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2921por Terashi, Koji“…The existence of dark matter (DM) is a cornerstone of extensive search programs at colliders. …”
Publicado 2019
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2922
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2923
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2924por The ATLAS collaboration“…This is an update of a summary plot from the Exotics WG for the axial-vector $Z^{\prime}$ dark matter simplified model, using new results as of May 2020.…”
Publicado 2020
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2925
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2926por Vogt, Ramona“…Possible cold and hot matter effects on these correlations are investigated through the effects of nuclear modifications of the parton densities, enhanced $k_T$ broadening and energy loss…”
Publicado 2020
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2927“…On the scales of galaxies and beyond there is evidence for unseen dark matter. In this paper we find the experimental limits to the density of dark matter bound in the solar system by studying its effect upon planetary motion.…”
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2928
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2929
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2930
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2931“…We show how this changes if a part of neutral Dark Matter has a magnetic susceptibility. In this way, by studying Dark Matter one can obtain information about the properties of primordial magnetic fields, even if the latter have a comoving amplitude $B_0 \lesssim0.01~\mbox{nG}$. …”
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2932por 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.“…Dark matter is a well-established theoretical addition to the Standard Model supported by many observations in modern astrophysics and cosmology. …”
Publicado 2020
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2933por Yao, Xiaojun“…The construction can be easily generalized to the interaction between quarkonium and cold nuclear matter, which is of much relevance for quarkonium production in eA collisions, to be carried out in the future Electron Ion Collider.…”
Publicado 2021
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2934por Lushozi, Mawande“…We confirm that the struck nucleus is compressed by a factor proportional to the saturation momentum of the projectile and that the dynamics of the early times of the collision are best described by two separate fluids as the produced radiation’s velocity distribution is very different to the velocity distribution of the matter in the struck nucleus. [1]: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.101.054012 [2]: https://arxiv.org/pdf/2009.05680.pdf…”
Publicado 2021
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2935por Freegard, Arran Charles“…--HTML-->While overwhelming cosmological evidences point to the existence of Dark Matter (DM), only its gravitational interaction has been experimentally confirmed. …”
Publicado 2021
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2936
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2937
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2938“…In these proceedings, we present a study of a combined singlet--doublet fermion and triplet scalar model for dark matter (DM). Together, these models form a simple extension of the Standard Model (SM) that can account for DM and explain the existence of neutrino masses, which are generated radiatively. …”
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2939por Keeton, Charles“…A Ray of Light in a Sea of Dark Matter offers readers an accessible explanation of how astronomers probe dark matter. …”
Publicado 2014
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2940