Mostrando 7,661 - 7,680 Resultados de 8,091 Para Buscar '"Neutrino"', tiempo de consulta: 0.13s Limitar resultados
  1. 7661
    por Boulahouache, Chaouki
    Publicado 2008
    “…We study the possibility of an early discovery of first and second generation leptoquark pairs, and of right-handed W and heavy neutrinos.…”
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  2. 7662
    por Ehrich, Thies
    Publicado 2008
    “…In this channel a light charged Higgs boson is produced in ttbar decay and the final state consists of a lepton, a tau jet, 2 b jets and several neutrinos. The latter makes the reconstruction of the complete event impossible. …”
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  3. 7663
    por Stone, Sheldon
    Publicado 2011
    “…Specific topics include the CKM element |Vub|, the forward-backward asymmetry in B -> K* mu+ mu-, b-hadron fractions at the LHC, B(Bs -> mu+ mu-), first observations of several Bs and Bc decay modes, the X(4140), new b-baryons and their decays, searches for Majorana neutrinos, and Lepton Flavor Violation.…”
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  4. 7664
    “…The prospects for future high-power proton beams for producing neutrinos at CERN within the LAGUNA-LBNO study, include the design of a 2 MW High-Power Proton Synchrotron (HP-PS). …”
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  5. 7665
    por CMS Collaboration
    Publicado 2015
    “…For the standard model Higgs Boson discovery, MVA $E^{miss}_T$ played an importent role in analyses like $H \rightarrow \tau \tau$ with up to four neutrinos in the final state, where the mass resolution largely depends on the $E^{miss}_T$ resolution. …”
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  6. 7666
    por Blum, Kfir
    Publicado 2016
    “…Session 4: Interpreting IceCube’s neutrinos Session 5: Shedding light on dark matter with precision cosmology…”
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  7. 7667
    por The ATLAS collaboration
    Publicado 2016
    “…Candidate W-boson pairs are selected by identifying their leptonic decays into an electron, a muon and neutrinos. Events with reconstructed jets are not included in the candidate event sample. …”
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  8. 7668
    por Radloff, Peter Tonkin
    Publicado 2016
    “…The search focuses on scalar boson decays into tau lepton pairs, where each decays leptonically (τ → lν ν ̄) resulting in one muon, one electron and four neutrinos. No significant excess is observed and upper limits on the signal strength are determined as a function of scalar boson mass.…”
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  9. 7669
    por Santanastasio, Francesco
    Publicado 2016
    “…The document focuses on a selection of recent results from searches for heavy dijet resonances, leptoquarks, and heavy majorana neutrinos using proton-proton collision data at both $\sqrt{s}=$8 and 13 TeV. …”
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  10. 7670
    por Holzbock, Michael
    Publicado 2021
    “…These models are motivated by the hierarchy problem and for some parameters naturally explain the lightness of the standard model neutrinos. Searches for RPV SUSY signatures require dedicated signal regions and innovative techniques to estimate the challenging backgrounds. …”
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  11. 7671
    por Feligioni, Lorenzo
    Publicado 2021
    “…These models are motivated by the hierarchy problem and for some parameters naturally explain the lightness of the standard model neutrinos. Searches for RPV SUSY signatures require dedicated signal regions and innovative techniques to estimate the challenging backgrounds. …”
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  12. 7672
    por Jeamburaset, Sittha
    Publicado 2021
    “…Then, using this number and a muon decay simulation, we can calculate the total normalization of neutrinos per proton.…”
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  13. 7673
    por Jeamburaset, Sittha
    Publicado 2021
    “…Then, using this number and a muon decay simulation, we can calculate the total normalization of neutrinos per proton.…”
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  14. 7674
    por Delsart, Pierre Antoine
    Publicado 2022
    “…Jet and Missing transverse momentum (MET), used to infer the presence of high transverse momentum neutrinos or other weakly interacting neutral particles, are two of the most important quantities to reconstruct at a hadron collider. …”
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  15. 7675
    por Dash, Ganapati
    Publicado 2023
    “…The final state is considered where the Higgs boson decays to two W bosons, which subsequently decay to an electron, a muon, and a pair of neutrinos. The measured value of the integrated fiducial cross section is 86.5$\pm$9.5 fb, consistent with the standard model expectation of 82.5$\pm$4.2 fb.…”
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  16. 7676
    por Ky, N A, Long, H N, Van Soa, D
    Publicado 2000
    “…For an expected precision($\sim 4\times 10^{-10}$) of the BNL measurements the possible lower bounds on masses of the bileptons in the minimal version and in the version with right-handed neutrinos are around 940 GeV and 250 GeV, respectively.…”
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  17. 7677
    por Achard, P., Adriani, O., Aguilar-Benitez, M., Alcaraz, J., Alemanni, G., Allaby, J., Aloisio, A., Alviggi, M.G., Anderhub, H., Andreev, Valery P., Anselmo, F., Arefev, A., Azemoon, T., Aziz, T., Bagnaia, P., Bajo, A., Baksay, G., Baksay, L., Baldew, S.V., Banerjee, S., Banerjee, Sw., Barczyk, A., Barillere, R., Bartalini, P., Basile, M., Batalova, N., Battiston, R., Bay, A., Becattini, F., Becker, U., Behner, F., Bellucci, L., Berbeco, R., Berdugo, J., Berges, P., Bertucci, B., Betev, B.L., Biasini, M., Biglietti, M., Biland, A., Blaising, J.J., Blyth, S.C., Bobbink, G.J., Bohm, A., Boldizsar, L., Borgia, B., Bottai, S., Bourilkov, D., Bourquin, M., Braccini, S., Branson, J.G., Brochu, F., Burger, J.D., Burger, W.J., Cai, X.D., Capell, M., Cara Romeo, G., Carlino, G., Cartacci, A., Casaus, J., Cavallari, F., Cavallo, N., Cecchi, C., Cerrada, M., Chamizo, M., Chang, Y.H., Chemarin, M., Chen, A., Chen, G., Chen, G.M., Chen, H.F., Chen, H.S., Chiefari, G., Cifarelli, L., Cindolo, F., Clare, I., Clare, R., Coignet, G., Colino, N., Costantini, S., de la Cruz, B., Cucciarelli, S., van Dalen, J.A., de Asmundis, R., Deglon, P., Debreczeni, J., Degre, A., Dehmelt, K., Deiters, K., della Volpe, D., Delmeire, E., Denes, P., DeNotaristefani, F., De Salvo, A., Diemoz, M., Dierckxsens, M., Dionisi, C., Dittmar, M., Doria, A., Dova, M.T., Duchesneau, D., Duda, M., Echenard, B., Eline, A., El Hage, A., El Mamouni, H., Engler, A., Eppling, F.J., Extermann, P., Falagan, M.A., Falciano, S., Favara, A., Fay, J., Fedin, O., Felcini, M., Ferguson, T., Fesefeldt, H., Fiandrini, E., Field, J.H., Filthaut, F., Fisher, P.H., Fisher, W., Fisk, I., Forconi, G., Freudenreich, K., Furetta, C., Galaktionov, Iouri, Ganguli, S.N., Garcia-Abia, Pablo, Gataullin, M., Gentile, S., Giagu, S., Gong, Z.F., Grenier, Gerald Jean, Grimm, O., Gruenewald, M.W., Guida, M., van Gulik, R., Gupta, V.K., Gurtu, A., Gutay, L.J., Haas, D., Hatzifotiadou, D., Hebbeker, T., Herve, Alain, Hirschfelder, J., Hofer, H., Hohlmann, M., Holzner, G., Hou, S.R., Hu, Y., Jin, B.N., Jones, Lawrence W., de Jong, P., Josa-Mutuberria, I., Kaur, M., Kienzle-Focacci, M.N., Kim, J.K., Kirkby, Jasper, Kittel, W., Klimentov, A., Konig, A.C., Kopal, M., Koutsenko, V., Kraber, M., Kraemer, R.W., Kruger, A., Kunin, A., Ladron de Guevara, P., Laktineh, I., Landi, G., Lebeau, M., Lebedev, A., Lebrun, P., Lecomte, P., Lecoq, P., Le Coultre, P., Le Goff, J.M., Leiste, R., Levtchenko, M., Levtchenko, P., Li, C., Likhoded, S., Lin, C.H., Lin, W.T., Linde, F.L., Lista, L., Liu, Z.A., Lohmann, W., Longo, E., Lu, Y.S., Luci, C., Luminari, L., Lustermann, W., Ma, W.G., Malgeri, L., Malinin, A., Mana, C., Mans, J., Martin, J.P., Marzano, F., Mazumdar, K., McNeil, R.R., Mele, S., Merola, L., Meschini, M., Metzger, W.J., Mihul, A., Milcent, H., Mirabelli, G., Mnich, J., Mohanty, G.B., Muanza, G.S., Muijs, A.J.M., Musicar, B., Musy, M., Nagy, S., Natale, S., Napolitano, M., Nessi-Tedaldi, F., Newman, H., Nisati, A., Novak, T., Kluge, Hannelies, Ofierzynski, R., Organtini, G., Pal, I., Palomares, C., Paolucci, P., Paramatti, R., Passaleva, G., Patricelli, S., Paul, Thomas Cantzon, Pauluzzi, M., Paus, C., Pauss, F., Pedace, M., Pensotti, S., Perret-Gallix, D., Petersen, B., Piccolo, D., Pierella, F., Pioppi, M., Piroue, P.A., Pistolesi, E., Plyaskin, V., Pohl, M., Pojidaev, V., Pothier, J., Prokofev, D., Quartieri, J., Rahal-Callot, G., Rahaman, Mohammad Azizur, Raics, P., Raja, N., Ramelli, R., Rancoita, P.G., Ranieri, R., Raspereza, A., Razis, P., Ren, D., Rescigno, M., Reucroft, S., Riemann, S., Riles, Keith, Roe, B.P., Romero, L., Rosca, A., Rosemann, C., Rosenbleck, C., Rosier-Lees, S., Roth, Stefan, Rubio, J.A., Ruggiero, G., Rykaczewski, H., Sakharov, A., Saremi, S., Sarkar, S., Salicio, J., Sanchez, E., Schafer, C., Schegelsky, V., Schopper, H., Schotanus, D.J., Sciacca, C., Servoli, L., Shevchenko, S., Shivarov, N., Shoutko, V., Shumilov, E., Shvorob, A., Son, D., Souga, C., Spillantini, P., Steuer, M., Stickland, D.P., Stoyanov, B., Straessner, A., Sudhakar, K., Sultanov, G., Sun, L.Z., Sushkov, S., Suter, H., Swain, J.D., Szillasi, Z., Tang, X.W., Tarjan, P., Tauscher, L., Taylor, L., Tellili, B., Teyssier, D., Timmermans, Charles, Ting, Samuel C.C., Ting, S.M., Tonwar, S.C., Toth, J., Tully, C., Tung, K.L., Ulbricht, J., Valente, E., Van de Walle, R.T., Vasquez, R., Veszpremi, V., Vesztergombi, G., Vetlitsky, I., Vicinanza, D., Viertel, G., Villa, S., Vivargent, M., Vlachos, S., Vodopianov, I., Vogel, H., Vogt, H., Vorobev, I., Vorobyov, A.A., Wadhwa, M., Wang, Q., Wang, X.L., Wang, Z.M., Weber, M., Wilkens, H., Wynhoff, S., Xia, L., Xu, Z.Z., Yamamoto, J., Yang, B.Z., Yang, C.G., Yang, H.J., Yang, M., Yeh, S.C., Zalite, An., Zalite, Yu., Zhang, Z.P., Zhao, J., Zhu, G.Y., Zhu, R.Y., Zhuang, H.L., Zichichi, A., Zimmermann, B., Zoller, M.
    Publicado 2004
    “…The process e^+e^- --> Z gamma, where the Z boson decays into hadrons or neutrinos, is studied with data collected with the L3 detector at LEP at centre-of-mass energies from 189 GeV up to 209 GeV. …”
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  18. 7678
    “…Particular attention is paid to decay modes, production by neutrinos or antineutrinos, the analogues of K/sub 0/-K/sub 0/ mixing, and CP violation. (40 refs).…”
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  19. 7679
    por Rubakov, V.A.
    Publicado 2017
    “…On the dark matter side, we consider weakly interacting massive particles and axions/axion-like particles as cold dark matter, sterile neutrinos and gravitinos as warm dark matter. On the baryon asymmetry side, we discuss electroweak baryogenesis as a still-viable mechanism. …”
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    Enlace del recurso
  20. 7680
    por Brustein, Ram, Sherf, Yotam
    Publicado 2019
    “…We calculate the emission of gravitational waves, gravitons, photons, and neutrinos from a perturbed Schwarzschild black hole (BH). …”
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