; Buonocore, L.; Buontempo, S.; Cadeddu, S.; Calcaterra, A.; Calviani, M.; Campanelli, M.; Casolino, M.; Charitonidis, N.; Chau, P.; Chauveau, J.; Chepurnov, A.; Chernyavskiy, M.; Choi, K.-Y.; Chumakov, A.; Ciambrone, P.; Cicero, V.; Congedo, L.; Cornelis, K.; Cristinziani, M.; Crupano, A.; Dallavalle, G.M.; Datwyler, A.; D’Ambrosio, N.; D’Appollonio, G.; de Asmundis, R.; De Carvalho Saraiva, J.; De Lellis, G.; de Magistris, M.; De Roeck, A.; De Serio, M.; De Simone, D.; Dedenko, L.; Dergachev, P.; Di Crescenzo, A.; Di Giulio, L.; Di Marco, N.; Dib, C.; Dijkstra, H.; Dmitrenko, V.; Dougherty, L.A.; Dolmatov, A.; Domenici, D.; Donskov, S.; Drohan, V.; Dubreuil, A.; Durhan, O.; Ehlert, M.; Elikkaya, E.; Enik, T.; Etenko, A.; Fabbri, F.; Fedin, O.; Fedotovs, F.; Felici, G.; Ferrillo, M.; Ferro-Luzzi, M.; Filippov, K.; Fini, R.A.; Fonte, P.; Franco, C.; Fraser, M.; Fresa, R.; Froeschl, R.; Frugiuele, C.; Fukuda, T.; Galati, G.; Gall, J.; Gatignon, L.; Gavrilov, G.; Gentile, V.; Goddard, B.; Golinka-Bezshyyko, L.; Golovatiuk, A.; Golovtsov, V.; Golubkov, D.; Golutvin, A.; Gorbounov, P.; Gorbunov, D.; Gorbunov, S.; Gorkavenko, V.; Gorshenkov, M.; Grachev, V.; Grandchamp, A.L.; Graverini, E.; Grenard, J.-L.; Grenier, D.; Grichine, V.; Gruzinskii, N.; Guler, A.M.; Guz, Yu.; Haefeli, G.J.; Hagner, C.; Hakobyan, H.; Harris, I.W.; van Herwijnen, E.; Hessler, C.; Hollnagel, A.; Hosseini, B.; Hushchyn, M.; Iaselli, G.; Iuliano, A.; Jacobsson, R.; Joković, D.; Jonker, M.; Kadenko, I.; Kain, V.; Kaiser, B.; Kamiscioglu, ÇAĞIN; Karpenkov, D.; Kershaw, K.; Khabibullin, M.; Khalikov, E.; Khaustov, G.; Khoriauli, G.; Khotyantsev, A.; Kim, Y.G.; Kim, V.; Kitagawa, N.; Ko, J.-W.; Kodama, K.; Kolesnikov, A.; Kolev, D.I.; Kolosov, V.; Komatsu, M.; Kono, A.; Konovalova, N.; Kormannshaus, S.; Korol, I.; Korol’ko, I.; Korzenev, A.; Kostyukhin, V.; Koukovini Platia, E.; Kovalenko, S.; Krasilnikova, I.; Kudenko, Y.; Kurbatov, E.; Kurbatov, P.; Kurochka, V.; Kuznetsova, E.; Lacker, H.M.; Lamont, M.; Lanfranchi, G.; Lantwin, O.; Lauria, A.; Lee, K.S.; Lee, K.Y.; Lévy, J.-M.; Loschiavo, V.P.; Lopes, L.; Lopez Sola, E.; Lyubovitskij, V.; Maalmi, J.; Magnan, A.; Maleev, V.; Malinin, A.; Maltoni, F.; Manabe, Y.; Managadze, A.K.; Manfredi, M.; Marsh, S.; Marshall, A.M.; Mattelaer, O.; Mefodev, A.; Mermod, P.; Miano, A.; Mikado, S.; Mikhaylov, Yu.; Milstead, D.A.; Mineev, O.; Montanari, A.; Montesi, M.C.; Morishima, K.; Movchan, S.; Muttoni, Y.; Naganawa, N.; Nakamura, M.; Nakano, T.; Nasybulin, S.; Ninin, P.; Nishio, A.; Novikov, A.; Obinyakov, B.; Ogawa, S.; Okateva, N.; Opitz, B.; Osborne, J.; Ovchynnikov, M.; Owtscharenko, N.; Owen, P.H.; Pacholek, P.; Paoloni, A.; Park, B.D.; Pastore, A.; Patel, M.; Pereyma, D.; Perillo-Marcone, A.; Petkov, G.L.; Petridis, K.; Petrov, A.; Podgrudkov, D.; Poliakov, V.; Polukhina, N.; Prieto Prieto, J.; Prokudin, M.; Prota, A.; Quercia, A.; Rademakers, A.; Rakai, A.; Ratnikov, F.; Rawlings, T.; Redi, F.; Ricciardi, S.; Rinaldesi, M.; Rodin, Volodymyr; Rodin, Viktor; Robbe, P.; Rodrigues Cavalcante, A.B.; Roganova, T.; Rokujo, H.; Rosa, G.; Rovelli, T.; Ruchayskiy, O.; Ruf, T.; Samoylenko, V.; Samsonov, V.; Sanchez Galan, F.; Santos Diaz, P.; Sanz Ull, A.; Saputi, A.; Sato, O.; Savchenko, E.S.; Schliwinski, J.S.; Schmidt-Parzefall, W.; Serra, N.; Sgobba, S.; Shadura, O.; Shakin, A.; Shaposhnikov, M.; Shatalov, P.; Shchedrina, T.; Shchutska, L.; Shevchenko, V.; Shibuya, H.; Shirobokov, S.; Shustov, A.; Silverstein, S.B.; Simone, S.; Simoniello, R.; Skorokhvatov, M.; Smirnov, S.; Sohn, J.Y.; Sokolenko, A.; Solodko, E.; Starkov, N.; Stoel, L.; Stramaglia, M.E.; Sukhonos, D.; Suzuki, Y.; Takahashi, S.; Tastet, J.L.; Teterin, P.; Than Naing, S.; Timiryasov, I.; Tioukov, V.; Tommasini, D.; Torii, M.; Tosi, N.; Tramontano, F.; Treille, D.; Tsenov, R.; Ulin, S.; Ursov, E.; Ustyuzhanin, A.; Uteshev, Z.; Uvarov, L.; Vankova-Kirilova, G.; Vannucci, F.; Venturi, V.; Vilchinski, S.; Vincke, Heinz; Vincke, Helmut; Visone, C.; Vlasik, K.; Volkov, A.; Voronkov, R.; van Waasen, S.; Wanke, R.; Wertelaers, P.; Williams, O.; Woo, J.-K.; Wurm, M.; Xella, S.; Yilmaz, DENİZ; Yilmazer, A.U.; Yoon, C.S.; Zaytsev, Yu.; Zelenov, A.; Zimmerman, J.

doi:10.1007/jhep04(2021)199

Sensitivity of the SHiP experiment to light dark matter

Atıf İçin Kopyala

Ahdida C., Akmete A., Albanese R., Alexandrov A., Anokhina A., Aoki S., ...Daha Fazla

JOURNAL OF HIGH ENERGY PHYSICS, cilt.2021, sa.4, 2021 (SCI-Expanded)

Yayın Türü: Makale / Tam Makale
Cilt numarası: 2021 Sayı: 4
Basım Tarihi: 2021
Doi Numarası: 10.1007/jhep04(2021)199
Dergi Adı: JOURNAL OF HIGH ENERGY PHYSICS
Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, INSPEC, zbMATH, Directory of Open Access Journals
Anahtar Kelimeler: Beyond Standard Model, Dark matter, Fixed target experiments
Ankara Üniversitesi Adresli: Evet

Özet

Dark matter is a well-established theoretical addition to the Standard Model supported by many observations in modern astrophysics and cosmology. In this context, the existence of weakly interacting massive particles represents an appealing solution to the observed thermal relic in the Universe. Indeed, a large experimental campaign is ongoing for the detection of such particles in the sub-GeV mass range. Adopting the benchmark scenario for light dark matter particles produced in the decay of a dark photon, with alpha(D) = 0.1 and m(A ') = 3m(chi), we study the potential of the SHiP experiment to detect such elusive particles through its Scattering and Neutrino detector (SND). In its 5-years run, corresponding to 2 center dot 10(20) protons on target from the CERN SPS, we find that SHiP will improve the current limits in the mass range for the dark matter from about 1 MeV to 300 MeV. In particular, we show that SHiP will probe the thermal target for Majorana candidates in most of this mass window and even reach the Pseudo-Dirac thermal relic.