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Sensitivity of the SHiP experiment to light dark matter
- Authors
- Ahdida, C[Ahdida, C.]; Akmete, A[Akmete, A.]; Albanese, R[Albanese, R.]; Alexandrov, A[Alexandrov, A.]; Anokhina, A[Anokhina, A.]; Aoki, S[Aoki, S.]; Arduini, G[Arduini, G.]; Atkin, E[Atkin, E.]; Azorskiy, N[Azorskiy, N.]; Back, JJ[Back, J. J.]; Bagulya, A[Bagulya, A.]; Dos Santos, FB[Baaltasar Dos Santos, F.]; Baranov, A[Baranov, A.]; Bardou, F[Bardou, F.]; Barker, GJ[Barker, G. J.]; Battistin, M[Battistin, M.]; Bauche, J[Bauche, J.]; Bay, A[Bay, A.]; Bayliss, V[Bayliss, V.]; Bencivenni, G[Bencivenni, G.]; Berdnikov, AY[Berdnikov, A. Y.]; Berdnikov, YA[Berdnikov, Y. A.]; Bertani, M[Bertani, M.]; Betancourt, C[Betancourt, C.]; Bezshyiko, I[Bezshyiko, I.]; Bezshyyko, O[Bezshyyko, O.]; Bick, D[Bick, D.]; Bieschke, S[Bieschke, S.]; Blanco, A[Blanco, A.]; Boehm, J[Boehm, J.]; Bogomilov, M[Bogomilov, M.]; Boiarska, I[Boiarska, I.]; Bondarenko, K[Bondarenko, K.]; Bonivento, WM[Bonivento, W. M.]; Borburgh, J[Borburgh, J.]; Boyarsky, A[Boyarsky, A.]; Brenner, R[Brenner, R.]; Breton, D[Breton, D.]; Buscher, V[Buscher, V.]; Buonaura, A[Buonaura, A.]; Buonocore, L[Buonocore, L.]; Buontempo, S[Buontempo, S.]; Cadeddu, S[Cadeddu, S.]; Calcaterra, A[Calcaterra, A.]; Calviani, M[Calviani, M.]; Campanelli, M[Campanelli, M.]; Casolino, M[Casolino, M.]; Charitonidis, N[Charitonidis, N.]; Chau, P[Chau, P.]; Chauveau, J[Chauveau, J.]; Chepurnov, A[Chepurnov, A.]; Chernyavskiy, M[Chernyavskiy, M.]; Choi, KY[Choi, K. -Y.]; Chumakov, A[Chumakov, A.]; Ciambrone, P[Ciambrone, P.]; Cicero, V[Cicero, V.]; Congedo, L[Congedo, L.]; Cornelis, K[Cornelis, K.]; Cristinziani, M[Cristinziani, M.]; Crupano, A[Crupano, A.]; Dallavalle, GM[Dallavalle, G. M.]; Datwyler, A[Datwyler, A.]; D'Ambrosio, N[D'Ambrosio, N.]; D'Appollonio, G[D'Appollonio, G.]; de Asmundis, R[de Asmundis, R.]; Saraiva, JD[De Carvalho Saraiva, J.]; De Lellis, G[De Lellis, G.]; de Magistris, M[de Magistris, M.]; De Roeck, A[De Roeck, A.]; De Serio, M[De Serio, M.]; De Simone, D[De Simone, D.]; Dedenko, L[Dedenko, L.]; Dergachev, P[Dergachev, P.]; Di Crescenzo, A[Di Crescenzo, A.]; Di Giulio, L[Di Giulio, L.]; Di Marco, N[Di Marco, N.]; Dib, C[Dib, C.]; Dijkstra, H[Dijkstra, H.]; Dmitrenko, V[Dmitrenko, V.]; Dougherty, LA[Dougherty, L. A.]; Dolmatov, A[Dolmatov, A.]; Domenici, D[Domenici, D.]; Donskov, S[Donskov, S.]; Drohan, V[Drohan, V.]; Dubreuil, A[Dubreuil, A.]; Durhan, O[Durhan, O.]; Ehlert, M[Ehlert, M.]; Elikkaya, E[Elikkaya, E.]; Enik, T[Enik, T.]; Etenko, A[Etenko, A.]; Fabbri, F[Fabbri, F.]; Fedin, O[Fedin, O.]; Fedotovs, F[Fedotovs, F.]; Felici, G[Felici, G.]; Ferrillo, M[Ferrillo, M.]; Ferro-Luzzi, M[Ferro-Luzzi, M.]; Filippov, K[Filippov, K.]; Fini, RA[Fini, R. A.]; Fonte, P[Fonte, P.]; Franco, C[Franco, C.]; Fraser, M[Fraser, M.]; Fresa, R[Fresa, R.]; Froeschl, R[Froeschl, R.]; Frugiuele, C[Frugiuele, C.]; Fukuda, T[Fukuda, T.]; Galati, G[Galati, G.]; Gall, J[Gall, J.]; Gatignon, L[Gatignon, L.]; Gavrilov, G[Gavrilov, G.]; Gentile, V[Gentile, V.]; Goddard, B[Goddard, B.]; Golinka-Bezshyyko, L[Golinka-Bezshyyko, L.]; Golovatiuk, A[Golovatiuk, A.]; Golovtsov, V[Golovtsov, V.]; Golubkov, D[Golubkov, D.]; Golutvin, A[Golutvin, A.]; Gorbounov, P[Gorbounov, P.]; Gorbunov, D[Gorbunov, D.]; Gorbunov, S[Gorbunov, S.]; Gorkavenko, V[Gorkavenko, V.]; Gorshenkov, M[Gorshenkov, M.]; Grachev, V[Grachev, V.]; Grandchamp, AL[Grandchamp, A. L.]; Graverini, E[Graverini, E.]; Grenard, JL[Grenard, J. -L.]; Grenier, D[Grenier, D.]; Grichine, V[Grichine, V.]; Gruzinskii, N[Gruzinskii, N.]; Guler, AM[Guler, A. M.]; Guz, Y[Guz, Yu.]; Haefeli, GJ[Haefeli, G. J.]; Hagner, C[Hagner, C.]; Hakobyan, H[Hakobyan, H.]; Harris, IW[Harris, I. W.]; van Herwijnen, E[van Herwijnen, E.]; Hessler, C[Hessler, C.]; Hollnagel, A[Hollnagel, A.]; Hosseini, B[Hosseini, B.]; Hushchyn, M[Hushchyn, M.]; Iaselli, G[Iaselli, G.]; Iuliano, A[Iuliano, A.]; Jacobsson, R[Jacobsson, R.]; Jokovic, D[Jokovic, D.]; Jonker, M[Jonker, M.]; Kadenko, I[Kadenko, I.]; Kain, V[Kain, V.]; Kaiser, B[Kaiser, B.]; Kamiscioglu, C[Kamiscioglu, C.]; Karpenkov, D[Karpenkov, D.]; Kershaw, K[Kershaw, K.]; Khabibullin, M[Khabibullin, M.]; Khalikov, E[Khalikov, E.]; Khaustov, G[Khaustov, G.]; Khoriauli, G[Khoriauli, G.]; Khotyantsev, A[Khotyantsev, A.]; Kim, YG[Kim, Y. G.]; Kim, V[Kim, V.]; Kitagawa, N[Kitagawa, N.]; Ko, JW[Ko, J. -W.]; Kodama, K[Kodama, K.]; Kolesnikov, A[Kolesnikov, A.]; Kolev, DI[Kolev, D. 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B.]; Roganova, T[Roganova, T.]; Rokujo, H[Rokujo, H.]; Rosa, G[Rosa, G.]; Rovelli, T[Rovelli, T.]; Ruchayskiy, O[Ruchayskiy, O.]; Ruf, T[Ruf, T.]; Samoylenko, V[Samoylenko, V.]; Samsonov, V[Samsonov, V.]; Galan, FS[Sanchez Galan, F.]; Diaz, PS[Santos Diaz, P.]; Ull, AS[Sanz Ull, A.]; Saputi, A[Saputi, A.]; Sato, O[Sato, O.]; Savchenko, ES[Savchenko, E. S.]; Schliwinski, JS[Schliwinski, J. S.]; Schmidt-Parzefall, W[Schmidt-Parzefall, W.]; Serra, N[Serra, N.]; Sgobba, S[Sgobba, S.]; Shadura, O[Shadura, O.]; Shakin, A[Shakin, A.]; Shaposhnikov, M[Shaposhnikov, M.]; Shatalov, P[Shatalov, P.]; Shchedrina, T[Shchedrina, T.]; Shchutska, L[Shchutska, L.]; Shevchenko, V[Shevchenko, V.]; Shibuya, H[Shibuya, H.]; Shirobokov, S[Shirobokov, S.]; Shustov, A[Shustov, A.]; Silverstein, SB[Silverstein, S. B.]; Simone, S[Simone, S.]; Simoniello, R[Simoniello, R.]; Skorokhvatov, M[Skorokhvatov, M.]; Smirnov, S[Smirnov, S.]; Sohn, JY[Sohn, J. 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- Issue Date
- 20-Apr-2021
- Publisher
- SPRINGER
- Keywords
- Beyond Standard Model; Dark matter; Fixed target experiments
- Citation
- JOURNAL OF HIGH ENERGY PHYSICS, v.2021, no.4
- Indexed
- SCIE
SCOPUS
- Journal Title
- JOURNAL OF HIGH ENERGY PHYSICS
- Volume
- 2021
- Number
- 4
- ISSN
- 1126-6708
- Abstract
- 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.
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