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2961
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2962por Antypas, D., Banerjee, A., Bartram, C., Baryakhtar, M., Betz, J., Bollinger, J.J., Boutan, C., Bowring, D., Budker, D., Carney, D., Carosi, G., Chaudhuri, S., Cheong, S., Chou, A., Chowdhury, M.D., Co, R.T., Crespo López-Urrutia, J.R., Demarteau, M., DePorzio, N., Derbin, A.V., Deshpande, T., Chowdhury, M.D., Di Luzio, L., Diaz-Morcillo, A., Doyle, J.M., Drlica-Wagner, A., Droster, A., Du, N., Döbrich, B., Eby, J., Essig, R., Farren, G.S., Figueroa, N.L., Fry, J.T., Gardner, S., Geraci, A.A., Ghalsasi, A., Ghosh, S., Giannotti, M., Gimeno, B., Griffin, S.M., Grin, D., Grin, D., Grote, H., Gundlach, J.H., Guzzetti, M., Hanneke, D., Harnik, R., Henning, R., Irsic, V., Jackson, H., Kimball, D.F. Jackson, Jaeckel, J., Kagan, M., Kedar, D., Khatiwada, R., Knirck, S., Kolkowitz, S., Kovachy, T., Kuenstner, S.E., Lasner, Z., Leder, A.F., Lehnert, R., Leibrandt, D.R., Lentz, E., Lewis, S.M., Liu, Z., Manley, J., Maruyama, R.H., Millar, A.J., Muratova, V.N., Musoke, N., Nagaitsev, S., Noroozian, O., O'Hare, C.A.J., Ouellet, J.L., Pappas, K.M.W., Peik, E., Perez, G., Phipps, A., Rapidis, N.M., Robinson, J.M., Robles, V.H., Rogers, K.K., Rudolph, J., Rybka, G., Safdari, M., Safdari, M., Safronova, M.S., Salemi, C.P., Schmidt, P.O., Schumm, T., Schwartzman, A., Shu, J., Simanovskaia, M., Singh, J., Singh, S., Smith, M.S., Snow, W.M., Stadnik, Y.V., Sun, C., Sushkov, A.O., Tait, T.M.P., Takhistov, V., Tanner, D.B., Temples, D.J., Thirolf, P.G., Thomas, J.H., Tobar, M.E., Tretiak, O., Tsai, Y.-D., Tyson, J.A., Vandegar, M., Vermeulen, S., Visinelli, L., Vitagliano, E., Wang, Z., Wilson, D.J., Winslow, L., Withington, S., Wooten, M., Yang, J., Ye, J., Young, B.A., Yu, F., Zaheer, M.H., Zelevinsky, T., Zhao, Y., Zhou, K.“…The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. …”
Publicado 2022
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2963
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2964
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2965
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2966
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2967por Deepak Kumar“…Searches in CMS for dark matter in final states with invisible particles recoiling against visible states are presented. …”
Publicado 2022
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2968por Chang, Christopher“…<!--HTML-->Dark matter candidates can arise from a wide range of extensions to the Standard Model. …”
Publicado 2022
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2969por Queitsch-Maitland, Michaela“…The Forward Search Experiment (FASER) is the newest experiment at CERN’s Large Hadron Collider (LHC) and is at the forefront of the lifetime frontier in the search for dark matter and other new phenomena. It is uniquely situated around 500 m from the LHC interaction point 1 (IP1) and will be able to detect the decays of new, low mass, weakly interacting particles which are thought to act as a mediator between the particles that make up ordinary matter and a new dark sector. …”
Publicado 2022
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Enlace del recurso
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2970
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2971
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2972por Robles, Sandra“…This requires pondering all possible sources of background. Sub-GeV dark matter (DM) which annihilates into neutrinos is a potential background that has not been considered so far. …”
Publicado 2023
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2973por Dome, Tibor“…<!--HTML-->Fuzzy dark matter (FDM) modifies the internal properties of dark matter halos and large-scale cosmic environments. …”
Publicado 2023
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2974por Belfkir, Mohamed“…Collider searches for dark matter (DM) so far have mostly focussed on scenarios where DM particles are produced in association with heavy standard model (SM) particles or jets. …”
Publicado 2023
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2975por Barman, Basabendu“…In this case, the absence of a helicity suppression enhances the production of DM and baryon asymmetry, and allows a great range for the parameters including a dark matter mass below an MeV where dark matter warmness can be observable by cosmic 21-cm lines, even when gravitational interactions are responsible for reheating. …”
Publicado 2023
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2976por Wagner, Felix“…--HTML--><p><span>In the past decades, numerous experiments have emerged to unveil the nature of dark matter (DM), one of the most discussed open questions in modern particle physics. …”
Publicado 2023
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2977por Andreev, Yu.M., Banerjee, D., Oberhauser, B. Banto, Bernhard, J., Bisio, P., Celentano, A., Charitonidis, N., Chumakov, A.G., Cooke, D., Crivelli, P., Depero, E., Dermenev, A.V., Donskov, S.V., Dusaev, R.R., Enik, T., Frolov, V.N., Silva, R.B. Galleguillos, Gardikiotis, A., Gertsenberger, S.V., Girod, S., Gninenko, S.N., Hösgen, M., Kachanov, V.A., Kambar, Y., Karneyeu, A.E., Kasianova, E.A., Kekelidze, G.D., Ketzer, B., Kirpichnikov, D.V., Kirsanov, M.M., Kolosov, V.N., Kramarenko, V.A., Kravchuk, L.V., Krasnikov, N.V., Kuleshov, S.V., Lyubovitskij, V.E., Lysan, V., Marini, A., Marsicano, L., Matveev, V.A., Fredes, R. Mena, Yanssen, R.G. Mena, Bueno, L. Molina, Mongillo, M., Peshekhonov, D.V., Polyakov, V.A., Radics, B., Salamatin, K.M., Samoylenko, V.D., Sieber, H., Shchukin, D.A., Soto, O., Tikhomirov, V.O., Tlisova, I.V., Toropin, A.N., Tuzi, M., Vasilishin, B.I., Volkov, P.V., Volkov, V.Yu., Voronchikhin, I.V., Zamora-Saá, J., Zhevlakov, A.S.“…Thermal dark matter models with particle <math display="inline"><mi>χ</mi></math> masses below the electroweak scale can provide an explanation for the observed relic dark matter density. …”
Publicado 2023
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2978“…We study the formation and evolution of solitons supported by repulsive self-interactions inside extended halos, for scalar-field dark matter scenarios. We focus on the semiclassical regime where the quantum pressure is typically much smaller than the self-interactions. …”
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2979por Kramer, Peter“…Non-WIMP dark matter searches with the ATLAS detector…”
Publicado 2023
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2980por Vujinovic, Olivera“…Collider searches for dark matter (DM) so far have mostly focussed on scenarios where DM particles are produced in association with heavy standard model (SM) particles or jets. …”
Publicado 2023
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