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7661por Boulahouache, Chaouki“…We study the possibility of an early discovery of first and second generation leptoquark pairs, and of right-handed W and heavy neutrinos.…”
Publicado 2008
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7662por Ehrich, Thies“…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. …”
Publicado 2008
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7663por Stone, Sheldon“…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.…”
Publicado 2011
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7664por Papaphilippou, Y, Alabau-Gonzalvo, J, Alekou, A, Antoniou, F, Efthymiopoulos, I, Steerenberg, R“…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). …”
Publicado 2014
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7665por CMS Collaboration“…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. …”
Publicado 2015
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7666por Blum, Kfir“…Session 4: Interpreting IceCube’s neutrinos Session 5: Shedding light on dark matter with precision cosmology…”
Publicado 2016
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7667por The ATLAS collaboration“…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. …”
Publicado 2016
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7668por Radloff, Peter Tonkin“…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.…”
Publicado 2016
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7669por Santanastasio, Francesco“…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}=$8 and 13 TeV. …”
Publicado 2016
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7670por Holzbock, Michael“…These models are motivated by the hierarchy problem and for some parameters naturally explain the lightness of the standard model neutrinos. Searches for RPV SUSY signatures require dedicated signal regions and innovative techniques to estimate the challenging backgrounds. …”
Publicado 2021
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7671por Feligioni, Lorenzo“…These models are motivated by the hierarchy problem and for some parameters naturally explain the lightness of the standard model neutrinos. Searches for RPV SUSY signatures require dedicated signal regions and innovative techniques to estimate the challenging backgrounds. …”
Publicado 2021
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7672por Jeamburaset, Sittha“…Then, using this number and a muon decay simulation, we can calculate the total normalization of neutrinos per proton.…”
Publicado 2021
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7673por Jeamburaset, Sittha“…Then, using this number and a muon decay simulation, we can calculate the total normalization of neutrinos per proton.…”
Publicado 2021
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7674por Delsart, Pierre Antoine“…Jet and Missing transverse momentum (MET), used to infer the presence of high transverse momentum neutrinos or other weakly interacting neutral particles, are two of the most important quantities to reconstruct at a hadron collider. …”
Publicado 2022
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7675por Dash, Ganapati“…The final state is considered where the Higgs boson decays to two W bosons, which subsequently decay to an electron, a muon, and a pair of neutrinos. The measured value of the integrated fiducial cross section is 86.5$\pm$9.5 fb, consistent with the standard model expectation of 82.5$\pm$4.2 fb.…”
Publicado 2023
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7676“…For an expected precision($\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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7677por 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.“…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. …”
Publicado 2004
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7678por Ellis, Jonathan Richard, Gaillard, Mary Katherin, Nanopoulos, Dimitri V, Rudaz, S“…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).…”
Publicado 1977
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7679por Rubakov, V.A.“…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. …”
Publicado 2017
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7680“…We calculate the emission of gravitational waves, gravitons, photons, and neutrinos from a perturbed Schwarzschild black hole (BH). …”
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