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Sensitivity of the SHiP experiment to light dark matter
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. Ind...
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Lenguaje: | eng |
Publicado: |
2020
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1007/JHEP04(2021)199 http://cds.cern.ch/record/2743145 |
_version_ | 1780968541459054592 |
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author | 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. Buscher, 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.D. 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. Gavroliv, 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, Y.U. 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. Jokovic, D. Jonker, M. Kadenko, I. Kain, V. Kaiser, B. Kamiscioglu, C. 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. Levy, 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, Y.U. 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, D. Yilmazer, A.U. Yoon, C.S. Zaytsev, Y.U. Zelenov, A. Zimmerman, J. |
author_facet | 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. Buscher, 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.D. 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. Gavroliv, 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, Y.U. 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. Jokovic, D. Jonker, M. Kadenko, I. Kain, V. Kaiser, B. Kamiscioglu, C. 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. Levy, 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, Y.U. 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, D. Yilmazer, A.U. Yoon, C.S. Zaytsev, Y.U. Zelenov, A. Zimmerman, J. |
author_sort | Ahdida, C. |
collection | CERN |
description | 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 α$_{D}$ = 0.1 and m$_{A′}$ = 3m$_{χ}$, 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 · 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.[graphic not available: see fulltext] |
id | cern-2743145 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2020 |
record_format | invenio |
spelling | cern-27431452023-10-26T07:07:41Zdoi:10.1007/JHEP04(2021)199http://cds.cern.ch/record/2743145engAhdida, 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.Buscher, 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.D.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.Gavroliv, 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, Y.U.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.Jokovic, D.Jonker, M.Kadenko, I.Kain, V.Kaiser, B.Kamiscioglu, C.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.Levy, 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, Y.U.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, VolodymyrRodin, ViktorRobbe, 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, HeinzVincke, HelmutVisone, C.Vlasik, K.Volkov, A.Voronkov, R.van Waasen, S.Wanke, R.Wertelaers, P.Williams, O.Woo, J.-K.Wurm, M.Xella, S.Yilmaz, D.Yilmazer, A.U.Yoon, C.S.Zaytsev, Y.U.Zelenov, A.Zimmerman, J.Sensitivity of the SHiP experiment to light dark matterhep-phParticle Physics - Phenomenologyhep-exParticle Physics - ExperimentDark 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 α$_{D}$ = 0.1 and m$_{A′}$ = 3m$_{χ}$, 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 · 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.[graphic not available: see fulltext]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 $2\cdot 10^{20}$ 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.arXiv:2010.11057oai:cds.cern.ch:27431452020-10-21 |
spellingShingle | hep-ph Particle Physics - Phenomenology hep-ex Particle Physics - Experiment 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. Buscher, 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.D. 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. Gavroliv, 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, Y.U. 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. Jokovic, D. Jonker, M. Kadenko, I. Kain, V. Kaiser, B. Kamiscioglu, C. 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. Levy, 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, Y.U. 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, D. Yilmazer, A.U. Yoon, C.S. Zaytsev, Y.U. Zelenov, A. Zimmerman, J. Sensitivity of the SHiP experiment to light dark matter |
title | Sensitivity of the SHiP experiment to light dark matter |
title_full | Sensitivity of the SHiP experiment to light dark matter |
title_fullStr | Sensitivity of the SHiP experiment to light dark matter |
title_full_unstemmed | Sensitivity of the SHiP experiment to light dark matter |
title_short | Sensitivity of the SHiP experiment to light dark matter |
title_sort | sensitivity of the ship experiment to light dark matter |
topic | hep-ph Particle Physics - Phenomenology hep-ex Particle Physics - Experiment |
url | https://dx.doi.org/10.1007/JHEP04(2021)199 http://cds.cern.ch/record/2743145 |
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sensitivityoftheshipexperimenttolightdarkmatter AT visonec sensitivityoftheshipexperimenttolightdarkmatter AT vlasikk sensitivityoftheshipexperimenttolightdarkmatter AT volkova sensitivityoftheshipexperimenttolightdarkmatter AT voronkovr sensitivityoftheshipexperimenttolightdarkmatter AT vanwaasens sensitivityoftheshipexperimenttolightdarkmatter AT wanker sensitivityoftheshipexperimenttolightdarkmatter AT wertelaersp sensitivityoftheshipexperimenttolightdarkmatter AT williamso sensitivityoftheshipexperimenttolightdarkmatter AT woojk sensitivityoftheshipexperimenttolightdarkmatter AT wurmm sensitivityoftheshipexperimenttolightdarkmatter AT xellas sensitivityoftheshipexperimenttolightdarkmatter AT yilmazd sensitivityoftheshipexperimenttolightdarkmatter AT yilmazerau sensitivityoftheshipexperimenttolightdarkmatter AT yooncs sensitivityoftheshipexperimenttolightdarkmatter AT zaytsevyu sensitivityoftheshipexperimenttolightdarkmatter AT zelenova sensitivityoftheshipexperimenttolightdarkmatter AT zimmermanj sensitivityoftheshipexperimenttolightdarkmatter |